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</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/1112.6353">arXiv:1112.6353</a> <span> [<a href="https://arxiv.org/pdf/1112.6353">pdf</a>, <a href="https://arxiv.org/ps/1112.6353">ps</a>, <a href="https://arxiv.org/format/1112.6353">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/10.1103/PhysRevLett.108.131801">10.1103/PhysRevLett.108.131801 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Indication for the disappearance of reactor electron antineutrinos in the Double Chooz experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Abe%2C+Y">Y. Abe</a>, <a href="/search/hep-ex?searchtype=author&query=Aberle%2C+C">C. Aberle</a>, <a href="/search/hep-ex?searchtype=author&query=Akiri%2C+T">T. Akiri</a>, <a href="/search/hep-ex?searchtype=author&query=Anjos%2C+J+C+d">J. C. dos Anjos</a>, <a href="/search/hep-ex?searchtype=author&query=Ardellier%2C+F">F. Ardellier</a>, <a href="/search/hep-ex?searchtype=author&query=Barbosa%2C+A+F">A. F. Barbosa</a>, <a href="/search/hep-ex?searchtype=author&query=Baxter%2C+A">A. Baxter</a>, <a href="/search/hep-ex?searchtype=author&query=Bergevin%2C+M">M. Bergevin</a>, <a href="/search/hep-ex?searchtype=author&query=Bernstein%2C+A">A. Bernstein</a>, <a href="/search/hep-ex?searchtype=author&query=Bezerra%2C+T+J+C">T. J. C. Bezerra</a>, <a href="/search/hep-ex?searchtype=author&query=Bezrukhov%2C+L">L. Bezrukhov</a>, <a href="/search/hep-ex?searchtype=author&query=Blucher%2C+E">E. Blucher</a>, <a href="/search/hep-ex?searchtype=author&query=Bongrand%2C+M">M. Bongrand</a>, <a href="/search/hep-ex?searchtype=author&query=Bowden%2C+N+S">N. S. Bowden</a>, <a href="/search/hep-ex?searchtype=author&query=Buck%2C+C">C. Buck</a>, <a href="/search/hep-ex?searchtype=author&query=Busenitz%2C+J">J. Busenitz</a>, <a href="/search/hep-ex?searchtype=author&query=Cabrera%2C+A">A. Cabrera</a>, <a href="/search/hep-ex?searchtype=author&query=Caden%2C+E">E. Caden</a>, <a href="/search/hep-ex?searchtype=author&query=Camilleri%2C+L">L. Camilleri</a>, <a href="/search/hep-ex?searchtype=author&query=Carr%2C+R">R. Carr</a>, <a href="/search/hep-ex?searchtype=author&query=Cerrada%2C+M">M. Cerrada</a>, <a href="/search/hep-ex?searchtype=author&query=Chang%2C+P+-">P. -J. Chang</a>, <a href="/search/hep-ex?searchtype=author&query=Chimenti%2C+P">P. Chimenti</a>, <a href="/search/hep-ex?searchtype=author&query=Classen%2C+T">T. Classen</a>, <a href="/search/hep-ex?searchtype=author&query=Collin%2C+A+P">A. P. Collin</a> , et al. (160 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="1112.6353v3-abstract-short" style="display: inline;"> The Double Chooz Experiment presents an indication of reactor electron antineutrino disappearance consistent with neutrino oscillations. A ratio of 0.944 $\pm$ 0.016 (stat) $\pm$ 0.040 (syst) observed to predicted events was obtained in 101 days of running at the Chooz Nuclear Power Plant in France, with two 4.25 GW$_{th}$ reactors. The results were obtained from a single 10 m$^3$ fiducial volume… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1112.6353v3-abstract-full').style.display = 'inline'; document.getElementById('1112.6353v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1112.6353v3-abstract-full" style="display: none;"> The Double Chooz Experiment presents an indication of reactor electron antineutrino disappearance consistent with neutrino oscillations. A ratio of 0.944 $\pm$ 0.016 (stat) $\pm$ 0.040 (syst) observed to predicted events was obtained in 101 days of running at the Chooz Nuclear Power Plant in France, with two 4.25 GW$_{th}$ reactors. The results were obtained from a single 10 m$^3$ fiducial volume detector located 1050 m from the two reactor cores. The reactor antineutrino flux prediction used the Bugey4 measurement as an anchor point. The deficit can be interpreted as an indication of a non-zero value of the still unmeasured neutrino mixing parameter \sang. Analyzing both the rate of the prompt positrons and their energy spectrum we find \sang = 0.086 $\pm$ 0.041 (stat) $\pm$ 0.030 (syst), or, at 90% CL, 0.015 $<$ \sang $\ <$ 0.16. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1112.6353v3-abstract-full').style.display = 'none'; document.getElementById('1112.6353v3-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 March, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 29 December, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 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">7 pages, 4 figures, (new version after PRL referee's comments)</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1111.6645">arXiv:1111.6645</a> <span> [<a href="https://arxiv.org/pdf/1111.6645">pdf</a>, <a href="https://arxiv.org/ps/1111.6645">ps</a>, <a href="https://arxiv.org/format/1111.6645">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/10.1016/j.astropartphys.2011.08.001">10.1016/j.astropartphys.2011.08.001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger Observatory </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=The+Pierre+Auger+Collaboration"> The Pierre Auger Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Abreu%2C+P">P. Abreu</a>, <a href="/search/hep-ex?searchtype=author&query=Aglietta%2C+M">M. Aglietta</a>, <a href="/search/hep-ex?searchtype=author&query=Ahn%2C+E+J">E. J. Ahn</a>, <a href="/search/hep-ex?searchtype=author&query=Albuquerque%2C+I+F+M">I. F. M. Albuquerque</a>, <a href="/search/hep-ex?searchtype=author&query=Allard%2C+D">D. Allard</a>, <a href="/search/hep-ex?searchtype=author&query=Allekotte%2C+I">I. Allekotte</a>, <a href="/search/hep-ex?searchtype=author&query=Allen%2C+J">J. Allen</a>, <a href="/search/hep-ex?searchtype=author&query=Allison%2C+P">P. Allison</a>, <a href="/search/hep-ex?searchtype=author&query=Castillo%2C+J+A">J. Alvarez Castillo</a>, <a href="/search/hep-ex?searchtype=author&query=Alvarez-Mu%C3%B1iz%2C+J">J. Alvarez-Mu帽iz</a>, <a href="/search/hep-ex?searchtype=author&query=Ambrosio%2C+M">M. Ambrosio</a>, <a href="/search/hep-ex?searchtype=author&query=Aminaei%2C+A">A. Aminaei</a>, <a href="/search/hep-ex?searchtype=author&query=Anchordoqui%2C+L">L. Anchordoqui</a>, <a href="/search/hep-ex?searchtype=author&query=Andringa%2C+S">S. Andringa</a>, <a href="/search/hep-ex?searchtype=author&query=Anti%C4%8Di%C4%87%2C+T">T. Anti膷i膰</a>, <a href="/search/hep-ex?searchtype=author&query=Anzalone%2C+A">A. Anzalone</a>, <a href="/search/hep-ex?searchtype=author&query=Aramo%2C+C">C. Aramo</a>, <a href="/search/hep-ex?searchtype=author&query=Arganda%2C+E">E. Arganda</a>, <a href="/search/hep-ex?searchtype=author&query=Arqueros%2C+F">F. Arqueros</a>, <a href="/search/hep-ex?searchtype=author&query=Asorey%2C+H">H. Asorey</a>, <a href="/search/hep-ex?searchtype=author&query=Assis%2C+P">P. Assis</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Ave%2C+M">M. Ave</a>, <a href="/search/hep-ex?searchtype=author&query=Avenier%2C+M">M. Avenier</a> , et al. (473 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="1111.6645v1-abstract-short" style="display: inline;"> In this paper we introduce the concept of Lateral Trigger Probability (LTP) function, i.e., the probability for an extensive air shower (EAS) to trigger an individual detector of a ground based array as a function of distance to the shower axis, taking into account energy, mass and direction of the primary cosmic ray. We apply this concept to the surface array of the Pierre Auger Observatory consi… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1111.6645v1-abstract-full').style.display = 'inline'; document.getElementById('1111.6645v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1111.6645v1-abstract-full" style="display: none;"> In this paper we introduce the concept of Lateral Trigger Probability (LTP) function, i.e., the probability for an extensive air shower (EAS) to trigger an individual detector of a ground based array as a function of distance to the shower axis, taking into account energy, mass and direction of the primary cosmic ray. We apply this concept to the surface array of the Pierre Auger Observatory consisting of a 1.5 km spaced grid of about 1600 water Cherenkov stations. Using Monte Carlo simulations of ultra-high energy showers the LTP functions are derived for energies in the range between 10^{17} and 10^{19} eV and zenith angles up to 65 degs. A parametrization combining a step function with an exponential is found to reproduce them very well in the considered range of energies and zenith angles. The LTP functions can also be obtained from data using events simultaneously observed by the fluorescence and the surface detector of the Pierre Auger Observatory (hybrid events). We validate the Monte-Carlo results showing how LTP functions from data are in good agreement with simulations. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1111.6645v1-abstract-full').style.display = 'none'; document.getElementById('1111.6645v1-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> 28 November, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 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">22 pages, 8 figures. Published in 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 35 (2011) 266-276 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1107.4809">arXiv:1107.4809</a> <span> [<a href="https://arxiv.org/pdf/1107.4809">pdf</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> <p class="title is-5 mathjax"> The Pierre Auger Observatory I: The Cosmic Ray Energy Spectrum and Related Measurements </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=The+Pierre+Auger+Collaboration"> The Pierre Auger Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Abreu%2C+P">P. Abreu</a>, <a href="/search/hep-ex?searchtype=author&query=Aglietta%2C+M">M. Aglietta</a>, <a href="/search/hep-ex?searchtype=author&query=Ahn%2C+E+J">E. J. Ahn</a>, <a href="/search/hep-ex?searchtype=author&query=Albuquerque%2C+I+F+M">I. F. M. Albuquerque</a>, <a href="/search/hep-ex?searchtype=author&query=Allard%2C+D">D. Allard</a>, <a href="/search/hep-ex?searchtype=author&query=Allekotte%2C+I">I. Allekotte</a>, <a href="/search/hep-ex?searchtype=author&query=Allen%2C+J">J. Allen</a>, <a href="/search/hep-ex?searchtype=author&query=Allison%2C+P">P. Allison</a>, <a href="/search/hep-ex?searchtype=author&query=Castillo%2C+J+A">J. Alvarez Castillo</a>, <a href="/search/hep-ex?searchtype=author&query=Alvarez-Mu%C3%B1iz%2C+J">J. Alvarez-Mu帽iz</a>, <a href="/search/hep-ex?searchtype=author&query=Ambrosio%2C+M">M. Ambrosio</a>, <a href="/search/hep-ex?searchtype=author&query=Aminaei%2C+A">A. Aminaei</a>, <a href="/search/hep-ex?searchtype=author&query=Anchordoqui%2C+L">L. Anchordoqui</a>, <a href="/search/hep-ex?searchtype=author&query=Andringa%2C+S">S. Andringa</a>, <a href="/search/hep-ex?searchtype=author&query=Anti%C4%8Di%C4%87%2C+T">T. Anti膷i膰</a>, <a href="/search/hep-ex?searchtype=author&query=Anzalone%2C+A">A. Anzalone</a>, <a href="/search/hep-ex?searchtype=author&query=Aramo%2C+C">C. Aramo</a>, <a href="/search/hep-ex?searchtype=author&query=Arganda%2C+E">E. Arganda</a>, <a href="/search/hep-ex?searchtype=author&query=Arqueros%2C+F">F. Arqueros</a>, <a href="/search/hep-ex?searchtype=author&query=Asorey%2C+H">H. Asorey</a>, <a href="/search/hep-ex?searchtype=author&query=Assis%2C+P">P. Assis</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Ave%2C+M">M. Ave</a>, <a href="/search/hep-ex?searchtype=author&query=Avenier%2C+M">M. Avenier</a> , et al. (471 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="1107.4809v1-abstract-short" style="display: inline;"> Studies of the cosmic ray energy spectrum at the highest energies with the Pierre Auger Observatory </span> <span class="abstract-full has-text-grey-dark mathjax" id="1107.4809v1-abstract-full" style="display: none;"> Studies of the cosmic ray energy spectrum at the highest energies with the Pierre Auger Observatory <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1107.4809v1-abstract-full').style.display = 'none'; document.getElementById('1107.4809v1-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 July, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">Contributions to the 32nd International Cosmic Ray Conference, Beijing, China, August 2011</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1107.4807">arXiv:1107.4807</a> <span> [<a href="https://arxiv.org/pdf/1107.4807">pdf</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/10.1088/1742-6596/375/1/052006">10.1088/1742-6596/375/1/052006 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The Pierre Auger Observatory V: Enhancements </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=The+Pierre+Auger+Collaboration"> The Pierre Auger Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Abreu%2C+P">P. Abreu</a>, <a href="/search/hep-ex?searchtype=author&query=Aglietta%2C+M">M. Aglietta</a>, <a href="/search/hep-ex?searchtype=author&query=Ahn%2C+E+J">E. J. Ahn</a>, <a href="/search/hep-ex?searchtype=author&query=Albuquerque%2C+I+F+M">I. F. M. Albuquerque</a>, <a href="/search/hep-ex?searchtype=author&query=Allard%2C+D">D. Allard</a>, <a href="/search/hep-ex?searchtype=author&query=Allekotte%2C+I">I. Allekotte</a>, <a href="/search/hep-ex?searchtype=author&query=Allen%2C+J">J. Allen</a>, <a href="/search/hep-ex?searchtype=author&query=Allison%2C+P">P. Allison</a>, <a href="/search/hep-ex?searchtype=author&query=Castillo%2C+J+A">J. Alvarez Castillo</a>, <a href="/search/hep-ex?searchtype=author&query=Alvarez-Mu%C3%B1iz%2C+J">J. Alvarez-Mu帽iz</a>, <a href="/search/hep-ex?searchtype=author&query=Ambrosio%2C+M">M. Ambrosio</a>, <a href="/search/hep-ex?searchtype=author&query=Aminaei%2C+A">A. Aminaei</a>, <a href="/search/hep-ex?searchtype=author&query=Anchordoqui%2C+L">L. Anchordoqui</a>, <a href="/search/hep-ex?searchtype=author&query=Andringa%2C+S">S. Andringa</a>, <a href="/search/hep-ex?searchtype=author&query=Anti%C4%8Di%C4%87%2C+T">T. Anti膷i膰</a>, <a href="/search/hep-ex?searchtype=author&query=Anzalone%2C+A">A. Anzalone</a>, <a href="/search/hep-ex?searchtype=author&query=Aramo%2C+C">C. Aramo</a>, <a href="/search/hep-ex?searchtype=author&query=Arganda%2C+E">E. Arganda</a>, <a href="/search/hep-ex?searchtype=author&query=Arqueros%2C+F">F. Arqueros</a>, <a href="/search/hep-ex?searchtype=author&query=Asorey%2C+H">H. Asorey</a>, <a href="/search/hep-ex?searchtype=author&query=Assis%2C+P">P. Assis</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Ave%2C+M">M. Ave</a>, <a href="/search/hep-ex?searchtype=author&query=Avenier%2C+M">M. Avenier</a> , et al. (471 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="1107.4807v1-abstract-short" style="display: inline;"> Ongoing and planned enhancements of the Pierre Auger Observatory </span> <span class="abstract-full has-text-grey-dark mathjax" id="1107.4807v1-abstract-full" style="display: none;"> Ongoing and planned enhancements of the Pierre Auger Observatory <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1107.4807v1-abstract-full').style.display = 'none'; document.getElementById('1107.4807v1-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 July, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">Contributions to 32nd International Cosmic Ray Conference, Beijing, China, August 2011</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1107.4806">arXiv:1107.4806</a> <span> [<a href="https://arxiv.org/pdf/1107.4806">pdf</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> <p class="title is-5 mathjax"> The Pierre Auger Observatory IV: Operation and Monitoring </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=The+Pierre+Auger+Collaboration"> The Pierre Auger Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Abreu%2C+P">P. Abreu</a>, <a href="/search/hep-ex?searchtype=author&query=Aglietta%2C+M">M. Aglietta</a>, <a href="/search/hep-ex?searchtype=author&query=Ahn%2C+E+J">E. J. Ahn</a>, <a href="/search/hep-ex?searchtype=author&query=Albuquerque%2C+I+F+M">I. F. M. Albuquerque</a>, <a href="/search/hep-ex?searchtype=author&query=Allard%2C+D">D. Allard</a>, <a href="/search/hep-ex?searchtype=author&query=Allekotte%2C+I">I. Allekotte</a>, <a href="/search/hep-ex?searchtype=author&query=Allen%2C+J">J. Allen</a>, <a href="/search/hep-ex?searchtype=author&query=Allison%2C+P">P. Allison</a>, <a href="/search/hep-ex?searchtype=author&query=Castillo%2C+J+A">J. Alvarez Castillo</a>, <a href="/search/hep-ex?searchtype=author&query=Alvarez-Mu%C3%B1iz%2C+J">J. Alvarez-Mu帽iz</a>, <a href="/search/hep-ex?searchtype=author&query=Ambrosio%2C+M">M. Ambrosio</a>, <a href="/search/hep-ex?searchtype=author&query=Aminaei%2C+A">A. Aminaei</a>, <a href="/search/hep-ex?searchtype=author&query=Anchordoqui%2C+L">L. Anchordoqui</a>, <a href="/search/hep-ex?searchtype=author&query=Andringa%2C+S">S. Andringa</a>, <a href="/search/hep-ex?searchtype=author&query=Anti%C4%8Di%C4%87%2C+T">T. Anti膷i膰</a>, <a href="/search/hep-ex?searchtype=author&query=Anzalone%2C+A">A. Anzalone</a>, <a href="/search/hep-ex?searchtype=author&query=Aramo%2C+C">C. Aramo</a>, <a href="/search/hep-ex?searchtype=author&query=Arganda%2C+E">E. Arganda</a>, <a href="/search/hep-ex?searchtype=author&query=Arqueros%2C+F">F. Arqueros</a>, <a href="/search/hep-ex?searchtype=author&query=Asorey%2C+H">H. Asorey</a>, <a href="/search/hep-ex?searchtype=author&query=Assis%2C+P">P. Assis</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Ave%2C+M">M. Ave</a>, <a href="/search/hep-ex?searchtype=author&query=Avenier%2C+M">M. Avenier</a> , et al. (471 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="1107.4806v1-abstract-short" style="display: inline;"> Technical reports on operations and monitoring of the Pierre Auger Observatory </span> <span class="abstract-full has-text-grey-dark mathjax" id="1107.4806v1-abstract-full" style="display: none;"> Technical reports on operations and monitoring of the Pierre Auger Observatory <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1107.4806v1-abstract-full').style.display = 'none'; document.getElementById('1107.4806v1-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 July, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">Constributions to 32nd International Cosmic Ray Conference, Beijing, China, August 2011</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1107.4805">arXiv:1107.4805</a> <span> [<a href="https://arxiv.org/pdf/1107.4805">pdf</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> <p class="title is-5 mathjax"> The Pierre Auger Observatory III: Other Astrophysical Observations </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=The+Pierre+Auger+Collaboration"> The Pierre Auger Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Abreu%2C+P">P. Abreu</a>, <a href="/search/hep-ex?searchtype=author&query=Aglietta%2C+M">M. Aglietta</a>, <a href="/search/hep-ex?searchtype=author&query=Ahn%2C+E+J">E. J. Ahn</a>, <a href="/search/hep-ex?searchtype=author&query=Albuquerque%2C+I+F+M">I. F. M. Albuquerque</a>, <a href="/search/hep-ex?searchtype=author&query=Allard%2C+D">D. Allard</a>, <a href="/search/hep-ex?searchtype=author&query=Allekotte%2C+I">I. Allekotte</a>, <a href="/search/hep-ex?searchtype=author&query=Allen%2C+J">J. Allen</a>, <a href="/search/hep-ex?searchtype=author&query=Allison%2C+P">P. Allison</a>, <a href="/search/hep-ex?searchtype=author&query=Castillo%2C+J+A">J. Alvarez Castillo</a>, <a href="/search/hep-ex?searchtype=author&query=Alvarez-Mu%C3%B1iz%2C+J">J. Alvarez-Mu帽iz</a>, <a href="/search/hep-ex?searchtype=author&query=Ambrosio%2C+M">M. Ambrosio</a>, <a href="/search/hep-ex?searchtype=author&query=Aminaei%2C+A">A. Aminaei</a>, <a href="/search/hep-ex?searchtype=author&query=Anchordoqui%2C+L">L. Anchordoqui</a>, <a href="/search/hep-ex?searchtype=author&query=Andringa%2C+S">S. Andringa</a>, <a href="/search/hep-ex?searchtype=author&query=Anti%C4%8Di%C4%87%2C+T">T. Anti膷i膰</a>, <a href="/search/hep-ex?searchtype=author&query=Anzalone%2C+A">A. Anzalone</a>, <a href="/search/hep-ex?searchtype=author&query=Aramo%2C+C">C. Aramo</a>, <a href="/search/hep-ex?searchtype=author&query=Arganda%2C+E">E. Arganda</a>, <a href="/search/hep-ex?searchtype=author&query=Arqueros%2C+F">F. Arqueros</a>, <a href="/search/hep-ex?searchtype=author&query=Asorey%2C+H">H. Asorey</a>, <a href="/search/hep-ex?searchtype=author&query=Assis%2C+P">P. Assis</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Ave%2C+M">M. Ave</a>, <a href="/search/hep-ex?searchtype=author&query=Avenier%2C+M">M. Avenier</a> , et al. (471 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="1107.4805v1-abstract-short" style="display: inline;"> Astrophysical observations of ultra-high-energy cosmic rays with the Pierre Auger Observatory </span> <span class="abstract-full has-text-grey-dark mathjax" id="1107.4805v1-abstract-full" style="display: none;"> Astrophysical observations of ultra-high-energy cosmic rays with the Pierre Auger Observatory <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1107.4805v1-abstract-full').style.display = 'none'; document.getElementById('1107.4805v1-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 July, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">Contributions to the 32nd International Cosmic Ray Conference, Beijing, China, August 2011</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1107.4804">arXiv:1107.4804</a> <span> [<a href="https://arxiv.org/pdf/1107.4804">pdf</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> <p class="title is-5 mathjax"> The Pierre Auger Observatory II: Studies of Cosmic Ray Composition and Hadronic Interaction models </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=The+Pierre+Auger+Collaboration"> The Pierre Auger Collaboration</a>, <a href="/search/hep-ex?searchtype=author&query=Abreu%2C+P">P. Abreu</a>, <a href="/search/hep-ex?searchtype=author&query=Aglietta%2C+M">M. Aglietta</a>, <a href="/search/hep-ex?searchtype=author&query=Ahn%2C+E+J">E. J. Ahn</a>, <a href="/search/hep-ex?searchtype=author&query=Albuquerque%2C+I+F+M">I. F. M. Albuquerque</a>, <a href="/search/hep-ex?searchtype=author&query=Allard%2C+D">D. Allard</a>, <a href="/search/hep-ex?searchtype=author&query=Allekotte%2C+I">I. Allekotte</a>, <a href="/search/hep-ex?searchtype=author&query=Allen%2C+J">J. Allen</a>, <a href="/search/hep-ex?searchtype=author&query=Allison%2C+P">P. Allison</a>, <a href="/search/hep-ex?searchtype=author&query=Castillo%2C+J+A">J. Alvarez Castillo</a>, <a href="/search/hep-ex?searchtype=author&query=Alvarez-Mu%C3%B1iz%2C+J">J. Alvarez-Mu帽iz</a>, <a href="/search/hep-ex?searchtype=author&query=Ambrosio%2C+M">M. Ambrosio</a>, <a href="/search/hep-ex?searchtype=author&query=Aminaei%2C+A">A. Aminaei</a>, <a href="/search/hep-ex?searchtype=author&query=Anchordoqui%2C+L">L. Anchordoqui</a>, <a href="/search/hep-ex?searchtype=author&query=Andringa%2C+S">S. Andringa</a>, <a href="/search/hep-ex?searchtype=author&query=Anti%C4%8Di%C4%87%2C+T">T. Anti膷i膰</a>, <a href="/search/hep-ex?searchtype=author&query=Anzalone%2C+A">A. Anzalone</a>, <a href="/search/hep-ex?searchtype=author&query=Aramo%2C+C">C. Aramo</a>, <a href="/search/hep-ex?searchtype=author&query=Arganda%2C+E">E. Arganda</a>, <a href="/search/hep-ex?searchtype=author&query=Arqueros%2C+F">F. Arqueros</a>, <a href="/search/hep-ex?searchtype=author&query=Asorey%2C+H">H. Asorey</a>, <a href="/search/hep-ex?searchtype=author&query=Assis%2C+P">P. Assis</a>, <a href="/search/hep-ex?searchtype=author&query=Aublin%2C+J">J. Aublin</a>, <a href="/search/hep-ex?searchtype=author&query=Ave%2C+M">M. Ave</a>, <a href="/search/hep-ex?searchtype=author&query=Avenier%2C+M">M. Avenier</a> , et al. (471 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="1107.4804v1-abstract-short" style="display: inline;"> Studies of the composition of the highest energy cosmic rays with the Pierre Auger Observatory, including examination of hadronic physics effects on the structure of extensive air showers. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1107.4804v1-abstract-full" style="display: none;"> Studies of the composition of the highest energy cosmic rays with the Pierre Auger Observatory, including examination of hadronic physics effects on the structure of extensive air showers. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1107.4804v1-abstract-full').style.display = 'none'; document.getElementById('1107.4804v1-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 July, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">Contributions to the 32nd International Cosmic Ray Conference, Beijing, China, August 2011</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/0511059">arXiv:hep-ex/0511059</a> <span> [<a href="https://arxiv.org/pdf/hep-ex/0511059">pdf</a>, <a href="https://arxiv.org/ps/hep-ex/0511059">ps</a>, <a href="https://arxiv.org/format/hep-ex/0511059">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.nuclphysbps.2006.02.058">10.1016/j.nuclphysbps.2006.02.058 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Angra Neutrino Project: status and plans </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&query=Anjos%2C+J+C">J. C. Anjos</a>, <a href="/search/hep-ex?searchtype=author&query=Barbosa%2C+A+F">A. F. Barbosa</a>, <a href="/search/hep-ex?searchtype=author&query=Funchal%2C+R+Z">R. Z. Funchal</a>, <a href="/search/hep-ex?searchtype=author&query=Kemp%2C+E">E. Kemp</a>, <a href="/search/hep-ex?searchtype=author&query=Magnin%2C+J">J. Magnin</a>, <a href="/search/hep-ex?searchtype=author&query=Nunokawa%2C+H">H. Nunokawa</a>, <a href="/search/hep-ex?searchtype=author&query=Peres%2C+O+L+G">O. L. G. Peres</a>, <a href="/search/hep-ex?searchtype=author&query=Reyna%2C+D">D. Reyna</a>, <a href="/search/hep-ex?searchtype=author&query=Shellard%2C+R+C">R. C. Shellard</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/0511059v1-abstract-short" style="display: inline;"> We present the status and plans of the Angra Project, a new nuclear reactor neutrino oscillation experiment, proposed to be built in Brazil at the Angra dos Reis nuclear reactor complex. This experiment is aimed to measure theta_13, the last unknown of the three neutrino mixing angles. Combining a high luminosity design, very low background from cosmic rays and careful control of systematic erro… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('hep-ex/0511059v1-abstract-full').style.display = 'inline'; document.getElementById('hep-ex/0511059v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="hep-ex/0511059v1-abstract-full" style="display: none;"> We present the status and plans of the Angra Project, a new nuclear reactor neutrino oscillation experiment, proposed to be built in Brazil at the Angra dos Reis nuclear reactor complex. This experiment is aimed to measure theta_13, the last unknown of the three neutrino mixing angles. Combining a high luminosity design, very low background from cosmic rays and careful control of systematic errors at the 1% level, we propose a high sensitivity multi-detector experiment, able to reach a sensitivity to antineutrino disappearance down to sin^2(2*theta_13) = 0.006 in a three years running period, improving present limits constrained by the CHOOZ experiment by more than an order of magnitude. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('hep-ex/0511059v1-abstract-full').style.display = 'none'; document.getElementById('hep-ex/0511059v1-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> 29 November, 2005; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2005. </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">2 pages, 1 figure, talk presented by J.C. Anjos (janjos@cbpf.br) at NuFact05, 21-26 June 2005, Frascati, Italy</span> </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>

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