Search | arXiv e-print repository

<!DOCTYPE html> <html lang="en"> <head> <meta charset="utf-8"/> <meta name="viewport" content="width=device-width, initial-scale=1"/>  <link rel="apple-touch-icon" sizes="180x180" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/apple-touch-icon.png"> <link rel="icon" type="image/png" sizes="32x32" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/favicon-32x32.png"> <link rel="icon" type="image/png" sizes="16x16" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/favicon-16x16.png"> <link rel="manifest" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/site.webmanifest"> <link rel="mask-icon" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/safari-pinned-tab.svg" color="#b31b1b"> <link rel="shortcut icon" href="https://static.arxiv.org/static/base/1.0.0a5/images/icons/favicon.ico"> <meta name="msapplication-TileColor" content="#b31b1b"> <meta name="msapplication-config" content="images/icons/browserconfig.xml"> <meta name="theme-color" content="#b31b1b">  <title>Search | arXiv e-print repository</title> <script defer src="https://static.arxiv.org/static/base/1.0.0a5/fontawesome-free-5.11.2-web/js/all.js"></script> <link rel="stylesheet" href="https://static.arxiv.org/static/base/1.0.0a5/css/arxivstyle.css" /> <script type="text/x-mathjax-config"> MathJax.Hub.Config({ messageStyle: "none", extensions: ["tex2jax.js"], jax: ["input/TeX", "output/HTML-CSS"], tex2jax: { inlineMath: [ ['$','$'], ["\$","\$"] ], displayMath: [ ['$$','$$'], ["\\[","\\]"] ], processEscapes: true, ignoreClass: '.*', processClass: 'mathjax.*' }, TeX: { extensions: ["AMSmath.js", "AMSsymbols.js", "noErrors.js"], noErrors: { inlineDelimiters: ["$","$"], multiLine: false, style: { "font-size": "normal", "border": "" } } }, "HTML-CSS": { availableFonts: ["TeX"] } }); </script> <script src='//static.arxiv.org/MathJax-2.7.3/MathJax.js'></script> <script src="https://static.arxiv.org/static/base/1.0.0a5/js/notification.js"></script> <link rel="stylesheet" href="https://static.arxiv.org/static/search/0.5.6/css/bulma-tooltip.min.css" /> <link rel="stylesheet" href="https://static.arxiv.org/static/search/0.5.6/css/search.css" /> <script src="https://code.jquery.com/jquery-3.2.1.slim.min.js" integrity="sha256-k2WSCIexGzOj3Euiig+TlR8gA0EmPjuc79OEeY5L45g=" crossorigin="anonymous"></script> <script src="https://static.arxiv.org/static/search/0.5.6/js/fieldset.js"></script> <style> radio#cf-customfield_11400 { display: none; } </style> </head> <body> <header><a href="#main-container" class="is-sr-only">Skip to main content</a>  <div class="attribution level is-marginless" role="banner"> <div class="level-left"> <a class="level-item" href="https://cornell.edu/"><img src="https://static.arxiv.org/static/base/1.0.0a5/images/cornell-reduced-white-SMALL.svg" alt="Cornell University" width="200" aria-label="logo" /></a> </div> <div class="level-right is-marginless"><p class="sponsors level-item is-marginless"><span id="support-ack-url">We gratefully acknowledge support from<br /> the Simons Foundation, <a href="https://info.arxiv.org/about/ourmembers.html">member institutions</a>, and all contributors. <a href="https://info.arxiv.org/about/donate.html">Donate</a></span></p></div> </div>  <div class="identity level is-marginless"> <div class="level-left"> <div class="level-item"> <a class="arxiv" href="https://arxiv.org/" aria-label="arxiv-logo"> <img src="https://static.arxiv.org/static/base/1.0.0a5/images/arxiv-logo-one-color-white.svg" aria-label="logo" alt="arxiv logo" width="85" style="width:85px;"/> </a> </div> </div> <div class="search-block level-right"> <form class="level-item mini-search" method="GET" action="https://arxiv.org/search"> <div class="field has-addons"> <div class="control"> <input class="input is-small" type="text" name="query" placeholder="Search..." aria-label="Search term or terms" /> <p class="help"><a href="https://info.arxiv.org/help">Help</a> | <a href="https://arxiv.org/search/advanced">Advanced Search</a></p> </div> <div class="control"> <div class="select is-small"> <select name="searchtype" aria-label="Field to search"> <option value="all" selected="selected">All fields</option> <option value="title">Title</option> <option value="author">Author</option> <option value="abstract">Abstract</option> <option value="comments">Comments</option> <option value="journal_ref">Journal reference</option> <option value="acm_class">ACM classification</option> <option value="msc_class">MSC classification</option> <option value="report_num">Report number</option> <option value="paper_id">arXiv identifier</option> <option value="doi">DOI</option> <option value="orcid">ORCID</option> <option value="author_id">arXiv author ID</option> <option value="help">Help pages</option> <option value="full_text">Full text</option> </select> </div> </div> <input type="hidden" name="source" value="header"> <button class="button is-small is-cul-darker">Search</button> </div> </form> </div> </div>  <div class="container"> <div class="user-tools is-size-7 has-text-right has-text-weight-bold" role="navigation" aria-label="User menu"> <a href="https://arxiv.org/login">Login</a> </div> </div> </header> <main class="container" id="main-container"> <div class="level is-marginless"> <div class="level-left"> <h1 class="title is-clearfix"> Showing 1–33 of 33 results for author: <span class="mathjax">Anghinolfi, M</span> </h1> </div> <div class="level-right is-hidden-mobile">  <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 2020-02-24</a>  </span> </div> </div> <div class="content"> <form method="GET" action="/search/hep-ex" aria-role="search"> Searching in archive <strong>hep-ex</strong>. <a href="/search/?searchtype=author&query=Anghinolfi%2C+M">Search in all archives.</a> <div class="field has-addons-tablet"> <div class="control is-expanded"> <label for="query" class="hidden-label">Search term or terms</label> <input class="input is-medium" id="query" name="query" placeholder="Search term..." type="text" value="Anghinolfi, M"> </div> <div class="select control is-medium"> <label class="is-hidden" for="searchtype">Field</label> <select class="is-medium" id="searchtype" name="searchtype"><option value="all">All fields</option><option value="title">Title</option><option selected value="author">Author(s)</option><option value="abstract">Abstract</option><option value="comments">Comments</option><option value="journal_ref">Journal reference</option><option value="acm_class">ACM classification</option><option value="msc_class">MSC classification</option><option value="report_num">Report number</option><option value="paper_id">arXiv identifier</option><option value="doi">DOI</option><option value="orcid">ORCID</option><option value="license">License (URI)</option><option value="author_id">arXiv author ID</option><option value="help">Help pages</option><option value="full_text">Full text</option></select> </div> <div class="control"> <button class="button is-link is-medium">Search</button> </div> </div> <div class="field"> <div class="control is-size-7"> <label class="radio"> <input checked id="abstracts-0" name="abstracts" type="radio" value="show"> Show abstracts </label> <label class="radio"> <input id="abstracts-1" name="abstracts" type="radio" value="hide"> Hide abstracts </label> </div> </div> <div class="is-clearfix" style="height: 2.5em"> <div class="is-pulled-right"> <a href="/search/advanced?terms-0-term=Anghinolfi%2C+M&terms-0-field=author&size=50&order=-announced_date_first">Advanced Search</a> </div> </div> <input type="hidden" name="order" value="-announced_date_first"> <input type="hidden" name="size" value="50"> </form> <div class="level breathe-horizontal"> <div class="level-left"> <form method="GET" action="/search/"> <div style="display: none;"> <select id="searchtype" name="searchtype"><option value="all">All fields</option><option value="title">Title</option><option selected value="author">Author(s)</option><option value="abstract">Abstract</option><option value="comments">Comments</option><option value="journal_ref">Journal reference</option><option value="acm_class">ACM classification</option><option value="msc_class">MSC classification</option><option value="report_num">Report number</option><option value="paper_id">arXiv identifier</option><option value="doi">DOI</option><option value="orcid">ORCID</option><option value="license">License (URI)</option><option value="author_id">arXiv author ID</option><option value="help">Help pages</option><option value="full_text">Full text</option></select> <input id="query" name="query" type="text" value="Anghinolfi, M"> <ul id="abstracts"><li><input checked id="abstracts-0" name="abstracts" type="radio" value="show"> <label for="abstracts-0">Show abstracts</label></li><li><input id="abstracts-1" name="abstracts" type="radio" value="hide"> <label for="abstracts-1">Hide abstracts</label></li></ul> </div> <div class="box field is-grouped is-grouped-multiline level-item"> <div class="control"> <span class="select is-small"> <select id="size" name="size"><option value="25">25</option><option selected value="50">50</option><option value="100">100</option><option value="200">200</option></select> </span> <label for="size">results per page</label>. </div> <div class="control"> <label for="order">Sort results by</label> <span class="select is-small"> <select id="order" name="order"><option selected value="-announced_date_first">Announcement date (newest first)</option><option value="announced_date_first">Announcement date (oldest first)</option><option value="-submitted_date">Submission date (newest first)</option><option value="submitted_date">Submission date (oldest first)</option><option value="">Relevance</option></select> </span> </div> <div class="control"> <button class="button is-small is-link">Go</button> </div> </div> </form> </div> </div> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2302.02717">arXiv:2302.02717</a> <span> [<a href="https://arxiv.org/pdf/2302.02717">pdf</a>, <a href="https://arxiv.org/format/2302.02717">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1007/JHEP04(2023)090">10.1007/JHEP04(2023)090 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Probing invisible neutrino decay with KM3NeT-ORCA </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=KM3NeT+Collaboration"> KM3NeT Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Aiello%2C+S">S. Aiello</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Garre%2C+S+A">S. Alves Garre</a>, <a href="/search/hep-ex?searchtype=author&query=Aly%2C+Z">Z. Aly</a>, <a href="/search/hep-ex?searchtype=author&query=Ambrosone%2C+A">A. Ambrosone</a>, <a href="/search/hep-ex?searchtype=author&query=Ameli%2C+F">F. Ameli</a>, <a href="/search/hep-ex?searchtype=author&query=Andre%2C+M">M. Andre</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anguita%2C+M">M. Anguita</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+S">S. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Bagatelas%2C+C">C. Bagatelas</a>, <a href="/search/hep-ex?searchtype=author&query=Bailly-Salins%2C+L">L. Bailly-Salins</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Pree%2C+S+B+d">S. Basegmez du Pree</a>, <a href="/search/hep-ex?searchtype=author&query=Becherini%2C+Y">Y. Becherini</a>, <a href="/search/hep-ex?searchtype=author&query=Bendahman%2C+M">M. Bendahman</a>, <a href="/search/hep-ex?searchtype=author&query=Benfenati%2C+F">F. Benfenati</a>, <a href="/search/hep-ex?searchtype=author&query=Berbee%2C+E">E. Berbee</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Boettcher%2C+M">M. Boettcher</a>, <a href="/search/hep-ex?searchtype=author&query=Cabo%2C+M+B">M. Bou Cabo</a> , et al. (230 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2302.02717v3-abstract-short" style="display: inline;"> In the era of precision measurements of the neutrino oscillation parameters, upcoming neutrino experiments will also be sensitive to physics beyond the Standard Model. KM3NeT/ORCA is a neutrino detector optimised for measuring atmospheric neutrinos from a few GeV to around 100 GeV. In this paper, the sensitivity of the KM3NeT/ORCA detector to neutrino decay has been explored. A three-flavour neutr… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2302.02717v3-abstract-full').style.display = 'inline'; document.getElementById('2302.02717v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2302.02717v3-abstract-full" style="display: none;"> In the era of precision measurements of the neutrino oscillation parameters, upcoming neutrino experiments will also be sensitive to physics beyond the Standard Model. KM3NeT/ORCA is a neutrino detector optimised for measuring atmospheric neutrinos from a few GeV to around 100 GeV. In this paper, the sensitivity of the KM3NeT/ORCA detector to neutrino decay has been explored. A three-flavour neutrino oscillation scenario, where the third neutrino mass state $谓_3$ decays into an invisible state, e.g. a sterile neutrino, is considered. We find that KM3NeT/ORCA would be sensitive to invisible neutrino decays with $1/伪_3=蟿_3/m_3 < 180$~$\mathrm{ps/eV}$ at $90\%$ confidence level, assuming true normal ordering. Finally, the impact of neutrino decay on the precision of KM3NeT/ORCA measurements for $胃_{23}$, $螖m^2_{31}$ and mass ordering have been studied. No significant effect of neutrino decay on the sensitivity to these measurements has been found. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2302.02717v3-abstract-full').style.display = 'none'; document.getElementById('2302.02717v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 27 March, 2023; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 6 February, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2023. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">27 pages, 14 figures, bibliography updated, typos corrected</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2112.14517">arXiv:2112.14517</a> <span> [<a href="https://arxiv.org/pdf/2112.14517">pdf</a>, <a href="https://arxiv.org/format/2112.14517">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Search for non-standard neutrino interactions with 10 years of ANTARES data </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Alves%2C+S">S. Alves</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+S">S. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Belhorma%2C+B">B. Belhorma</a>, <a href="/search/hep-ex?searchtype=author&query=Bendahman%2C+M">M. Bendahman</a>, <a href="/search/hep-ex?searchtype=author&query=Benfenati%2C+F">F. Benfenati</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bissinger%2C+M">M. Bissinger</a>, <a href="/search/hep-ex?searchtype=author&query=Boumaaza%2C+J">J. Boumaaza</a>, <a href="/search/hep-ex?searchtype=author&query=Bouta%2C+M">M. Bouta</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Br%C3%A2nzas%2C+H">H. Br芒nzas</a>, <a href="/search/hep-ex?searchtype=author&query=Bruijn%2C+R">R. Bruijn</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Caiffi%2C+B">B. Caiffi</a> , et al. (123 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2112.14517v2-abstract-short" style="display: inline;"> Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neu… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2112.14517v2-abstract-full').style.display = 'inline'; document.getElementById('2112.14517v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2112.14517v2-abstract-full" style="display: none;"> Non-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from $\sim$16 GeV to $100$ GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients $\varepsilon_{渭蟿}$ and $\varepsilon_{蟿蟿} - \varepsilon_{渭渭}$ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7$蟽$ away from the null result. However, the 68% and 95% confidence level intervals for $\varepsilon_{渭蟿}$ and $\varepsilon_{蟿蟿} - \varepsilon_{渭渭}$, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on $\varepsilon_{渭蟿}$ is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the $渭- 蟿$ sector. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2112.14517v2-abstract-full').style.display = 'none'; document.getElementById('2112.14517v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 2 June, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 29 December, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2021. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">22 pages, 4 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2108.06293">arXiv:2108.06293</a> <span> [<a href="https://arxiv.org/pdf/2108.06293">pdf</a>, <a href="https://arxiv.org/format/2108.06293">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1007/JHEP03(2022)055">10.1007/JHEP03(2022)055 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Combined sensitivity of JUNO and KM3NeT/ORCA to the neutrino mass ordering </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=KM3NeT+Collaboration"> KM3NeT Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Aiello%2C+S">S. Aiello</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Alshamsi%2C+M">M. Alshamsi</a>, <a href="/search/hep-ex?searchtype=author&query=Garre%2C+S+A">S. Alves Garre</a>, <a href="/search/hep-ex?searchtype=author&query=Aly%2C+Z">Z. Aly</a>, <a href="/search/hep-ex?searchtype=author&query=Ambrosone%2C+A">A. Ambrosone</a>, <a href="/search/hep-ex?searchtype=author&query=Ameli%2C+F">F. Ameli</a>, <a href="/search/hep-ex?searchtype=author&query=Andre%2C+M">M. Andre</a>, <a href="/search/hep-ex?searchtype=author&query=Androulakis%2C+G">G. Androulakis</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anguita%2C+M">M. Anguita</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+S">S. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Bagatelas%2C+C">C. Bagatelas</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Pree%2C+S+B+d">S. Basegmez du Pree</a>, <a href="/search/hep-ex?searchtype=author&query=Bendahman%2C+M">M. Bendahman</a>, <a href="/search/hep-ex?searchtype=author&query=Benfenati%2C+F">F. Benfenati</a>, <a href="/search/hep-ex?searchtype=author&query=Berbee%2C+E">E. Berbee</a>, <a href="/search/hep-ex?searchtype=author&query=Berg%2C+A+M+v+d">A. M. van den Berg</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Boettcher%2C+M">M. Boettcher</a> , et al. (253 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2108.06293v1-abstract-short" style="display: inline;"> This article presents the potential of a combined analysis of the JUNO and KM3NeT/ORCA experiments to determine the neutrino mass ordering. This combination is particularly interesting as it significantly boosts the potential of either detector, beyond simply adding their neutrino mass ordering sensitivities, by removing a degeneracy in the determination of $螖m_{31}^2$ between the two experiments… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2108.06293v1-abstract-full').style.display = 'inline'; document.getElementById('2108.06293v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2108.06293v1-abstract-full" style="display: none;"> This article presents the potential of a combined analysis of the JUNO and KM3NeT/ORCA experiments to determine the neutrino mass ordering. This combination is particularly interesting as it significantly boosts the potential of either detector, beyond simply adding their neutrino mass ordering sensitivities, by removing a degeneracy in the determination of $螖m_{31}^2$ between the two experiments when assuming the wrong ordering. The study is based on the latest projected performances for JUNO, and on simulation tools using a full Monte Carlo approach to the KM3NeT/ORCA response with a careful assessment of its energy systematics. From this analysis, a $5蟽$ determination of the neutrino mass ordering is expected after 6 years of joint data taking for any value of the oscillation parameters. This sensitivity would be achieved after only 2 years of joint data taking assuming the current global best-fit values for those parameters for normal ordering. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2108.06293v1-abstract-full').style.display = 'none'; document.getElementById('2108.06293v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 13 August, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2021. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">24 pages, 9 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JHEP 03 (2022) 055 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2107.00344">arXiv:2107.00344</a> <span> [<a href="https://arxiv.org/pdf/2107.00344">pdf</a>, <a href="https://arxiv.org/format/2107.00344">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Aiello%2C+S">S. Aiello</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Alshamsi%2C+M">M. Alshamsi</a>, <a href="/search/hep-ex?searchtype=author&query=Garre%2C+S+A">S. Alves Garre</a>, <a href="/search/hep-ex?searchtype=author&query=Aly%2C+Z">Z. Aly</a>, <a href="/search/hep-ex?searchtype=author&query=Ambrosone%2C+A">A. Ambrosone</a>, <a href="/search/hep-ex?searchtype=author&query=Ameli%2C+F">F. Ameli</a>, <a href="/search/hep-ex?searchtype=author&query=Andre%2C+M">M. Andre</a>, <a href="/search/hep-ex?searchtype=author&query=Androulakis%2C+G">G. Androulakis</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anguita%2C+M">M. Anguita</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+S">S. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Bagatelas%2C+C">C. Bagatelas</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Pree%2C+S+B+d">S. Basegmez du Pree</a>, <a href="/search/hep-ex?searchtype=author&query=Bendahman%2C+M">M. Bendahman</a>, <a href="/search/hep-ex?searchtype=author&query=Benfenati%2C+F">F. Benfenati</a>, <a href="/search/hep-ex?searchtype=author&query=Berbee%2C+E">E. Berbee</a>, <a href="/search/hep-ex?searchtype=author&query=Berg%2C+A+M+v+d">A. M. van den Berg</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bissinger%2C+M">M. Bissinger</a> , et al. (223 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2107.00344v2-abstract-short" style="display: inline;"> KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile mixing angles $胃_{14}$, $胃_{24}$, $胃_{34}$ and the effective angle $胃_{渭e}$, over a broad range of… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2107.00344v2-abstract-full').style.display = 'inline'; document.getElementById('2107.00344v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2107.00344v2-abstract-full" style="display: none;"> KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile mixing angles $胃_{14}$, $胃_{24}$, $胃_{34}$ and the effective angle $胃_{渭e}$, over a broad range of mass squared difference $螖m^2_{41} \sim [10^{-5}, 10]$ $\rm{eV}^2$, allowing to test the eV-mass sterile neutrino hypothesis as the origin of short baseline anomalies, as well as probing the hypothesis of a very light sterile neutrino, not yet constrained by cosmology. ORCA will be able to explore a relevant fraction of the parameter space not yet reached by present measurements. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2107.00344v2-abstract-full').style.display = 'none'; document.getElementById('2107.00344v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 23 November, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 1 July, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2021. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2103.09885">arXiv:2103.09885</a> <span> [<a href="https://arxiv.org/pdf/2103.09885">pdf</a>, <a href="https://arxiv.org/format/2103.09885">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-021-09893-0">10.1140/epjc/s10052-021-09893-0 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Determining the Neutrino Mass Ordering and Oscillation Parameters with KM3NeT/ORCA </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Aiello%2C+S">S. Aiello</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Garre%2C+S+A">S. Alves Garre</a>, <a href="/search/hep-ex?searchtype=author&query=Aly%2C+Z">Z. Aly</a>, <a href="/search/hep-ex?searchtype=author&query=Ambrosone%2C+A">A. Ambrosone</a>, <a href="/search/hep-ex?searchtype=author&query=Ameli%2C+F">F. Ameli</a>, <a href="/search/hep-ex?searchtype=author&query=Andre%2C+M">M. Andre</a>, <a href="/search/hep-ex?searchtype=author&query=Androulakis%2C+G">G. Androulakis</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anguita%2C+M">M. Anguita</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+S">S. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Bagatelas%2C+C">C. Bagatelas</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Pree%2C+S+B+d">S. Basegmez du Pree</a>, <a href="/search/hep-ex?searchtype=author&query=Bendahman%2C+M">M. Bendahman</a>, <a href="/search/hep-ex?searchtype=author&query=Benfenati%2C+F">F. Benfenati</a>, <a href="/search/hep-ex?searchtype=author&query=Berbee%2C+E">E. Berbee</a>, <a href="/search/hep-ex?searchtype=author&query=Berg%2C+A+M+v+d">A. M. van den Berg</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bissinger%2C+M">M. Bissinger</a>, <a href="/search/hep-ex?searchtype=author&query=Boettcher%2C+M">M. Boettcher</a> , et al. (217 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2103.09885v2-abstract-short" style="display: inline;"> The next generation of water Cherenkov neutrino telescopes in the Mediterranean Sea are under construction offshore France (KM3NeT/ORCA) and Sicily (KM3NeT/ARCA). The KM3NeT/ORCA detector features an energy detection threshold which allows to collect atmospheric neutrinos to study flavour oscillation. This paper reports the KM3NeT/ORCA sensitivity to this phenomenon. The event reconstruction, sele… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2103.09885v2-abstract-full').style.display = 'inline'; document.getElementById('2103.09885v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2103.09885v2-abstract-full" style="display: none;"> The next generation of water Cherenkov neutrino telescopes in the Mediterranean Sea are under construction offshore France (KM3NeT/ORCA) and Sicily (KM3NeT/ARCA). The KM3NeT/ORCA detector features an energy detection threshold which allows to collect atmospheric neutrinos to study flavour oscillation. This paper reports the KM3NeT/ORCA sensitivity to this phenomenon. The event reconstruction, selection and classification are described. The sensitivity to determine the neutrino mass ordering was evaluated and found to be 4.4 $蟽$ if the true ordering is normal and 2.3 $蟽$ if inverted, after three years of data taking. The precision to measure $螖m^2_{32}$ and $胃_{23}$ were also estimated and found to be $85\cdot10^{-6}$ eV$^2$ and $(^{+1.9}_{-3.1})^{\circ}$ for normal neutrino mass ordering and, $75\cdot10^{-6}$ eV$^2$ and $(^{+2.0}_{-7.0})^{\circ}$ for inverted ordering. Finally, a unitarity test of the leptonic mixing matrix by measuring the rate of tau neutrinos is described. Three years of data taking were found to be sufficient to exclude $谓_蟿$ and $\bar谓_蟿$ event rate variations larger than 20% at $3蟽$ level. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2103.09885v2-abstract-full').style.display = 'none'; document.getElementById('2103.09885v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 November, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 17 March, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2021. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Accepted for publication at EPJ-C</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur. Phys. J. C 82, 26 (2022) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2101.12170">arXiv:2101.12170</a> <span> [<a href="https://arxiv.org/pdf/2101.12170">pdf</a>, <a href="https://arxiv.org/format/2101.12170">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.physletb.2021.136228">10.1016/j.physletb.2021.136228 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of the atmospheric $谓_e$ and $谓_渭$ energy spectra with the ANTARES neutrino telescope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Alves%2C+S">S. Alves</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Belhorma%2C+B">B. Belhorma</a>, <a href="/search/hep-ex?searchtype=author&query=Bendahman%2C+M">M. Bendahman</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bissinger%2C+M">M. Bissinger</a>, <a href="/search/hep-ex?searchtype=author&query=Boumaaza%2C+J">J. Boumaaza</a>, <a href="/search/hep-ex?searchtype=author&query=Bouta%2C+M">M. Bouta</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Br%C3%A2nza%C5%9F%2C+H">H. Br芒nza艧</a>, <a href="/search/hep-ex?searchtype=author&query=Bruijn%2C+R">R. Bruijn</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Caramete%2C+L">L. Caramete</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+J">J. Carr</a> , et al. (117 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2101.12170v2-abstract-short" style="display: inline;"> This letter presents a combined measurement of the energy spectra of atmospheric $谓_e$ and $谓_渭$ in the energy range between $\sim$100 GeV and $\sim$50 TeV with the ANTARES neutrino telescope. The analysis uses 3012 days of detector livetime in the period 2007--2017, and selects 1016 neutrinos interacting in (or close to) the instrumented volume of the detector, yielding shower-like events (mainly… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2101.12170v2-abstract-full').style.display = 'inline'; document.getElementById('2101.12170v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2101.12170v2-abstract-full" style="display: none;"> This letter presents a combined measurement of the energy spectra of atmospheric $谓_e$ and $谓_渭$ in the energy range between $\sim$100 GeV and $\sim$50 TeV with the ANTARES neutrino telescope. The analysis uses 3012 days of detector livetime in the period 2007--2017, and selects 1016 neutrinos interacting in (or close to) the instrumented volume of the detector, yielding shower-like events (mainly from $谓_e+\overline 谓_e$ charged current plus all neutrino neutral current interactions) and starting track events (mainly from $谓_渭+ \overline 谓_渭$ charged current interactions). The contamination by atmospheric muons in the final sample is suppressed at the level of a few per mill by different steps in the selection analysis, including a Boosted Decision Tree classifier. The distribution of reconstructed events is unfolded in terms of electron and muon neutrino fluxes. The derived energy spectra are compared with previous measurements that, above 100 GeV, are limited to experiments in polar ice and, for $谓_渭$, to Super-Kamiokande. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2101.12170v2-abstract-full').style.display = 'none'; document.getElementById('2101.12170v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 March, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 28 January, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2021. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Accepted to PLB</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2008.02127">arXiv:2008.02127</a> <span> [<a href="https://arxiv.org/pdf/2008.02127">pdf</a>, <a href="https://arxiv.org/format/2008.02127">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1093/mnras/staa3503">10.1093/mnras/staa3503 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Constraining the contribution of Gamma-Ray Bursts to the high-energy diffuse neutrino flux with 10 years of ANTARES data </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=ANTARES+Collaboration"> ANTARES Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Belhorma%2C+B">B. Belhorma</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bissinger%2C+M">M. Bissinger</a>, <a href="/search/hep-ex?searchtype=author&query=Boumaaza%2C+J">J. Boumaaza</a>, <a href="/search/hep-ex?searchtype=author&query=Bouta%2C+M">M. Bouta</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Br%C3%A2nza%C5%9F%2C+H">H. Br芒nza艧</a>, <a href="/search/hep-ex?searchtype=author&query=Bruijn%2C+R">R. Bruijn</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Caramete%2C+L">L. Caramete</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+J">J. Carr</a>, <a href="/search/hep-ex?searchtype=author&query=Celli%2C+S">S. Celli</a> , et al. (111 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2008.02127v2-abstract-short" style="display: inline;"> Addressing the origin of the astrophysical neutrino flux observed by IceCube is of paramount importance. Gamma-Ray Bursts (GRBs) are among the few astrophysical sources capable of achieving the required energy to contribute to such neutrino flux through p$纬$ interactions. In this work, ANTARES data have been used to search for upward going muon neutrinos in spatial and temporal coincidence with 78… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2008.02127v2-abstract-full').style.display = 'inline'; document.getElementById('2008.02127v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2008.02127v2-abstract-full" style="display: none;"> Addressing the origin of the astrophysical neutrino flux observed by IceCube is of paramount importance. Gamma-Ray Bursts (GRBs) are among the few astrophysical sources capable of achieving the required energy to contribute to such neutrino flux through p$纬$ interactions. In this work, ANTARES data have been used to search for upward going muon neutrinos in spatial and temporal coincidence with 784 GRBs occurred from 2007 to 2017. For each GRB, the expected neutrino flux has been calculated in the framework of the internal shock model and the impact of the lack of knowledge on the majority of source redshifts and on other intrinsic parameters of the emission mechanism has been quantified. It is found that the model parameters that set the radial distance where shock collisions occur have the largest impact on neutrino flux expectations. In particular, the bulk Lorentz factor of the source ejecta and the minimum variability timescale are found to contribute significantly to the GRB-neutrino flux uncertainty. For the selected sources, ANTARES data have been analysed, by maximising the discovery probability of the stacking sample through an extended maximum-likelihood strategy. Since no neutrino event passed the quality cuts set by the optimisation procedure, 90\% confidence level upper limits (with their uncertainty) on the total expected diffuse neutrino flux have been derived, according to the model. The GRB contribution to the observed diffuse astrophysical neutrino flux around 100 TeV is constrained to be less than 10\%. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2008.02127v2-abstract-full').style.display = 'none'; document.getElementById('2008.02127v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 November, 2020; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 5 August, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Accepted to MNRAS</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> MNRAS 500 (2021) 5614 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2007.00931">arXiv:2007.00931</a> <span> [<a href="https://arxiv.org/pdf/2007.00931">pdf</a>, <a href="https://arxiv.org/ps/2007.00931">ps</a>, <a href="https://arxiv.org/format/2007.00931">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevD.102.122007">10.1103/PhysRevD.102.122007 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Observation of the cosmic ray shadow of the Sun with the ANTARES neutrino telescope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=ANTARES+Collaboration"> ANTARES Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Belhorma1%2C+B">B. Belhorma1</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bissinger%2C+M">M. Bissinger</a>, <a href="/search/hep-ex?searchtype=author&query=Boumaaza%2C+J">J. Boumaaza</a>, <a href="/search/hep-ex?searchtype=author&query=Bouta%2C+M">M. Bouta</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Br%C3%A2nza%C5%9F%2C+H">H. Br芒nza艧</a>, <a href="/search/hep-ex?searchtype=author&query=Bruijn%2C+R">R. Bruijn</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Caramete%2C+L">L. Caramete</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+J">J. Carr</a>, <a href="/search/hep-ex?searchtype=author&query=Celli%2C+S">S. Celli</a> , et al. (112 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2007.00931v2-abstract-short" style="display: inline;"> The ANTARES detector is an undersea neutrino telescope in the Mediterranean Sea. The search for point-like neutrino sources is one of the main goals of the ANTARES telescope, requiring a reliable method to evaluate the detector angular resolution and pointing accuracy. This work describes the study of the Sun "shadow" effect with the ANTARES detector. The shadow is the deficit in the atmospheric m… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2007.00931v2-abstract-full').style.display = 'inline'; document.getElementById('2007.00931v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2007.00931v2-abstract-full" style="display: none;"> The ANTARES detector is an undersea neutrino telescope in the Mediterranean Sea. The search for point-like neutrino sources is one of the main goals of the ANTARES telescope, requiring a reliable method to evaluate the detector angular resolution and pointing accuracy. This work describes the study of the Sun "shadow" effect with the ANTARES detector. The shadow is the deficit in the atmospheric muon flux in the direction of the Sun caused by the absorption of the primary cosmic rays. This analysis is based on the data collected between 2008 and 2017 by the ANTARES telescope. The observed statistical significance of the Sun shadow detection is $3.7蟽$, with an estimated angular resolution of $0.59^\circ\pm0.10^\circ$ for downward-going muons. The pointing accuracy is found to be consistent with the expectations and no evidence of systematic pointing shifts is observed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2007.00931v2-abstract-full').style.display = 'none'; document.getElementById('2007.00931v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 2 December, 2020; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 2 July, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">7 pages, 5 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 102, 122007 (2020) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2004.08254">arXiv:2004.08254</a> <span> [<a href="https://arxiv.org/pdf/2004.08254">pdf</a>, <a href="https://arxiv.org/format/2004.08254">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/15/10/P10005">10.1088/1748-0221/15/10/P10005 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Event reconstruction for KM3NeT/ORCA using convolutional neural networks </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Aiello%2C+S">Sebastiano Aiello</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">Arnauld Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Garre%2C+S+A">Sergio Alves Garre</a>, <a href="/search/hep-ex?searchtype=author&query=Aly%2C+Z">Zineb Aly</a>, <a href="/search/hep-ex?searchtype=author&query=Ameli%2C+F">Fabrizio Ameli</a>, <a href="/search/hep-ex?searchtype=author&query=Andre%2C+M">Michel Andre</a>, <a href="/search/hep-ex?searchtype=author&query=Androulakis%2C+G">Giorgos Androulakis</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">Marco Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anguita%2C+M">Mancia Anguita</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">Gisela Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">Miquel Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">Julien Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Bagatelas%2C+C">Christos Bagatelas</a>, <a href="/search/hep-ex?searchtype=author&query=Barbarino%2C+G">Giancarlo Barbarino</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">Bruny Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Pree%2C+S+B+d">Suzan Basegmez du Pree</a>, <a href="/search/hep-ex?searchtype=author&query=Bendahman%2C+M">Meriem Bendahman</a>, <a href="/search/hep-ex?searchtype=author&query=Berbee%2C+E">Edward Berbee</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">Vincent Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">Simone Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Biagioni%2C+A">Andrea Biagioni</a>, <a href="/search/hep-ex?searchtype=author&query=Bissinger%2C+M">Matthias Bissinger</a>, <a href="/search/hep-ex?searchtype=author&query=Boettcher%2C+M">Markus Boettcher</a>, <a href="/search/hep-ex?searchtype=author&query=Boumaaza%2C+J">Jihad Boumaaza</a>, <a href="/search/hep-ex?searchtype=author&query=Bouta%2C+M">Mohammed Bouta</a> , et al. (207 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2004.08254v1-abstract-short" style="display: inline;"> The KM3NeT research infrastructure is currently under construction at two locations in the Mediterranean Sea. The KM3NeT/ORCA water-Cherenkov neutrino detector off the French coast will instrument several megatons of seawater with photosensors. Its main objective is the determination of the neutrino mass ordering. This work aims at demonstrating the general applicability of deep convolutional neur… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2004.08254v1-abstract-full').style.display = 'inline'; document.getElementById('2004.08254v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2004.08254v1-abstract-full" style="display: none;"> The KM3NeT research infrastructure is currently under construction at two locations in the Mediterranean Sea. The KM3NeT/ORCA water-Cherenkov neutrino detector off the French coast will instrument several megatons of seawater with photosensors. Its main objective is the determination of the neutrino mass ordering. This work aims at demonstrating the general applicability of deep convolutional neural networks to neutrino telescopes, using simulated datasets for the KM3NeT/ORCA detector as an example. To this end, the networks are employed to achieve reconstruction and classification tasks that constitute an alternative to the analysis pipeline presented for KM3NeT/ORCA in the KM3NeT Letter of Intent. They are used to infer event reconstruction estimates for the energy, the direction, and the interaction point of incident neutrinos. The spatial distribution of Cherenkov light generated by charged particles induced in neutrino interactions is classified as shower- or track-like, and the main background processes associated with the detection of atmospheric neutrinos are recognized. Performance comparisons to machine-learning classification and maximum-likelihood reconstruction algorithms previously developed for KM3NeT/ORCA are provided. It is shown that this application of deep convolutional neural networks to simulated datasets for a large-volume neutrino telescope yields competitive reconstruction results and performance improvements with respect to classical approaches. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2004.08254v1-abstract-full').style.display = 'none'; document.getElementById('2004.08254v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 17 April, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JINST 15 P10005 (2020) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2003.04022">arXiv:2003.04022</a> <span> [<a href="https://arxiv.org/pdf/2003.04022">pdf</a>, <a href="https://arxiv.org/format/2003.04022">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-020-8015-6">10.1140/epjc/s10052-020-8015-6 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=ANTARES+Collaboration"> ANTARES Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+J">J. J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Belhorma%2C+B">B. Belhorma</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bissinger%2C+M">M. Bissinger</a>, <a href="/search/hep-ex?searchtype=author&query=Boumaaza%2C+J">J. Boumaaza</a>, <a href="/search/hep-ex?searchtype=author&query=Bouta%2C+M">M. Bouta</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Br%C3%A2nza%C5%9F%2C+H">H. Br芒nza艧</a>, <a href="/search/hep-ex?searchtype=author&query=Bruijn%2C+R">R. Bruijn</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Caramete%2C+L">L. Caramete</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+J">J. Carr</a>, <a href="/search/hep-ex?searchtype=author&query=Celli%2C+S">S. Celli</a> , et al. (113 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2003.04022v4-abstract-short" style="display: inline;"> An offline search for a neutrino counterpart to gravitational-wave (GW) events detected during the second observation run (O2) of Advanced-LIGO and Advanced-Virgo performed with ANTARES data is presented. In addition to the search for long tracks induced by $谓_渭$ ($\bar谓_渭$) charged current interactions, a search for showering events induced by interactions of neutrinos of any flavour is conducted… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2003.04022v4-abstract-full').style.display = 'inline'; document.getElementById('2003.04022v4-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2003.04022v4-abstract-full" style="display: none;"> An offline search for a neutrino counterpart to gravitational-wave (GW) events detected during the second observation run (O2) of Advanced-LIGO and Advanced-Virgo performed with ANTARES data is presented. In addition to the search for long tracks induced by $谓_渭$ ($\bar谓_渭$) charged current interactions, a search for showering events induced by interactions of neutrinos of any flavour is conducted. The severe spatial and time coincidence provided by the gravitational-wave alert allows regions above the detector horizon to be probed, extending the ANTARES sensitivity over the entire sky. The results of this all-neutrino-flavour and all-sky time dependent analysis are presented. The search for prompt neutrino emission within $\pm$500~s around the time of six GW events yields no neutrino counterparts. Upper limits on the neutrino spectral fluence and constraints on the isotropic radiated energy are set for each GW event analysed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2003.04022v4-abstract-full').style.display = 'none'; document.getElementById('2003.04022v4-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 February, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 9 March, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur. Phys. J. C volume 80 (2020) 487 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1910.00112">arXiv:1910.00112</a> <span> [<a href="https://arxiv.org/pdf/1910.00112">pdf</a>, <a href="https://arxiv.org/format/1910.00112">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.cpc.2020.107433">10.1016/j.cpc.2020.107433 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The Control Unit of the KM3NeT Data Acquisition System </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Aiello%2C+S">S. Aiello</a>, <a href="/search/hep-ex?searchtype=author&query=Ameli%2C+F">F. Ameli</a>, <a href="/search/hep-ex?searchtype=author&query=Andre%2C+M">M. Andre</a>, <a href="/search/hep-ex?searchtype=author&query=Androulakis%2C+G">G. Androulakis</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Bagatelas%2C+C">C. Bagatelas</a>, <a href="/search/hep-ex?searchtype=author&query=Barbarino%2C+G">G. Barbarino</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Pree%2C+S+B+d">S. Basegmez du Pree</a>, <a href="/search/hep-ex?searchtype=author&query=Bendahman%2C+M">M. Bendahman</a>, <a href="/search/hep-ex?searchtype=author&query=Berbee%2C+E">E. Berbee</a>, <a href="/search/hep-ex?searchtype=author&query=Berg%2C+A+M+v+d">A. M. van den Berg</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Biagioni%2C+A">A. Biagioni</a>, <a href="/search/hep-ex?searchtype=author&query=Bissinger%2C+M">M. Bissinger</a>, <a href="/search/hep-ex?searchtype=author&query=Boumaaza%2C+J">J. Boumaaza</a>, <a href="/search/hep-ex?searchtype=author&query=Bourret%2C+S">S. Bourret</a>, <a href="/search/hep-ex?searchtype=author&query=Bouta%2C+M">M. Bouta</a>, <a href="/search/hep-ex?searchtype=author&query=Bouvet%2C+G">G. Bouvet</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M">M. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Bozza%2C+C">C. Bozza</a> , et al. (195 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1910.00112v1-abstract-short" style="display: inline;"> The KM3NeT Collaboration runs a multi-site neutrino observatory in the Mediterranean Sea. Water Cherenkov particle detectors, deep in the sea and far off the coasts of France and Italy, are already taking data while incremental construction progresses. Data Acquisition Control software is operating off-shore detectors as well as testing and qualification stations for their components. The software… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1910.00112v1-abstract-full').style.display = 'inline'; document.getElementById('1910.00112v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1910.00112v1-abstract-full" style="display: none;"> The KM3NeT Collaboration runs a multi-site neutrino observatory in the Mediterranean Sea. Water Cherenkov particle detectors, deep in the sea and far off the coasts of France and Italy, are already taking data while incremental construction progresses. Data Acquisition Control software is operating off-shore detectors as well as testing and qualification stations for their components. The software, named Control Unit, is highly modular. It can undergo upgrades and reconfiguration with the acquisition running. Interplay with the central database of the Collaboration is obtained in a way that allows for data taking even if Internet links fail. In order to simplify the management of computing resources in the long term, and to cope with possible hardware failures of one or more computers, the KM3NeT Control Unit software features a custom dynamic resource provisioning and failover technology, which is especially important for ensuring continuity in case of rare transient events in multi-messenger astronomy. The software architecture relies on ubiquitous tools and broadly adopted technologies and has been successfully tested on several operating systems. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1910.00112v1-abstract-full').style.display = 'none'; document.getElementById('1910.00112v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 September, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2019. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1906.02704">arXiv:1906.02704</a> <span> [<a href="https://arxiv.org/pdf/1906.02704">pdf</a>, <a href="https://arxiv.org/format/1906.02704">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-020-7629-z">10.1140/epjc/s10052-020-7629-z <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Dependence of atmospheric muon flux on seawater depth measured with the first KM3NeT detection units </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=KM3NeT+Collaboration"> KM3NeT Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Ageron%2C+M">M. Ageron</a>, <a href="/search/hep-ex?searchtype=author&query=Aiello%2C+S">S. Aiello</a>, <a href="/search/hep-ex?searchtype=author&query=Ameli%2C+F">F. Ameli</a>, <a href="/search/hep-ex?searchtype=author&query=Andre%2C+M">M. Andre</a>, <a href="/search/hep-ex?searchtype=author&query=Androulakis%2C+G">G. Androulakis</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Bagatelas%2C+C">C. Bagatelas</a>, <a href="/search/hep-ex?searchtype=author&query=Barbarino%2C+G">G. Barbarino</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Pree%2C+S+B+d">S. Basegmez du Pree</a>, <a href="/search/hep-ex?searchtype=author&query=Belias%2C+A">A. Belias</a>, <a href="/search/hep-ex?searchtype=author&query=Berbee%2C+E">E. Berbee</a>, <a href="/search/hep-ex?searchtype=author&query=Berg%2C+A+M+v+d">A. M. van den Berg</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=van+Beveren%2C+V">V. van Beveren</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Biagioni%2C+A">A. Biagioni</a>, <a href="/search/hep-ex?searchtype=author&query=Bianucci%2C+S">S. Bianucci</a>, <a href="/search/hep-ex?searchtype=author&query=Billault%2C+M">M. Billault</a>, <a href="/search/hep-ex?searchtype=author&query=Bissinger%2C+M">M. Bissinger</a>, <a href="/search/hep-ex?searchtype=author&query=de+Boer%2C+R">R. de Boer</a> , et al. (240 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1906.02704v3-abstract-short" style="display: inline;"> KM3NeT is a research infrastructure located in the Mediterranean Sea, that will consist of two deep-sea Cherenkov neutrino detectors. With one detector (ARCA), the KM3NeT Collaboration aims at identifying and studying TeV-PeV astrophysical neutrino sources. With the other detector (ORCA), the neutrino mass ordering will be determined by studying GeV-scale atmospheric neutrino oscillations. The fir… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1906.02704v3-abstract-full').style.display = 'inline'; document.getElementById('1906.02704v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1906.02704v3-abstract-full" style="display: none;"> KM3NeT is a research infrastructure located in the Mediterranean Sea, that will consist of two deep-sea Cherenkov neutrino detectors. With one detector (ARCA), the KM3NeT Collaboration aims at identifying and studying TeV-PeV astrophysical neutrino sources. With the other detector (ORCA), the neutrino mass ordering will be determined by studying GeV-scale atmospheric neutrino oscillations. The first KM3NeT detection units were deployed at the Italian and French sites between 2015 and 2017. In this paper, a description of the detector is presented, together with a summary of the procedures used to calibrate the detector in-situ. Finally, the measurement of the atmospheric muon flux between 2232-3386 m seawater depth is obtained. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1906.02704v3-abstract-full').style.display = 'none'; document.getElementById('1906.02704v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 4 February, 2020; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 6 June, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2019. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">15 pages, 9 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur. Phys. J. C 80, 99 (2020) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1812.08650">arXiv:1812.08650</a> <span> [<a href="https://arxiv.org/pdf/1812.08650">pdf</a>, <a href="https://arxiv.org/format/1812.08650">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> Measuring the atmospheric neutrino oscillation parameters and constraining the 3+1 neutrino model with ten years of ANTARES data </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=ANTARES+Collaboration"> ANTARES Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Avgitas%2C+T">T. Avgitas</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Barrios-Mart%C3%AD%2C+J">J. Barrios-Mart铆</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Belhorma%2C+B">B. Belhorma</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bormuth%2C+R">R. Bormuth</a>, <a href="/search/hep-ex?searchtype=author&query=Boumaaza%2C+J">J. Boumaaza</a>, <a href="/search/hep-ex?searchtype=author&query=Bourret%2C+S">S. Bourret</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Br%C3%A2nza%C5%9F%2C+H">H. Br芒nza艧</a>, <a href="/search/hep-ex?searchtype=author&query=Bruijn%2C+R">R. Bruijn</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Caramete%2C+L">L. Caramete</a> , et al. (111 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1812.08650v3-abstract-short" style="display: inline;"> The ANTARES neutrino telescope has an energy threshold of a few tens of GeV. This allows to study the phenomenon of atmospheric muon neutrino disappearance due to neutrino oscillations. In a similar way, constraints on the 3+1 neutrino model, which foresees the existence of one sterile neutrino, can be inferred. Using data collected by the ANTARES neutrino telescope from 2007 to 2016, a new measur… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1812.08650v3-abstract-full').style.display = 'inline'; document.getElementById('1812.08650v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1812.08650v3-abstract-full" style="display: none;"> The ANTARES neutrino telescope has an energy threshold of a few tens of GeV. This allows to study the phenomenon of atmospheric muon neutrino disappearance due to neutrino oscillations. In a similar way, constraints on the 3+1 neutrino model, which foresees the existence of one sterile neutrino, can be inferred. Using data collected by the ANTARES neutrino telescope from 2007 to 2016, a new measurement of $螖m^2_{32}$ and $胃_{23}$ has been performed - which is consistent with world best-fit values - and constraints on the 3+1 neutrino model have been derived. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1812.08650v3-abstract-full').style.display = 'none'; document.getElementById('1812.08650v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 21 May, 2019; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 20 December, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2018. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1807.11815">arXiv:1807.11815</a> <span> [<a href="https://arxiv.org/pdf/1807.11815">pdf</a>, <a href="https://arxiv.org/format/1807.11815">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-018-6451-3">10.1140/epjc/s10052-018-6451-3 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Avgitas%2C+T">T. Avgitas</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Barrios-Mart%C3%ADt%2C+J">J. Barrios-Mart铆t</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Belhorma%2C+B">B. Belhorma</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bormuth%2C+R">R. Bormuth</a>, <a href="/search/hep-ex?searchtype=author&query=Boumaaza%2C+J">J. Boumaaza</a>, <a href="/search/hep-ex?searchtype=author&query=Bourret%2C+S">S. Bourret</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Br%C3%A2nza%2C+H">H. Br芒nza</a>, <a href="/search/hep-ex?searchtype=author&query=Bruijn%2C+R">R. Bruijn</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Caramete%2C+L">L. Caramete</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+J">J. Carr</a> , et al. (102 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1807.11815v1-abstract-short" style="display: inline;"> One of the main objectives of the ANTARES telescope is the search for point-like neutrino sources. Both the pointing accuracy and the angular resolution of the detector are important in this context and a reliable way to evaluate this performance is needed. In order to measure the pointing accuracy of the detector, one possibility is to study the shadow of the Moon, i.e. the deficit of the atmosph… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.11815v1-abstract-full').style.display = 'inline'; document.getElementById('1807.11815v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1807.11815v1-abstract-full" style="display: none;"> One of the main objectives of the ANTARES telescope is the search for point-like neutrino sources. Both the pointing accuracy and the angular resolution of the detector are important in this context and a reliable way to evaluate this performance is needed. In order to measure the pointing accuracy of the detector, one possibility is to study the shadow of the Moon, i.e. the deficit of the atmospheric muon flux from the direction of the Moon induced by the absorption of cosmic rays. Analysing the data taken between 2007 and 2016, the Moon shadow is observed with $3.5蟽$ statistical significance. The detector angular resolution for downward-going muons is 0.73$^{\circ}\pm0.14^{\circ}.$ The resulting pointing performance is consistent with the expectations. An independent check of the telescope pointing accuracy is realised with the data collected by a shower array detector onboard of a ship temporarily moving around the ANTARES location. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.11815v1-abstract-full').style.display = 'none'; document.getElementById('1807.11815v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 31 July, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2018. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">22 pages, 9 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1711.01496">arXiv:1711.01496</a> <span> [<a href="https://arxiv.org/pdf/1711.01496">pdf</a>, <a href="https://arxiv.org/format/1711.01496">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> The ANTARES Collaboration: Contributions to ICRC 2017 Part III: Searches for dark matter and exotics, neutrino oscillations and detector calibration </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=ANTARES+Collaboration"> ANTARES Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Avgitas%2C+T">T. Avgitas</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Barrios-Mart%C3%AD%2C+J">J. Barrios-Mart铆</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Belhorma%2C+B">B. Belhorma</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bormuth%2C+R">R. Bormuth</a>, <a href="/search/hep-ex?searchtype=author&query=Bourret%2C+S">S. Bourret</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Br%C3%A2nza%C5%9F%2C+H">H. Br芒nza艧</a>, <a href="/search/hep-ex?searchtype=author&query=Bruijn%2C+R">R. Bruijn</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Caramete%2C+L">L. Caramete</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+J">J. Carr</a>, <a href="/search/hep-ex?searchtype=author&query=Celli%2C+S">S. Celli</a> , et al. (103 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1711.01496v1-abstract-short" style="display: inline;"> Papers on the searches for dark matter and exotics, neutrino oscillations and detector calibration, prepared for the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the ANTARES Collaboration </span> <span class="abstract-full has-text-grey-dark mathjax" id="1711.01496v1-abstract-full" style="display: none;"> Papers on the searches for dark matter and exotics, neutrino oscillations and detector calibration, prepared for the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the ANTARES Collaboration <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1711.01496v1-abstract-full').style.display = 'none'; document.getElementById('1711.01496v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 4 November, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2017. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1706.01857">arXiv:1706.01857</a> <span> [<a href="https://arxiv.org/pdf/1706.01857">pdf</a>, <a href="https://arxiv.org/format/1706.01857">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevD.96.082001">10.1103/PhysRevD.96.082001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> First all-flavour Neutrino Point-like Source Search with the ANTARES Neutrino Telescope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=ANTARES+Collaboration"> ANTARES Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Avgitas%2C+T">T. Avgitas</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Barrios-Mart%C3%AD%2C+J">J. Barrios-Mart铆</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Belhorma%2C+B">B. Belhorma</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bormuth%2C+R">R. Bormuth</a>, <a href="/search/hep-ex?searchtype=author&query=Bourret%2C+S">S. Bourret</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Br%C3%A2nza%C5%9F%2C+H">H. Br芒nza艧</a>, <a href="/search/hep-ex?searchtype=author&query=Bruijn%2C+R">R. Bruijn</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Caramete%2C+L">L. Caramete</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+J">J. Carr</a>, <a href="/search/hep-ex?searchtype=author&query=Celli%2C+S">S. Celli</a> , et al. (104 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1706.01857v2-abstract-short" style="display: inline;"> A search for cosmic neutrino sources using the data collected with the ANTARES neutrino telescope between early 2007 and the end of 2015 is performed. For the first time, all neutrino interactions --charged and neutral current interactions of all flavours-- are considered in a search for point-like sources with the ANTARES detector. In previous analyses, only muon neutrino charged current interact… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1706.01857v2-abstract-full').style.display = 'inline'; document.getElementById('1706.01857v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1706.01857v2-abstract-full" style="display: none;"> A search for cosmic neutrino sources using the data collected with the ANTARES neutrino telescope between early 2007 and the end of 2015 is performed. For the first time, all neutrino interactions --charged and neutral current interactions of all flavours-- are considered in a search for point-like sources with the ANTARES detector. In previous analyses, only muon neutrino charged current interactions were used. This is achieved by using a novel reconstruction algorithm for shower-like events in addition to the standard muon track reconstruction. The shower channel contributes about 23\% of all signal events for an $E^{-2}$ energy spectrum. No significant excess over background is found. The most signal-like cluster of events is located at $(伪,未) = (343.8^\circ, 23.5^\circ)$ with a significance of $1.9蟽$. The neutrino flux sensitivity of the search is about $E^2 d\varPhi/dE = 6\cdot10^{-9} GeV cm^{-2} s^{-1}$ for declinations from $-90^\circ$ up to $-42^\circ$, and below $10^{-8} GeV cm^{-2} s^{-1}$ for declinations up to $5^{\circ}$. The directions of 106 source candidates and of 13 muon track events from the IceCube HESE sample are investigated for a possible neutrino signal and upper limits on the signal flux are determined. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1706.01857v2-abstract-full').style.display = 'none'; document.getElementById('1706.01857v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 December, 2018; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 6 June, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2017. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">24 pages, 12 figures, submitted to Physical Review D</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 96, 082001 (2017) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1612.06792">arXiv:1612.06792</a> <span> [<a href="https://arxiv.org/pdf/1612.06792">pdf</a>, <a href="https://arxiv.org/format/1612.06792">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> Search for Dark Matter Annihilation in the Earth using the ANTARES Neutrino Telescope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=ANTARES+Collaboration"> ANTARES Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Avgitas%2C+T">T. Avgitas</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Barrios-Mart%C3%AD%2C+J">J. Barrios-Mart铆</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bormuth%2C+R">R. Bormuth</a>, <a href="/search/hep-ex?searchtype=author&query=Bourret%2C+S">S. Bourret</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Bruijn%2C+R">R. Bruijn</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Caramete%2C+L">L. Caramete</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+J">J. Carr</a>, <a href="/search/hep-ex?searchtype=author&query=Celli%2C+S">S. Celli</a>, <a href="/search/hep-ex?searchtype=author&query=Chiarusi%2C+T">T. Chiarusi</a>, <a href="/search/hep-ex?searchtype=author&query=Circella%2C+M">M. Circella</a> , et al. (104 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1612.06792v2-abstract-short" style="display: inline;"> A search for a neutrino signal from WIMP pair annihilations in the centre of the Earth has been performed with the data collected with the ANTARES neutrino telescope from 2007 to 2012. The event selection criteria have been developed and tuned to maximise the sensitivity of the experiment to such a neutrino signal. No significant excess of neutrinos over the expected background has been observed.… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1612.06792v2-abstract-full').style.display = 'inline'; document.getElementById('1612.06792v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1612.06792v2-abstract-full" style="display: none;"> A search for a neutrino signal from WIMP pair annihilations in the centre of the Earth has been performed with the data collected with the ANTARES neutrino telescope from 2007 to 2012. The event selection criteria have been developed and tuned to maximise the sensitivity of the experiment to such a neutrino signal. No significant excess of neutrinos over the expected background has been observed. Upper limits at $90\%$ C.L. on the WIMP annihilation rate in the Earth and the spin independent scattering cross-section of WIMPs to nucleons $蟽^{SI}_p$ were calculated for WIMP pair annihilations into either $蟿^{+}蟿^{-}$, $W^+W^-$, $b\overline{b}$ or the non-SUSY $谓_渭\bar谓_渭$ as a function of the WIMP mass (between $25\,\mathrm{GeV/c^2}$ and $1000\,\mathrm{GeV/c^2}$) and as a function of the thermally averaged annihilation cross section times velocity $\langle蟽_{A} v\rangle_{Earth}$ of the WIMPs in the centre of the Earth. For masses of the WIMP close to the mass of iron nuclei ($50\,\mathrm{GeV/c^2}$), the obtained limits on $蟽^{SI}_p$ are more stringent than those obtained by other indirect searches. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1612.06792v2-abstract-full').style.display = 'none'; document.getElementById('1612.06792v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 April, 2017; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 20 December, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Revised version for journal submission</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1612.05621">arXiv:1612.05621</a> <span> [<a href="https://arxiv.org/pdf/1612.05621">pdf</a>, <a href="https://arxiv.org/format/1612.05621">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1007/JHEP05(2017)008">10.1007/JHEP05(2017)008 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Intrinsic limits on resolutions in muon- and electron-neutrino charged-current events in the KM3NeT/ORCA detector </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Adri%C3%A1n-Mart%C3%ADnez%2C+S">S. Adri谩n-Mart铆nez</a>, <a href="/search/hep-ex?searchtype=author&query=Ageron%2C+M">M. Ageron</a>, <a href="/search/hep-ex?searchtype=author&query=Aiello%2C+S">S. Aiello</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Ameli%2C+F">F. Ameli</a>, <a href="/search/hep-ex?searchtype=author&query=Anassontzis%2C+E+G">E. G. Anassontzis</a>, <a href="/search/hep-ex?searchtype=author&query=Andre%2C+M">M. Andre</a>, <a href="/search/hep-ex?searchtype=author&query=Androulakis%2C+G">G. Androulakis</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Avgitas%2C+T">T. Avgitas</a>, <a href="/search/hep-ex?searchtype=author&query=Barbarino%2C+G">G. Barbarino</a>, <a href="/search/hep-ex?searchtype=author&query=Barbarito%2C+E">E. Barbarito</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Barrios-Mart%C3%AD%2C+J">J. Barrios-Mart铆</a>, <a href="/search/hep-ex?searchtype=author&query=Belias%2C+A">A. Belias</a>, <a href="/search/hep-ex?searchtype=author&query=Berbee%2C+E">E. Berbee</a>, <a href="/search/hep-ex?searchtype=author&query=Berg%2C+A+v+d">A. van den Berg</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Beurthey%2C+S">S. Beurthey</a>, <a href="/search/hep-ex?searchtype=author&query=van+Beveren%2C+V">V. van Beveren</a>, <a href="/search/hep-ex?searchtype=author&query=Beverini%2C+N">N. Beverini</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Biagioni%2C+A">A. Biagioni</a> , et al. (228 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1612.05621v2-abstract-short" style="display: inline;"> Studying atmospheric neutrino oscillations in the few-GeV range with a multimegaton detector promises to determine the neutrino mass hierarchy. This is the main science goal pursued by the future KM3NeT/ORCA water Cherenkov detector in the Mediterranean Sea. In this paper, the processes that limit the obtainable resolution in both energy and direction in charged-current neutrino events in the ORCA… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1612.05621v2-abstract-full').style.display = 'inline'; document.getElementById('1612.05621v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1612.05621v2-abstract-full" style="display: none;"> Studying atmospheric neutrino oscillations in the few-GeV range with a multimegaton detector promises to determine the neutrino mass hierarchy. This is the main science goal pursued by the future KM3NeT/ORCA water Cherenkov detector in the Mediterranean Sea. In this paper, the processes that limit the obtainable resolution in both energy and direction in charged-current neutrino events in the ORCA detector are investigated. These processes include the composition of the hadronic fragmentation products, the subsequent particle propagation and the photon-sampling fraction of the detector. GEANT simulations of neutrino interactions in seawater produced by GENIE are used to study the effects in the 1 - 20 GeV range. It is found that fluctuations in the hadronic cascade in conjunction with the variation of the inelasticity y are most detrimental to the resolutions. The effect of limited photon sampling in the detector is of significantly less importance. These results will therefore also be applicable to similar detectors/media, such as those in ice. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1612.05621v2-abstract-full').style.display = 'none'; document.getElementById('1612.05621v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 May, 2017; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 29 November, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">37 pages, 28 figures, JHEP published version</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> The KM3NeT collaboration, Adri{谩}n-Mart{\'谋}nez, S., Ageron, M. et al. J. High Energ. Phys. (2017) 2017: 8 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1601.07459">arXiv:1601.07459</a> <span> [<a href="https://arxiv.org/pdf/1601.07459">pdf</a>, <a href="https://arxiv.org/format/1601.07459">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/0954-3899/43/8/084001">10.1088/0954-3899/43/8/084001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Letter of Intent for KM3NeT 2.0 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Adri%C3%A1n-Mart%C3%ADnez%2C+S">S. Adri谩n-Mart铆nez</a>, <a href="/search/hep-ex?searchtype=author&query=Ageron%2C+M">M. Ageron</a>, <a href="/search/hep-ex?searchtype=author&query=Aharonian%2C+F">F. Aharonian</a>, <a href="/search/hep-ex?searchtype=author&query=Aiello%2C+S">S. Aiello</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Ameli%2C+F">F. Ameli</a>, <a href="/search/hep-ex?searchtype=author&query=Anassontzis%2C+E">E. Anassontzis</a>, <a href="/search/hep-ex?searchtype=author&query=Andre%2C+M">M. Andre</a>, <a href="/search/hep-ex?searchtype=author&query=Androulakis%2C+G">G. Androulakis</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Avgitas%2C+T">T. Avgitas</a>, <a href="/search/hep-ex?searchtype=author&query=Barbarino%2C+G">G. Barbarino</a>, <a href="/search/hep-ex?searchtype=author&query=Barbarito%2C+E">E. Barbarito</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Barrios-Mart%C3%AD%2C+J">J. Barrios-Mart铆</a>, <a href="/search/hep-ex?searchtype=author&query=Belhorma%2C+B">B. Belhorma</a>, <a href="/search/hep-ex?searchtype=author&query=Belias%2C+A">A. Belias</a>, <a href="/search/hep-ex?searchtype=author&query=Berbee%2C+E">E. Berbee</a>, <a href="/search/hep-ex?searchtype=author&query=Berg%2C+A+v+d">A. van den Berg</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Beurthey%2C+S">S. Beurthey</a>, <a href="/search/hep-ex?searchtype=author&query=van+Beveren%2C+V">V. van Beveren</a>, <a href="/search/hep-ex?searchtype=author&query=Beverini%2C+N">N. Beverini</a> , et al. (222 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1601.07459v2-abstract-short" style="display: inline;"> The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of elect… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.07459v2-abstract-full').style.display = 'inline'; document.getElementById('1601.07459v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1601.07459v2-abstract-full" style="display: none;"> The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: 1) The high-energy astrophysical neutrino signal reported by IceCube and 2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergetic opportunities for the earth and sea sciences community. Three suitable deep-sea sites are identified, namely off-shore Toulon (France), Capo Passero (Italy) and Pylos (Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a 3-dimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be configured to fully explore the IceCube signal with different methodology, improved resolution and complementary field of view, including the Galactic plane. One building block will be configured to precisely measure atmospheric neutrino oscillations. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.07459v2-abstract-full').style.display = 'none'; document.getElementById('1601.07459v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 26 July, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 27 January, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2016. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">119 pages, published version, revised Eq. 6, 7</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Journal of Physics G: Nuclear and Particle Physics, 43 (8), 084001, 2016 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1510.01561">arXiv:1510.01561</a> <span> [<a href="https://arxiv.org/pdf/1510.01561">pdf</a>, <a href="https://arxiv.org/format/1510.01561">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-015-3868-9">10.1140/epjc/s10052-015-3868-9 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The prototype detection unit of the KM3NeT detector </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=KM3NeT+Collaboration"> KM3NeT Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Adri%C3%A1n-Mart%C3%ADnez%2C+S">S. Adri谩n-Mart铆nez</a>, <a href="/search/hep-ex?searchtype=author&query=Ageron%2C+M">M. Ageron</a>, <a href="/search/hep-ex?searchtype=author&query=Aharonian%2C+F">F. Aharonian</a>, <a href="/search/hep-ex?searchtype=author&query=Aiello%2C+S">S. Aiello</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Ameli%2C+F">F. Ameli</a>, <a href="/search/hep-ex?searchtype=author&query=Anassontzis%2C+E+G">E. G. Anassontzis</a>, <a href="/search/hep-ex?searchtype=author&query=Androulakis%2C+G+C">G. C. Androulakis</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Anvar%2C+S">S. Anvar</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Avgitas%2C+T">T. Avgitas</a>, <a href="/search/hep-ex?searchtype=author&query=Balasi%2C+K">K. Balasi</a>, <a href="/search/hep-ex?searchtype=author&query=Band%2C+H">H. Band</a>, <a href="/search/hep-ex?searchtype=author&query=Barbarino%2C+G">G. Barbarino</a>, <a href="/search/hep-ex?searchtype=author&query=Barbarito%2C+E">E. Barbarito</a>, <a href="/search/hep-ex?searchtype=author&query=Barbato%2C+F">F. Barbato</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Baron%2C+S">S. Baron</a>, <a href="/search/hep-ex?searchtype=author&query=Barrios%2C+J">J. Barrios</a>, <a href="/search/hep-ex?searchtype=author&query=Belias%2C+A">A. Belias</a>, <a href="/search/hep-ex?searchtype=author&query=Berbee%2C+E">E. Berbee</a>, <a href="/search/hep-ex?searchtype=author&query=Berg%2C+A+M+v+d">A. M. van den Berg</a> , et al. (224 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1510.01561v2-abstract-short" style="display: inline;"> A prototype detection unit of the KM3NeT deep-sea neutrino telescope has been installed at 3500m depth 80km offshore the Italian coast. KM3NeT in its final configuration will contain several hundreds of detection units. Each detection unit is a mechanical structure anchored to the sea floor, held vertical by a submerged buoy and supporting optical modules for the detection of Cherenkov light emitt… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1510.01561v2-abstract-full').style.display = 'inline'; document.getElementById('1510.01561v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1510.01561v2-abstract-full" style="display: none;"> A prototype detection unit of the KM3NeT deep-sea neutrino telescope has been installed at 3500m depth 80km offshore the Italian coast. KM3NeT in its final configuration will contain several hundreds of detection units. Each detection unit is a mechanical structure anchored to the sea floor, held vertical by a submerged buoy and supporting optical modules for the detection of Cherenkov light emitted by charged secondary particles emerging from neutrino interactions. This prototype string implements three optical modules with 31 photomultiplier tubes each. These optical modules were developed by the KM3NeT Collaboration to enhance the detection capability of neutrino interactions. The prototype detection unit was operated since its deployment in May 2014 until its decommissioning in July 2015. Reconstruction of the particle trajectories from the data requires a nanosecond accuracy in the time calibration. A procedure for relative time calibration of the photomultiplier tubes contained in each optical module is described. This procedure is based on the measured coincidences produced in the sea by the 40K background light and can easily be expanded to a detector with several thousands of optical modules. The time offsets between the different optical modules are obtained using LED nanobeacons mounted inside them. A set of data corresponding to 600 hours of livetime was analysed. The results show good agreement with Monte Carlo simulations of the expected optical background and the signal from atmospheric muons. An almost background-free sample of muons was selected by filtering the time correlated signals on all the three optical modules. The zenith angle of the selected muons was reconstructed with a precision of about 3掳. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1510.01561v2-abstract-full').style.display = 'none'; document.getElementById('1510.01561v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 23 December, 2015; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 6 October, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2015. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Accepted for publication by EPJ C</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur. Phys. J. C (2016) 76:54 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1412.0849">arXiv:1412.0849</a> <span> [<a href="https://arxiv.org/pdf/1412.0849">pdf</a>, <a href="https://arxiv.org/ps/1412.0849">ps</a>, <a href="https://arxiv.org/format/1412.0849">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.astropartphys.2014.12.010">10.1016/j.astropartphys.2014.12.010 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of the atmospheric muon depth intensity relation with the NEMO Phase-2 tower </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Aiello%2C+S">S. Aiello</a>, <a href="/search/hep-ex?searchtype=author&query=Ameli%2C+F">F. Ameli</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Barbarino%2C+G">G. Barbarino</a>, <a href="/search/hep-ex?searchtype=author&query=Barbarito%2C+E">E. Barbarito</a>, <a href="/search/hep-ex?searchtype=author&query=Barbato%2C+F">F. Barbato</a>, <a href="/search/hep-ex?searchtype=author&query=Beverini%2C+N">N. Beverini</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bouhadef%2C+B">B. Bouhadef</a>, <a href="/search/hep-ex?searchtype=author&query=Bozza%2C+C">C. Bozza</a>, <a href="/search/hep-ex?searchtype=author&query=Cacopardo%2C+G">G. Cacopardo</a>, <a href="/search/hep-ex?searchtype=author&query=Calamai%2C+M">M. Calamai</a>, <a href="/search/hep-ex?searchtype=author&query=Cal%C3%AC%2C+C">C. Cal矛</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Caruso%2C+F">F. Caruso</a>, <a href="/search/hep-ex?searchtype=author&query=Ceres%2C+A">A. Ceres</a>, <a href="/search/hep-ex?searchtype=author&query=Chiarusi%2C+T">T. Chiarusi</a>, <a href="/search/hep-ex?searchtype=author&query=Circella%2C+M">M. Circella</a>, <a href="/search/hep-ex?searchtype=author&query=Cocimano%2C+R">R. Cocimano</a>, <a href="/search/hep-ex?searchtype=author&query=Coniglione%2C+R">R. Coniglione</a>, <a href="/search/hep-ex?searchtype=author&query=Costa%2C+M">M. Costa</a>, <a href="/search/hep-ex?searchtype=author&query=Cuttone%2C+G">G. Cuttone</a>, <a href="/search/hep-ex?searchtype=author&query=D%27Amato%2C+C">C. D'Amato</a>, <a href="/search/hep-ex?searchtype=author&query=D%27Amico%2C+A">A. D'Amico</a>, <a href="/search/hep-ex?searchtype=author&query=De+Bonis%2C+G">G. De Bonis</a> , et al. (68 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1412.0849v2-abstract-short" style="display: inline;"> The results of the analysis of the data collected with the NEMO Phase-2 tower, deployed at 3500 m depth about 80 km off-shore Capo Passero (Italy), are presented. Cherenkov photons detected with the photomultipliers tubes were used to reconstruct the tracks of atmospheric muons. Their zenith-angle distribution was measured and the results compared with Monte Carlo simulations. An evaluation of the… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1412.0849v2-abstract-full').style.display = 'inline'; document.getElementById('1412.0849v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1412.0849v2-abstract-full" style="display: none;"> The results of the analysis of the data collected with the NEMO Phase-2 tower, deployed at 3500 m depth about 80 km off-shore Capo Passero (Italy), are presented. Cherenkov photons detected with the photomultipliers tubes were used to reconstruct the tracks of atmospheric muons. Their zenith-angle distribution was measured and the results compared with Monte Carlo simulations. An evaluation of the systematic effects due to uncertainties on environmental and detector parameters is also included. The associated depth intensity relation was evaluated and compared with previous measurements and theoretical predictions. With the present analysis, the muon depth intensity relation has been measured up to 13 km of water equivalent. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1412.0849v2-abstract-full').style.display = 'none'; document.getElementById('1412.0849v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 3 December, 2014; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 2 December, 2014; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2014. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">submitted to Astroparticle Physics</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Astroparticle Physics 66 (2015) 1 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1402.6182">arXiv:1402.6182</a> <span> [<a href="https://arxiv.org/pdf/1402.6182">pdf</a>, <a href="https://arxiv.org/ps/1402.6182">ps</a>, <a href="https://arxiv.org/format/1402.6182">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/2041-8205/786/1/L5">10.1088/2041-8205/786/1/L5 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Searches for Point-like and extended neutrino sources close to the Galactic Centre using the ANTARES neutrino Telescope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=ANTARES+Collaboration"> ANTARES Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Adri%C3%A1n-Mart%C3%ADnez%2C+S">S. Adri谩n-Mart铆nez</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Barrios-Mart%C3%AD%2C+J">J. Barrios-Mart铆</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bogazzi%2C+C">C. Bogazzi</a>, <a href="/search/hep-ex?searchtype=author&query=Bormuth%2C+R">R. Bormuth</a>, <a href="/search/hep-ex?searchtype=author&query=Bou-Cabo%2C+M">M. Bou-Cabo</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Bruijn%2C+R">R. Bruijn</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Caramete%2C+L">L. Caramete</a>, <a href="/search/hep-ex?searchtype=author&query=C%C3%A2rloganu%2C+C">C. C芒rloganu</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+J">J. Carr</a>, <a href="/search/hep-ex?searchtype=author&query=Chiarusi%2C+T">T. Chiarusi</a> , et al. (113 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1402.6182v1-abstract-short" style="display: inline;"> A search for cosmic neutrino sources using six years of data collected by the ANTARES neutrino telescope has been performed. Clusters of muon neutrinos over the expected atmospheric background have been looked for. No clear signal has been found. The most signal-like accumulation of events is located at equatorial coordinates RA=$-$46.8$^{\circ}$ and Dec=$-$64.9$^{\circ}$ and corresponds to a 2.2… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1402.6182v1-abstract-full').style.display = 'inline'; document.getElementById('1402.6182v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1402.6182v1-abstract-full" style="display: none;"> A search for cosmic neutrino sources using six years of data collected by the ANTARES neutrino telescope has been performed. Clusters of muon neutrinos over the expected atmospheric background have been looked for. No clear signal has been found. The most signal-like accumulation of events is located at equatorial coordinates RA=$-$46.8$^{\circ}$ and Dec=$-$64.9$^{\circ}$ and corresponds to a 2.2$蟽$ background fluctuation. In addition, upper limits on the flux normalization of an E$^{-2}$ muon neutrino energy spectrum have been set for 50 pre-selected astrophysical objects. Finally, motivated by an accumulation of 7 events relatively close to the Galactic Centre in the recently reported neutrino sample of the IceCube telescope, a search for point sources in a broad region around this accumulation has been carried out. No indication of a neutrino signal has been found in the ANTARES data and upper limits on the flux normalization of an E$^{-2}$ energy spectrum of neutrinos from point sources in that region have been set. The 90% confidence level upper limits on the muon neutrino flux normalization vary between 3.5 and 5.1$\times$10$^{-8}$ GeV$\,$cm$^{-2}$s$^{-1}$, depending on the exact location of the source. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1402.6182v1-abstract-full').style.display = 'none'; document.getElementById('1402.6182v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 25 February, 2014; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2014. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Submitted to ApJL. 18 pages, 4 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1207.3105">arXiv:1207.3105</a> <span> [<a href="https://arxiv.org/pdf/1207.3105">pdf</a>, <a href="https://arxiv.org/ps/1207.3105">ps</a>, <a href="https://arxiv.org/format/1207.3105">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/0004-637X/760/1/53">10.1088/0004-637X/760/1/53 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for Cosmic Neutrino Point Sources with Four Years of Data from the ANTARES Telescope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=ANTARES+Collaboration"> ANTARES Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Adri%C3%A1n-Mart%C3%ADnez%2C+S">S. Adri谩n-Mart铆nez</a>, <a href="/search/hep-ex?searchtype=author&query=Samarai%2C+I+A">I. Al Samarai</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Anvar%2C+S">S. Anvar</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Astraatmadja%2C+T">T. Astraatmadja</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bigongiari%2C+C">C. Bigongiari</a>, <a href="/search/hep-ex?searchtype=author&query=Bogazzi%2C+C">C. Bogazzi</a>, <a href="/search/hep-ex?searchtype=author&query=Bou-Cabo%2C+M">M. Bou-Cabo</a>, <a href="/search/hep-ex?searchtype=author&query=Bouhou%2C+B">B. Bouhou</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Carloganu%2C+C">C. Carloganu</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+J">J. Carr</a> , et al. (132 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1207.3105v2-abstract-short" style="display: inline;"> In this paper, a time integrated search for point sources of cosmic neutrinos is presented using the data collected from 2007 to 2010 by the ANTARES neutrino telescope. No statistically significant signal has been found and upper limits on the neutrino flux have been obtained. Assuming an $E_谓^{-2}$ spectrum, these flux limits are at $1-10\times10^{-8}$ GeV cm$^{-2}$ s$^{-1}$ for declinations rang… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1207.3105v2-abstract-full').style.display = 'inline'; document.getElementById('1207.3105v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1207.3105v2-abstract-full" style="display: none;"> In this paper, a time integrated search for point sources of cosmic neutrinos is presented using the data collected from 2007 to 2010 by the ANTARES neutrino telescope. No statistically significant signal has been found and upper limits on the neutrino flux have been obtained. Assuming an $E_谓^{-2}$ spectrum, these flux limits are at $1-10\times10^{-8}$ GeV cm$^{-2}$ s$^{-1}$ for declinations ranging from $-90^{\circ}$ to 40$^{\circ}$. Limits for specific models of RX J1713.7-3946 and Vela X, which include information on the source morphology and spectrum, are also given. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1207.3105v2-abstract-full').style.display = 'none'; document.getElementById('1207.3105v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 21 July, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 12 July, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2012. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">30 pages, 13 figures, submitted to ApJ</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1206.6355">arXiv:1206.6355</a> <span> [<a href="https://arxiv.org/pdf/1206.6355">pdf</a>, <a href="https://arxiv.org/format/1206.6355">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevLett.109.112001">10.1103/PhysRevLett.109.112001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of Exclusive $蟺^0$ Electroproduction Structure Functions and their Relationship to Transversity GPDs </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=CLAS+Collaboration"> CLAS Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Bedlinskiy%2C+I">I. Bedlinskiy</a>, <a href="/search/hep-ex?searchtype=author&query=Kubarovsky%2C+V">V. Kubarovsky</a>, <a href="/search/hep-ex?searchtype=author&query=Niccolai%2C+S">S. Niccolai</a>, <a href="/search/hep-ex?searchtype=author&query=Stoler%2C+P">P. Stoler</a>, <a href="/search/hep-ex?searchtype=author&query=Adhikari%2C+K+P">K. P. Adhikari</a>, <a href="/search/hep-ex?searchtype=author&query=Aghasyan%2C+M">M. Aghasyan</a>, <a href="/search/hep-ex?searchtype=author&query=Amaryan%2C+M+J">M. J. Amaryan</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Avakian%2C+H">H. Avakian</a>, <a href="/search/hep-ex?searchtype=author&query=Baghdasaryan%2C+H">H. Baghdasaryan</a>, <a href="/search/hep-ex?searchtype=author&query=Ball%2C+J">J. Ball</a>, <a href="/search/hep-ex?searchtype=author&query=Baltzell%2C+N+A">N. A. Baltzell</a>, <a href="/search/hep-ex?searchtype=author&query=Battaglieri%2C+M">M. Battaglieri</a>, <a href="/search/hep-ex?searchtype=author&query=Bennett%2C+R+P">R. P. Bennett</a>, <a href="/search/hep-ex?searchtype=author&query=Biselli%2C+A+S">A. S. Biselli</a>, <a href="/search/hep-ex?searchtype=author&query=Bookwalter%2C+C">C. Bookwalter</a>, <a href="/search/hep-ex?searchtype=author&query=Boiarinov%2C+S">S. Boiarinov</a>, <a href="/search/hep-ex?searchtype=author&query=Briscoe%2C+W+J">W. J. Briscoe</a>, <a href="/search/hep-ex?searchtype=author&query=Brooks%2C+W+K">W. K. Brooks</a>, <a href="/search/hep-ex?searchtype=author&query=Burkert%2C+V+D">V. D. Burkert</a>, <a href="/search/hep-ex?searchtype=author&query=Carman%2C+D+S">D. S. Carman</a>, <a href="/search/hep-ex?searchtype=author&query=Celentano%2C+A">A. Celentano</a>, <a href="/search/hep-ex?searchtype=author&query=Chandavar%2C+S">S. Chandavar</a>, <a href="/search/hep-ex?searchtype=author&query=Charles%2C+G">G. Charles</a> , et al. (129 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1206.6355v2-abstract-short" style="display: inline;"> Exclusive $蟺^0$ electroproduction at a beam energy of 5.75 GeV has been measured with the Jefferson Lab CLAS spectrometer. Differential cross sections were measured at more than 1800 kinematic values in $Q^2$, $x_B$, $t$, and $蠁_蟺$, in the $Q^2$ range from 1.0 to 4.6 GeV$^2$,\ $-t$ up to 2 GeV$^2$, and $x_B$ from 0.1 to 0.58. Structure functions $蟽_T +蔚蟽_L, 蟽_{TT}$ and $蟽_{LT}$ were extracted as f… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.6355v2-abstract-full').style.display = 'inline'; document.getElementById('1206.6355v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1206.6355v2-abstract-full" style="display: none;"> Exclusive $蟺^0$ electroproduction at a beam energy of 5.75 GeV has been measured with the Jefferson Lab CLAS spectrometer. Differential cross sections were measured at more than 1800 kinematic values in $Q^2$, $x_B$, $t$, and $蠁_蟺$, in the $Q^2$ range from 1.0 to 4.6 GeV$^2$,\ $-t$ up to 2 GeV$^2$, and $x_B$ from 0.1 to 0.58. Structure functions $蟽_T +蔚蟽_L, 蟽_{TT}$ and $蟽_{LT}$ were extracted as functions of $t$ for each of 17 combinations of $Q^2$ and $x_B$. The data were compared directly with two handbag-based calculations including both longitudinal and transversity GPDs. Inclusion of only longitudinal GPDs very strongly underestimates $蟽_T +蔚蟽_L$ and fails to account for $蟽_{TT}$ and $蟽_{LT}$, while inclusion of transversity GPDs brings the calculations into substantially better agreement with the data. There is very strong sensitivity to the relative contributions of nucleon helicity flip and helicity non-flip processes. The results confirm that exclusive $蟺^0$ electroproduction offers direct experimental access to the transversity GPDs. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.6355v2-abstract-full').style.display = 'none'; document.getElementById('1206.6355v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 24 September, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 27 June, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2012. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, 2 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> PRL 109, 112001 (2012) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1206.0645">arXiv:1206.0645</a> <span> [<a href="https://arxiv.org/pdf/1206.0645">pdf</a>, <a href="https://arxiv.org/ps/1206.0645">ps</a>, <a href="https://arxiv.org/format/1206.0645">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.physletb.2012.07.002">10.1016/j.physletb.2012.07.002 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of Atmospheric Neutrino Oscillations with the ANTARES Neutrino Telescope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=ANTARES+collaboration"> ANTARES collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Adrian-Martinez%2C+S">S. Adrian-Martinez</a>, <a href="/search/hep-ex?searchtype=author&query=Samarai%2C+I+A">I. Al Samarai</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andre%2C+M">M. Andre</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Anvar%2C+S">S. Anvar</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Astraatmadja%2C+T">T. Astraatmadja</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bigongiari%2C+C">C. Bigongiari</a>, <a href="/search/hep-ex?searchtype=author&query=Bogazzi%2C+C">C. Bogazzi</a>, <a href="/search/hep-ex?searchtype=author&query=Bou-Cabo%2C+M">M. Bou-Cabo</a>, <a href="/search/hep-ex?searchtype=author&query=Bouhou%2C+B">B. Bouhou</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a>, <a href="/search/hep-ex?searchtype=author&query=Carloganu%2C+C">C. Carloganu</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+J">J. Carr</a> , et al. (135 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1206.0645v2-abstract-short" style="display: inline;"> The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.0645v2-abstract-full').style.display = 'inline'; document.getElementById('1206.0645v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1206.0645v2-abstract-full" style="display: none;"> The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximum mixing, a mass difference of $螖m_{32}^2=(3.1\pm 0.9)\cdot 10^{-3}$ eV$^2$ is obtained, in good agreement with the world average value. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.0645v2-abstract-full').style.display = 'none'; document.getElementById('1206.0645v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 2 July, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 4 June, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2012. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">9 pages, 5 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1204.1105">arXiv:1204.1105</a> <span> [<a href="https://arxiv.org/pdf/1204.1105">pdf</a>, <a href="https://arxiv.org/ps/1204.1105">ps</a>, <a href="https://arxiv.org/format/1204.1105">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Comment on the narrow structure reported by Amaryan et al </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Ball%2C+J">J. Ball</a>, <a href="/search/hep-ex?searchtype=author&query=Baltzell%2C+N+A">N. A. Baltzell</a>, <a href="/search/hep-ex?searchtype=author&query=Battaglieri%2C+M">M. Battaglieri</a>, <a href="/search/hep-ex?searchtype=author&query=Bedlinskiy%2C+I">I. Bedlinskiy</a>, <a href="/search/hep-ex?searchtype=author&query=Bellis%2C+M">M. Bellis</a>, <a href="/search/hep-ex?searchtype=author&query=Biselli%2C+A+S">A. S. Biselli</a>, <a href="/search/hep-ex?searchtype=author&query=Bookwalter%2C+C">C. Bookwalter</a>, <a href="/search/hep-ex?searchtype=author&query=Boiarinov%2C+S">S. Boiarinov</a>, <a href="/search/hep-ex?searchtype=author&query=Bosted%2C+P">P. Bosted</a>, <a href="/search/hep-ex?searchtype=author&query=Burkert%2C+V+D">V. D. Burkert</a>, <a href="/search/hep-ex?searchtype=author&query=Carman%2C+D+S">D. S. Carman</a>, <a href="/search/hep-ex?searchtype=author&query=Celentano%2C+A">A. Celentano</a>, <a href="/search/hep-ex?searchtype=author&query=Chandavar%2C+S">S. Chandavar</a>, <a href="/search/hep-ex?searchtype=author&query=Cole%2C+P+L">P. L. Cole</a>, <a href="/search/hep-ex?searchtype=author&query=Crede%2C+V">V. Crede</a>, <a href="/search/hep-ex?searchtype=author&query=De+Vita%2C+R">R. De Vita</a>, <a href="/search/hep-ex?searchtype=author&query=De+Sanctis%2C+E">E. De Sanctis</a>, <a href="/search/hep-ex?searchtype=author&query=Dey%2C+B">B. Dey</a>, <a href="/search/hep-ex?searchtype=author&query=Dickson%2C+R">R. Dickson</a>, <a href="/search/hep-ex?searchtype=author&query=Doughty%2C+D">D. Doughty</a>, <a href="/search/hep-ex?searchtype=author&query=Dugger%2C+M">M. Dugger</a>, <a href="/search/hep-ex?searchtype=author&query=Dupre%2C+R">R. Dupre</a>, <a href="/search/hep-ex?searchtype=author&query=Egiyan%2C+H">H. Egiyan</a>, <a href="/search/hep-ex?searchtype=author&query=Alaoui%2C+A+E">A. El Alaoui</a> , et al. (72 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1204.1105v1-abstract-short" style="display: inline;"> The CLAS Collaboration provides a comment on the physics interpretation of the results presented in a paper published by M. Amaryan et al. regarding the possible observation of a narrow structure in the mass spectrum of a photoproduction experiment. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1204.1105v1-abstract-full" style="display: none;"> The CLAS Collaboration provides a comment on the physics interpretation of the results presented in a paper published by M. Amaryan et al. regarding the possible observation of a narrow structure in the mass spectrum of a photoproduction experiment. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1204.1105v1-abstract-full').style.display = 'none'; document.getElementById('1204.1105v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 4 April, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2012. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">to be published in Physical Review C</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1110.5184">arXiv:1110.5184</a> <span> [<a href="https://arxiv.org/pdf/1110.5184">pdf</a>, <a href="https://arxiv.org/ps/1110.5184">ps</a>, <a href="https://arxiv.org/format/1110.5184">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.astropartphys.2011.12.003">10.1016/j.astropartphys.2011.12.003 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of the Group Velocity of Light in Sea Water at the ANTARES Site </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Adri%C3%A1n-Mart%C3%ADnez%2C+S">S. Adri谩n-Mart铆nez</a>, <a href="/search/hep-ex?searchtype=author&query=Samarai%2C+I+A">I. Al Samarai</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Anvar%2C+S">S. Anvar</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Jesus%2C+A+C+A">A. C. Assis Jesus</a>, <a href="/search/hep-ex?searchtype=author&query=Astraatmadja%2C+T">T. Astraatmadja</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J">J-J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bigi%2C+A">A. Bigi</a>, <a href="/search/hep-ex?searchtype=author&query=Bigongiari%2C+C">C. Bigongiari</a>, <a href="/search/hep-ex?searchtype=author&query=Bogazzi%2C+C">C. Bogazzi</a>, <a href="/search/hep-ex?searchtype=author&query=Bou-Cabo%2C+M">M. Bou-Cabo</a>, <a href="/search/hep-ex?searchtype=author&query=Bouhou%2C+B">B. Bouhou</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Camarena%2C+F">F. Camarena</a>, <a href="/search/hep-ex?searchtype=author&query=Capone%2C+A">A. Capone</a> , et al. (133 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1110.5184v2-abstract-short" style="display: inline;"> The group velocity of light has been measured at eight different wavelengths between 385 nm and 532 nm in the Mediterranean Sea at a depth of about 2.2 km with the ANTARES optical beacon systems. A parametrisation of the dependence of the refractive index on wavelength based on the salinity, pressure and temperature of the sea water at the ANTARES site is in good agreement with these measurements. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1110.5184v2-abstract-full" style="display: none;"> The group velocity of light has been measured at eight different wavelengths between 385 nm and 532 nm in the Mediterranean Sea at a depth of about 2.2 km with the ANTARES optical beacon systems. A parametrisation of the dependence of the refractive index on wavelength based on the salinity, pressure and temperature of the sea water at the ANTARES site is in good agreement with these measurements. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1110.5184v2-abstract-full').style.display = 'none'; document.getElementById('1110.5184v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 13 February, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 24 October, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2011. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">14 pages, 5 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Astroparticle Physics 35 (2012), pp. 552-557 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1106.2293">arXiv:1106.2293</a> <span> [<a href="https://arxiv.org/pdf/1106.2293">pdf</a>, <a href="https://arxiv.org/ps/1106.2293">ps</a>, <a href="https://arxiv.org/format/1106.2293">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.physletb.2011.09.044">10.1016/j.physletb.2011.09.044 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Precise Measurements of Beam Spin Asymmetries in Semi-Inclusive $蟺^0$ production </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Aghasyan%2C+M">M. Aghasyan</a>, <a href="/search/hep-ex?searchtype=author&query=Avakian%2C+H">H. Avakian</a>, <a href="/search/hep-ex?searchtype=author&query=Rossi%2C+P">P. Rossi</a>, <a href="/search/hep-ex?searchtype=author&query=De+Sanctis%2C+E">E. De Sanctis</a>, <a href="/search/hep-ex?searchtype=author&query=Hasch%2C+D">D. Hasch</a>, <a href="/search/hep-ex?searchtype=author&query=Mirazita%2C+M">M. Mirazita</a>, <a href="/search/hep-ex?searchtype=author&query=Adikaram%2C+D">D. Adikaram</a>, <a href="/search/hep-ex?searchtype=author&query=Amaryan%2C+M+J">M. J. Amaryan</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Baghdasaryan%2C+H">H. Baghdasaryan</a>, <a href="/search/hep-ex?searchtype=author&query=Ball%2C+J">J. Ball</a>, <a href="/search/hep-ex?searchtype=author&query=Battaglieri%2C+M">M. Battaglieri</a>, <a href="/search/hep-ex?searchtype=author&query=Batourine%2C+V">V. Batourine</a>, <a href="/search/hep-ex?searchtype=author&query=Bedlinskiy%2C+I">I. Bedlinskiy</a>, <a href="/search/hep-ex?searchtype=author&query=Bennett%2C+R+P">R. P. Bennett</a>, <a href="/search/hep-ex?searchtype=author&query=Biselli%2C+A+S">A. S. Biselli</a>, <a href="/search/hep-ex?searchtype=author&query=Branford%2C+D">D. Branford</a>, <a href="/search/hep-ex?searchtype=author&query=Briscoe%2C+W+J">W. J. Briscoe</a>, <a href="/search/hep-ex?searchtype=author&query=B%C3%BCltmann%2C+S">S. B眉ltmann</a>, <a href="/search/hep-ex?searchtype=author&query=Burkert%2C+V+D">V. D. Burkert</a>, <a href="/search/hep-ex?searchtype=author&query=Carman%2C+D+S">D. S. Carman</a>, <a href="/search/hep-ex?searchtype=author&query=Chandavar%2C+S">S. Chandavar</a>, <a href="/search/hep-ex?searchtype=author&query=Cole%2C+P+L">P. L. Cole</a>, <a href="/search/hep-ex?searchtype=author&query=Collins%2C+P">P. Collins</a>, <a href="/search/hep-ex?searchtype=author&query=Contalbrigo%2C+M">M. Contalbrigo</a> , et al. (129 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1106.2293v2-abstract-short" style="display: inline;"> We present studies of single-spin asymmetries for neutral pion electroproduction in semi-inclusive deep-inelastic scattering of 5.776 GeV polarized electrons from an unpolarized hydrogen target, using the CEBAF Large Acceptance Spectrometer (CLAS) at the Thomas Jefferson National Accelerator Facility. A substantial $\sin 蠁_h$ amplitude has been measured in the distribution of the cross section asy… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1106.2293v2-abstract-full').style.display = 'inline'; document.getElementById('1106.2293v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1106.2293v2-abstract-full" style="display: none;"> We present studies of single-spin asymmetries for neutral pion electroproduction in semi-inclusive deep-inelastic scattering of 5.776 GeV polarized electrons from an unpolarized hydrogen target, using the CEBAF Large Acceptance Spectrometer (CLAS) at the Thomas Jefferson National Accelerator Facility. A substantial $\sin 蠁_h$ amplitude has been measured in the distribution of the cross section asymmetry as a function of the azimuthal angle $蠁_h$ of the produced neutral pion. The dependence of this amplitude on Bjorken $x$ and on the pion transverse momentum is extracted with significantly higher precision than previous data and is compared to model calculations. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1106.2293v2-abstract-full').style.display = 'none'; document.getElementById('1106.2293v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 12 September, 2011; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 12 June, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2011. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">to be submitted PLB</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Lett.B704:397-402,2011 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1105.4116">arXiv:1105.4116</a> <span> [<a href="https://arxiv.org/pdf/1105.4116">pdf</a>, <a href="https://arxiv.org/ps/1105.4116">ps</a>, <a href="https://arxiv.org/format/1105.4116">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Data Analysis, Statistics and Probability">physics.data-an</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.astropartphys.2011.01.003">10.1016/j.astropartphys.2011.01.003 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A Fast Algorithm for Muon Track Reconstruction and its Application to the ANTARES Neutrino Telescope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=ANTARES+collaboration"> ANTARES collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Aguilar%2C+J+A">J. A. Aguilar</a>, <a href="/search/hep-ex?searchtype=author&query=Samarai%2C+I+A">I. Al Samarai</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andre%2C+M">M. Andre</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Anvar%2C+S">S. Anvar</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Jesus%2C+A+C+A">A. C. Assis Jesus</a>, <a href="/search/hep-ex?searchtype=author&query=Astraatmadja%2C+T">T. Astraatmadja</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J">J-J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Auer%2C+R">R. Auer</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Bazzotti%2C+M">M. Bazzotti</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bigongiari%2C+C">C. Bigongiari</a>, <a href="/search/hep-ex?searchtype=author&query=Bogazzi%2C+C">C. Bogazzi</a>, <a href="/search/hep-ex?searchtype=author&query=Bou-Cabo%2C+M">M. Bou-Cabo</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Brown%2C+A+M">A. M. Brown</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a> , et al. (118 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1105.4116v1-abstract-short" style="display: inline;"> An algorithm is presented, that provides a fast and robust reconstruction of neutrino induced upward-going muons and a discrimination of these events from downward-going atmospheric muon background in data collected by the ANTARES neutrino telescope. The algorithm consists of a hit merging and hit selection procedure followed by fitting steps for a track hypothesis and a point-like light source. I… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1105.4116v1-abstract-full').style.display = 'inline'; document.getElementById('1105.4116v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1105.4116v1-abstract-full" style="display: none;"> An algorithm is presented, that provides a fast and robust reconstruction of neutrino induced upward-going muons and a discrimination of these events from downward-going atmospheric muon background in data collected by the ANTARES neutrino telescope. The algorithm consists of a hit merging and hit selection procedure followed by fitting steps for a track hypothesis and a point-like light source. It is particularly well-suited for real time applications such as online monitoring and fast triggering of optical follow-up observations for multi-messenger studies. The performance of the algorithm is evaluated with Monte Carlo simulations and various distributions are compared with that obtained in ANTARES data. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1105.4116v1-abstract-full').style.display = 'none'; document.getElementById('1105.4116v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 20 May, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2011. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Astropart.Phys.34:652-662,2011 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1012.2204">arXiv:1012.2204</a> <span> [<a href="https://arxiv.org/pdf/1012.2204">pdf</a>, <a href="https://arxiv.org/ps/1012.2204">ps</a>, <a href="https://arxiv.org/format/1012.2204">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.astropartphys.2010.12.004">10.1016/j.astropartphys.2010.12.004 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Time Calibration of the ANTARES Neutrino Telescope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=The+ANTARES+Collaboration"> The ANTARES Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Aguilar%2C+J+A">J. A. Aguilar</a>, <a href="/search/hep-ex?searchtype=author&query=Samarai%2C+I+A">I. Al Samarai</a>, <a href="/search/hep-ex?searchtype=author&query=Albert%2C+A">A. Albert</a>, <a href="/search/hep-ex?searchtype=author&query=Andr%C3%A9%2C+M">M. Andr茅</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Anton%2C+G">G. Anton</a>, <a href="/search/hep-ex?searchtype=author&query=Anvar%2C+S">S. Anvar</a>, <a href="/search/hep-ex?searchtype=author&query=Ardid%2C+M">M. Ardid</a>, <a href="/search/hep-ex?searchtype=author&query=Jesus%2C+A+C+A">A. C. Assis Jesus</a>, <a href="/search/hep-ex?searchtype=author&query=Astraatmadja%2C+T">T. Astraatmadja</a>, <a href="/search/hep-ex?searchtype=author&query=Aubert%2C+J+J">J. J. Aubert</a>, <a href="/search/hep-ex?searchtype=author&query=Auer%2C+R">R. Auer</a>, <a href="/search/hep-ex?searchtype=author&query=Baret%2C+B">B. Baret</a>, <a href="/search/hep-ex?searchtype=author&query=Basa%2C+S">S. Basa</a>, <a href="/search/hep-ex?searchtype=author&query=Bazzotti%2C+M">M. Bazzotti</a>, <a href="/search/hep-ex?searchtype=author&query=Bertin%2C+V">V. Bertin</a>, <a href="/search/hep-ex?searchtype=author&query=Biagi%2C+S">S. Biagi</a>, <a href="/search/hep-ex?searchtype=author&query=Bigongiari%2C+C">C. Bigongiari</a>, <a href="/search/hep-ex?searchtype=author&query=Bou-Cabo%2C+M">M. Bou-Cabo</a>, <a href="/search/hep-ex?searchtype=author&query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/hep-ex?searchtype=author&query=Brown%2C+A+M">A. M. Brown</a>, <a href="/search/hep-ex?searchtype=author&query=Brunner%2C+J">J. Brunner</a>, <a href="/search/hep-ex?searchtype=author&query=Busto%2C+J">J. Busto</a>, <a href="/search/hep-ex?searchtype=author&query=Camarena%2C+F">F. Camarena</a> , et al. (113 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1012.2204v1-abstract-short" style="display: inline;"> The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the detector. The large scattering length of light in the deep sea facilitates an angular resolution of a few tenths of a degree for neutrino energies exceeding 10 Te… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1012.2204v1-abstract-full').style.display = 'inline'; document.getElementById('1012.2204v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1012.2204v1-abstract-full" style="display: none;"> The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the detector. The large scattering length of light in the deep sea facilitates an angular resolution of a few tenths of a degree for neutrino energies exceeding 10 TeV. In order to achieve this optimal performance, the time calibration procedures should ensure a relative time calibration between the photomultipliers at the level of about 1ns. The methods developed to attain this level of precision are described. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1012.2204v1-abstract-full').style.display = 'none'; document.getElementById('1012.2204v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 December, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2010. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">23 pages, 20 figures, accepted by Astropart. Phys</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Astropart.Phys.34:539-549,2011 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1003.4549">arXiv:1003.4549</a> <span> [<a href="https://arxiv.org/pdf/1003.4549">pdf</a>, <a href="https://arxiv.org/ps/1003.4549">ps</a>, <a href="https://arxiv.org/format/1003.4549">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevLett.105.262002">10.1103/PhysRevLett.105.262002 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of Single and Double Spin Asymmetries in Deep Inelastic Pion Electroproduction with a Longitudinally Polarized Target </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=The+CLAS+Collaboration"> The CLAS Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Avakian%2C+H">H. Avakian</a>, <a href="/search/hep-ex?searchtype=author&query=Bosted%2C+P">P. Bosted</a>, <a href="/search/hep-ex?searchtype=author&query=Burkert%2C+V+D">V. D. Burkert</a>, <a href="/search/hep-ex?searchtype=author&query=Elouadrhiri%2C+L">L. Elouadrhiri</a>, <a href="/search/hep-ex?searchtype=author&query=Adhikari%2C+K+P">K. P. Adhikari</a>, <a href="/search/hep-ex?searchtype=author&query=Aghasyan%2C+M">M. Aghasyan</a>, <a href="/search/hep-ex?searchtype=author&query=Amaryan%2C+M">M. Amaryan</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Baghdasaryan%2C+H">H. Baghdasaryan</a>, <a href="/search/hep-ex?searchtype=author&query=Ball%2C+J">J. Ball</a>, <a href="/search/hep-ex?searchtype=author&query=Battaglieri%2C+M">M. Battaglieri</a>, <a href="/search/hep-ex?searchtype=author&query=Bedlinskiy%2C+I">I. Bedlinskiy</a>, <a href="/search/hep-ex?searchtype=author&query=Biselli%2C+A+S">A. S. Biselli</a>, <a href="/search/hep-ex?searchtype=author&query=Branford%2C+D">D. Branford</a>, <a href="/search/hep-ex?searchtype=author&query=Briscoe%2C+W+J">W. J. Briscoe</a>, <a href="/search/hep-ex?searchtype=author&query=Brooks%2C+W">W. Brooks</a>, <a href="/search/hep-ex?searchtype=author&query=Carman%2C+D+S">D. S. Carman</a>, <a href="/search/hep-ex?searchtype=author&query=Casey%2C+L">L. Casey</a>, <a href="/search/hep-ex?searchtype=author&query=Cole%2C+P+L">P. L. Cole</a>, <a href="/search/hep-ex?searchtype=author&query=Collins%2C+P">P. Collins</a>, <a href="/search/hep-ex?searchtype=author&query=Crabb%2C+D">D. Crabb</a>, <a href="/search/hep-ex?searchtype=author&query=Crede%2C+V">V. Crede</a>, <a href="/search/hep-ex?searchtype=author&query=D%27Angelo%2C+A">A. D'Angelo</a>, <a href="/search/hep-ex?searchtype=author&query=Daniel%2C+A">A. Daniel</a> , et al. (123 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1003.4549v1-abstract-short" style="display: inline;"> We report the first measurement of the transverse momentum dependence of double spin asymmetries in semi-inclusive production of pions in deep inelastic scattering off the longitudinally polarized proton. Data have been obtained using a polarized electron beam of 5.7 GeV with the CLAS detector at the Thomas Jefferson National Accelerator Facility (JLab). A significant non-zero $\sin2蠁$ single spin… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1003.4549v1-abstract-full').style.display = 'inline'; document.getElementById('1003.4549v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1003.4549v1-abstract-full" style="display: none;"> We report the first measurement of the transverse momentum dependence of double spin asymmetries in semi-inclusive production of pions in deep inelastic scattering off the longitudinally polarized proton. Data have been obtained using a polarized electron beam of 5.7 GeV with the CLAS detector at the Thomas Jefferson National Accelerator Facility (JLab). A significant non-zero $\sin2蠁$ single spin asymmetry was also observed for the first time indicating strong spin-orbit correlations for transversely polarized quarks in the longitudinally polarized proton. The azimuthal modulations of single spin asymmetries have been measured over a wide kinematic range. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1003.4549v1-abstract-full').style.display = 'none'; document.getElementById('1003.4549v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 23 March, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2010. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.Lett.105:262002,2010 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/hep-ex/0301033">arXiv:hep-ex/0301033</a> <span> [<a href="https://arxiv.org/pdf/hep-ex/0301033">pdf</a>, <a href="https://arxiv.org/ps/hep-ex/0301033">ps</a>, <a href="https://arxiv.org/format/hep-ex/0301033">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1142/9789812705167_0036">10.1142/9789812705167_0036 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The proton structure function F2 in the resonance region </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Osipenko%2C+M">M. Osipenko</a>, <a href="/search/hep-ex?searchtype=author&query=Ricco%2C+G">G. Ricco</a>, <a href="/search/hep-ex?searchtype=author&query=Taiuti%2C+M">M. Taiuti</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Battaglieri%2C+M">M. Battaglieri</a>, <a href="/search/hep-ex?searchtype=author&query=De+Vita%2C+R">R. De Vita</a>, <a href="/search/hep-ex?searchtype=author&query=Ripani%2C+M">M. Ripani</a>, <a href="/search/hep-ex?searchtype=author&query=Collaboration%2C+t+C">the CLAS Collaboration</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="hep-ex/0301033v2-abstract-short" style="display: inline;"> Unique measurement of the proton structure function F2 in a wide two-dimensional region of x and Q**2 has been reported. The accessible kinematics covers entire resonance region up to W=2.5 GeV in the Q**2 interval from 0.1 to 4.5 GeV**2. Obtained data allowed for the first time an evaluation of moments of the structure function F2 directly from experimental data as well as an intensive study of… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('hep-ex/0301033v2-abstract-full').style.display = 'inline'; document.getElementById('hep-ex/0301033v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="hep-ex/0301033v2-abstract-full" style="display: none;"> Unique measurement of the proton structure function F2 in a wide two-dimensional region of x and Q**2 has been reported. The accessible kinematics covers entire resonance region up to W=2.5 GeV in the Q**2 interval from 0.1 to 4.5 GeV**2. Obtained data allowed for the first time an evaluation of moments of the structure function F2 directly from experimental data as well as an intensive study of the Bloom-Gilman duality phenomenon. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('hep-ex/0301033v2-abstract-full').style.display = 'none'; document.getElementById('hep-ex/0301033v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 February, 2003; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 24 January, 2003; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2003. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, 4 figures, Proceedings of GDH2002 Conference, 3-6 July 2002, Genova, Italy, to be published in World Scientific</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/hep-ex/0011098">arXiv:hep-ex/0011098</a> <span> [<a href="https://arxiv.org/pdf/hep-ex/0011098">pdf</a>, <a href="https://arxiv.org/ps/hep-ex/0011098">ps</a>, <a href="https://arxiv.org/format/hep-ex/0011098">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/S0370-2693(02)01196-6">10.1016/S0370-2693(02)01196-6 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Differential cross section measurement of eta photoproduction on the proton from threshold to 1100 MeV </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=GRAAL+collaboration"> GRAAL collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Renard%2C+F">F. Renard</a>, <a href="/search/hep-ex?searchtype=author&query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/hep-ex?searchtype=author&query=Bartalini%2C+O">O. Bartalini</a>, <a href="/search/hep-ex?searchtype=author&query=Bellini%2C+V">V. Bellini</a>, <a href="/search/hep-ex?searchtype=author&query=Bocquet%2C+J+-">J. -P. Bocquet</a>, <a href="/search/hep-ex?searchtype=author&query=Capogni%2C+M">M. Capogni</a>, <a href="/search/hep-ex?searchtype=author&query=Castoldi%2C+M">M. Castoldi</a>, <a href="/search/hep-ex?searchtype=author&query=Corvisiero%2C+P">P. Corvisiero</a>, <a href="/search/hep-ex?searchtype=author&query=D%27Angelo%2C+A">A. D'Angelo</a>, <a href="/search/hep-ex?searchtype=author&query=Didelez%2C+J+-">J. -P. Didelez</a>, <a href="/search/hep-ex?searchtype=author&query=Di+Salvo%2C+R">R. Di Salvo</a>, <a href="/search/hep-ex?searchtype=author&query=Gaulard%2C+C">C. Gaulard</a>, <a href="/search/hep-ex?searchtype=author&query=Gervino%2C+G">G. Gervino</a>, <a href="/search/hep-ex?searchtype=author&query=Ghio%2C+F">F. Ghio</a>, <a href="/search/hep-ex?searchtype=author&query=Girolami%2C+B">B. Girolami</a>, <a href="/search/hep-ex?searchtype=author&query=Guidal%2C+M">M. Guidal</a>, <a href="/search/hep-ex?searchtype=author&query=Hourany%2C+E">E. Hourany</a>, <a href="/search/hep-ex?searchtype=author&query=Kouznetsov%2C+V">V. Kouznetsov</a>, <a href="/search/hep-ex?searchtype=author&query=Kunne%2C+R">R. Kunne</a>, <a href="/search/hep-ex?searchtype=author&query=Lapik%2C+A">A. Lapik</a>, <a href="/search/hep-ex?searchtype=author&query=Sandri%2C+P+L">P. Levi Sandri</a>, <a href="/search/hep-ex?searchtype=author&query=Lleres%2C+A">A. Lleres</a>, <a href="/search/hep-ex?searchtype=author&query=Moricciani%2C+D">D. Moricciani</a>, <a href="/search/hep-ex?searchtype=author&query=Nedorezov%2C+V">V. Nedorezov</a> , et al. (11 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="hep-ex/0011098v2-abstract-short" style="display: inline;"> The differential cross section for the reaction p(gamma, eta p) has been measured from threshold to 1100 MeV photon laboratory energy. For the first time, the region of the S11(1535) resonance is fully covered in a photoproduction experiment and allows a precise extraction of its parameters at the photon point. Above 1000 MeV, S-wave dominance vanishes while a P-wave contribution is observed who… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('hep-ex/0011098v2-abstract-full').style.display = 'inline'; document.getElementById('hep-ex/0011098v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="hep-ex/0011098v2-abstract-full" style="display: none;"> The differential cross section for the reaction p(gamma, eta p) has been measured from threshold to 1100 MeV photon laboratory energy. For the first time, the region of the S11(1535) resonance is fully covered in a photoproduction experiment and allows a precise extraction of its parameters at the photon point. Above 1000 MeV, S-wave dominance vanishes while a P-wave contribution is observed whose nature will have to be clarified. These high precision data together with the already measured beam asymmetry data will provide stringent constraints on the extraction of new couplings of baryon resonances to the eta meson. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('hep-ex/0011098v2-abstract-full').style.display = 'none'; document.getElementById('hep-ex/0011098v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 September, 2001; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 30 November, 2000; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2000. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">10 pages, 5 figures, submitted to Phys. Letters B. Typos corrected. Some more information on the S11(1535) parameters</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Lett.B528:215-220,2002 </p> </li> </ol> <div class="is-hidden-tablet">  <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 2020-02-24</a>  </span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary">  <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/about">About</a></li> <li><a href="https://info.arxiv.org/help">Help</a></li> </ul> </div> <div class="column"> <ul class="nav-spaced"> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>contact arXiv</title><desc>Click here to contact arXiv</desc><path d="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg> <a href="https://info.arxiv.org/help/contact.html"> Contact</a> </li> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>subscribe to arXiv mailings</title><desc>Click here to subscribe</desc><path d="M476 3.2L12.5 270.6c-18.1 10.4-15.8 35.6 2.2 43.2L121 358.4l287.3-253.2c5.5-4.9 13.3 2.6 8.6 8.3L176 407v80.5c0 23.6 28.5 32.9 42.5 15.8L282 426l124.6 52.2c14.2 6 30.4-2.9 33-18.2l72-432C515 7.8 493.3-6.8 476 3.2z"/></svg> <a href="https://info.arxiv.org/help/subscribe"> Subscribe</a> </li> </ul> </div> </div> </div>   <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/license/index.html">Copyright</a></li> <li><a href="https://info.arxiv.org/help/policies/privacy_policy.html">Privacy Policy</a></li> </ul> </div> <div class="column sorry-app-links"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/web_accessibility.html">Web Accessibility Assistance</a></li> <li> <p class="help"> <a class="a11y-main-link" href="https://status.arxiv.org" target="_blank">arXiv Operational Status <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 256 512" class="icon filter-dark_grey" role="presentation"><path d="M224.3 273l-136 136c-9.4 9.4-24.6 9.4-33.9 0l-22.6-22.6c-9.4-9.4-9.4-24.6 0-33.9l96.4-96.4-96.4-96.4c-9.4-9.4-9.4-24.6 0-33.9L54.3 103c9.4-9.4 24.6-9.4 33.9 0l136 136c9.5 9.4 9.5 24.6.1 34z"/></svg></a><br> Get status notifications via <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/email/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><path d="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg>email</a> or <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/slack/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 448 512" class="icon filter-black" role="presentation"><path d="M94.12 315.1c0 25.9-21.16 47.06-47.06 47.06S0 341 0 315.1c0-25.9 21.16-47.06 47.06-47.06h47.06v47.06zm23.72 0c0-25.9 21.16-47.06 47.06-47.06s47.06 21.16 47.06 47.06v117.84c0 25.9-21.16 47.06-47.06 47.06s-47.06-21.16-47.06-47.06V315.1zm47.06-188.98c-25.9 0-47.06-21.16-47.06-47.06S139 32 164.9 32s47.06 21.16 47.06 47.06v47.06H164.9zm0 23.72c25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06H47.06C21.16 243.96 0 222.8 0 196.9s21.16-47.06 47.06-47.06H164.9zm188.98 47.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06h-47.06V196.9zm-23.72 0c0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06V79.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06V196.9zM283.1 385.88c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06v-47.06h47.06zm0-23.72c-25.9 0-47.06-21.16-47.06-47.06 0-25.9 21.16-47.06 47.06-47.06h117.84c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06H283.1z"/></svg>slack</a> </p> </li> </ul> </div> </div> </div>  </div> </footer> <script src="https://static.arxiv.org/static/base/1.0.0a5/js/member_acknowledgement.js"></script> </body> </html>

CINXE.COM

Search | arXiv e-print repository