Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA

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gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA</span></h1></div> <div class="rendering rendering_researchoutput rendering_researchoutput_associatespersonsclassifiedportal rendering_contributiontojournal rendering_associatespersonsclassifiedportal rendering_contributiontojournal_associatespersonsclassifiedportal"><p class="relations persons">the KAGRA Collaboration, The LIGO Scientific Collaboration, Virgo Collaboration</div> <div class="rendering rendering_researchoutput rendering_researchoutput_associatesorganisationsportal rendering_contributiontojournal rendering_associatesorganisationsportal rendering_contributiontojournal_associatesorganisationsportal"><ul class="relations organisations"><li class="school_division"><a rel="Organisation" href="https://research.monash.edu/en/organisations/school-of-physics-and-astronomy" class="link"><span>School of Physics and Astronomy</span></a></li></ul></div> <div class="rendering rendering_researchoutput rendering_researchoutput_publicationcontenttyperendererportalng rendering_contributiontojournal rendering_publicationcontenttyperendererportalng rendering_contributiontojournal_publicationcontenttyperendererportalng"><p class="type"><span class="type_family">Research output<span class="type_family_sep">: </span></span><span class="type_classification_parent">Contribution to journal<span class="type_parent_sep"> › </span></span><span class="type_classification">Review Article</span><span class="type_classification"><span class="type_parent_sep"> › </span>Other</span><span class="type_classification"><span class="type_parent_sep"> › </span>peer-review</span></p></div> </div> <div class="publication-metrics" aria-label="Publication metrics section"> <div class="metrics-container"> <div class="metrics-wrap metrics-top one"> <div class="metric scopus-citations"> <a target="_blank" href="http://www.scopus.com/inward/citedby.url?scp=85046034556&partnerID=8YFLogxK" aria-label="Source: Scopus: 923"> <span class="count">923</span> </a> <span class="label">Citations (Scopus)</span> </div> </div> <div class="metrics-wrap metrics-bottom one"> <div class="metric metric-altmetric"> <div data-badge-popover="top" data-badge-type="donut" data-doi="10.1007/s41114-018-0012-9" data-hide-no-mentions="true" data-link-target='_blank' class="altmetric-embed"></div> </div> </div> </div> </div> </div> </div> <div class="subMenu"> <div class="content-profile-navigation"> <div class="container"> <nav role="navigation"> <ul class="has-overflow-navigation" role="menubar"> <li class="selected" role="none"> <a class="portal_link" role="menuitem" href="/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3"><span> <i class="icon icon-publication" aria-hidden="true"></i> <span class="label">Overview</span> </span></a> </li> <li class="" role="none"> <a class="portal_link" role="menuitem" href="/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3/publications/"><span> <i class="icon icon-publications"></i> <span class="label">Outputs</span> <span class="count">(2)</span> </span></a> </li> <li class="" role="none"> <a class="portal_link" role="menuitem" href="/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3/projects/"><span> <i class="icon icon-projects"></i> <span class="label">Projects</span> <span class="count">(1)</span> </span></a> </li> </ul> </nav> </div> </div> </div> </section> <div id="main-content" class="page-section-content page-section-content-publications page-section-content-publications-view "> <section class="page-section content-relation-section"> <div class="container"> <div class="clearfix"> <div class="content-content publication-content"> <h2 class="subheader">Abstract</h2> <div class="rendering rendering_researchoutput rendering_researchoutput_abstractportal rendering_contributiontojournal rendering_abstractportal rendering_contributiontojournal_abstractportal"><div class="textblock"><p>We present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron star systems, which are the most promising targets for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90 % credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5–20deg2 requires at least three detectors of sensitivity within a factor of ∼ 2 of each other and with a broad frequency bandwidth. When all detectors, including KAGRA and the third LIGO detector in India, reach design sensitivity, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.</p></div></div> <div class="rendering rendering_researchoutput rendering_researchoutput_detailsportal rendering_contributiontojournal rendering_detailsportal rendering_contributiontojournal_detailsportal"><div class="systematicreview"><table class="properties"><tbody><tr class="language"><th scope="row">Original language</th><td>English</td></tr><tr><th scope="row">Article number</th><td>3</td></tr><tr class="numberofpages"><th scope="row">Number of pages</th><td>52</td></tr><tr><th scope="row">Journal</th><td><a rel="Journal" href="#" class="link"><span>Living Reviews in Relativity</span></a></td></tr><tr><th scope="row">Volume</th><td>21</td></tr><tr><th scope="row">Issue number</th><td>1</td></tr><tr class="digital_object_identifiers"><th scope="row">DOIs</th><td><ul class="relations digital_object_identifiers"><li><a onclick="window.open(this.href, '_blank','noopener,noreferrer'); return false;" href="https://doi.org/10.1007/s41114-018-0012-9" class="link"><span>https://doi.org/10.1007/s41114-018-0012-9</span></a> </li></ul></td></tr><tr class="status"><th scope="row">Publication status</th><td><span class="prefix">Published - </span><span class="date">1 Dec 2018</span></td></tr></tbody></table></div></div> <div class="rendering rendering_keywordable rendering_expertkeywordgrouspbytypeportal rendering_keywordable_expertkeywordgrouspbytypeportal"><div class="keyword-group"><h2 class="subheader">Keywords</h2><ul class="relations keywords"><li class="userdefined-keyword"><span>Data analysis</span></li><li class="userdefined-keyword"><span>Electromagnetic counterparts</span></li><li class="userdefined-keyword"><span>Gravitational waves</span></li><li class="userdefined-keyword"><span>Gravitational-wave detectors</span></li></ul></div></div> </div> <div class="content-sidebar publication-sidebar"> <h2 class="subheader">Access to Document</h2> <div class="rendering rendering_researchoutput rendering_researchoutput_publicationaccessrenderer rendering_contributiontojournal rendering_publicationaccessrenderer rendering_contributiontojournal_publicationaccessrenderer"><ul class="dois"><li class="open-access"><div class="doi"><a onclick="window.open(this.href, '_blank','noopener,noreferrer'); return false;" href="https://doi.org/10.1007/s41114-018-0012-9" class="link"><span>10.1007/s41114-018-0012-9</span></a></div></li></ul><ul class="documents"><li class="open-access"><div class="document"><a onclick="if (this.href) {window.open(this.href)}; return false;" href="/files/245864733/245844654_oa.pdf" class="link document-link"><span>245844654-oa</span></a><span class="meta">Final published version, 2.78 MB</span></div></li></ul></div> <h2 class="subheader">Other files and links</h2> <div class="rendering rendering_researchoutput rendering_researchoutput_publicationotherfilesandlinksrenderer rendering_contributiontojournal rendering_publicationotherfilesandlinksrenderer rendering_contributiontojournal_publicationotherfilesandlinksrenderer"><ul class="links"><li><div class="link"><a onclick="window.open(this.href, '_blank','noopener,noreferrer'); return false;" href="http://www.scopus.com/inward/record.url?scp=85046034556&partnerID=8YFLogxK" class="link"><span>Link to publication in Scopus</span></a></div></li></ul></div> <div class="rendering rendering_researchoutput rendering_researchoutput_versioneddocumentspureportal rendering_contributiontojournal rendering_versioneddocumentspureportal rendering_contributiontojournal_versioneddocumentspureportal"><ul class="relations documents"></ul></div> </div> </div> </div> </section> <section class="page-section content-relation-section publication-publications"> <div class="container"> <div class="header"> <h2 class="section-title" id="related-publications-title"> <i class="icon icon-publications" aria-hidden="true"></i> <span class="title"> Research output </span> </h2> <div class="content-trends"> <button rel="toggle-publication-chart" data-year-url="/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3/publications/?publicationYear=" aria-label="Research output per year" class="chart-toggler" aria-expanded="false"> <span class="title"> Research output per year <img src="/assets/gizmo-expand-61f33ba7afaffaa77611abfb62f97a9e.svg" aria-hidden="true" alt="" class="expand" /> <img src="/assets/gizmo-contract-7adbcd523b1972d72d537e479dd74798.svg" aria-hidden="true" alt="" class="contract" /> </span> <span class="inline-trend-graph"> <span class="year year-start">2016</span> <span class="trend-graph-wrapper"> <span class="bar" style="height: 100%;"> <span aria-expanded="false" role="tooltip">2016</span> </span> <span class="bar" style="height: 100%;"> <span aria-expanded="false" role="tooltip">2020</span> </span> </span> <span class="year year-end">2020</span> </span> </button> <ul class="content-statistics"> <li class="citations index"> <span class="count increment-counter">923</span> Citations </li> <li class=""> <a class="portal_link count increment-counter" aria-label=" 2 Review Article" href="/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3/publications/?type=%2Fdk%2Fatira%2Fpure%2Fresearchoutput%2Fresearchoutputtypes%2Fcontributiontojournal%2Fsystematicreview"><span> 2 </span></a> <span class="label">Review Article</span> </li> </ul> <script> $("ul.content-statistics li.index").last().addClass("separator"); </script> <div class="flex-break"></div> <div class="chart-container" id="chart-content-publication-by-year" style="display: none;" aria-hidden="true" tabindex="-1"> <p class="legend">Research output per year</p> <div class="chart-wrapper"> <canvas></canvas> </div> <p class="legend">Research output per year</p> </div> <table id="publication-container-table" class="sr-only" aria-hidden="true"></table> <script> $("#chart-content-publication-by-year").contentChart({ toggle: "button[rel='toggle-publication-chart']", title: "Research output per year", labels: [2016, 2017, 2018, 2019, 2020], values: [1, 0, 0, 0, 1], tableContainer: $('#publication-container-table'), }); </script> </div> </div> <div class="relation-list relation-list-publications"> <ul class="list-results"> <li class="list-result-item"> <div class="result-container"> <div class="rendering rendering_researchoutput rendering_researchoutput_portal-short rendering_contributiontojournal rendering_portal-short rendering_contributiontojournal_portal-short"><h3 class="title"><a rel="ContributionToJournal" href="https://research.monash.edu/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-4" class="link"><span>Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA</span></a></h3><span>the KAGRA Collaboration</span>, <span>The LIGO Scientific Collaboration</span> & <span>Virgo Collaboration</span>, <span class="date">1 Dec 2020</span>, <span class="journal">In: <a rel="Journal" href="#" class="link"><span>Living Reviews in Relativity.</span></a></span> <span class="volume">23</span>, <span class="journalnumber">1</span>, <span class="numberofpages">69 p.</span>, 3.<p class="type"><span class="type_family">Research output<span class="type_family_sep">: </span></span><span class="type_classification_parent">Contribution to journal<span class="type_parent_sep"> › </span></span><span class="type_classification">Review Article</span><span class="type_classification"><span class="type_parent_sep"> › </span>Other</span><span class="type_classification"><span class="type_parent_sep"> › </span>peer-review</span></p></div> <div class="rendering rendering_researchoutput rendering_researchoutput_publicationattacheddocumentsportalrenderer rendering_contributiontojournal rendering_publicationattacheddocumentsportalrenderer rendering_contributiontojournal_publicationattacheddocumentsportalrenderer"><div class="open-access">Open Access</div></div> </div> <div class="publication-metrics" aria-label="Publication metrics section"> <div class="metrics-container"> <div class="metrics-wrap metrics-top one"> <div class="metric scopus-citations"> <a target="_blank" href="http://www.scopus.com/inward/citedby.url?scp=85091656606&partnerID=8YFLogxK" aria-label="Source: Scopus: 525"> <span class="count">525</span> </a> <span class="label">Citations (Scopus)</span> </div> </div> <div class="metrics-wrap metrics-bottom one"> <div class="metric metric-altmetric"> <div data-badge-popover="top" data-badge-type="donut" data-doi="10.1007/s41114-020-00026-9" data-hide-no-mentions="true" data-link-target='_blank' class="altmetric-embed"></div> </div> </div> </div> </div> </li> <li class="list-result-item"> <div class="result-container"> <div class="rendering rendering_researchoutput rendering_researchoutput_portal-short rendering_contributiontojournal rendering_portal-short rendering_contributiontojournal_portal-short"><h3 class="title"><a rel="ContributionToJournal" href="https://research.monash.edu/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie" class="link"><span>Prospects for observing and localizing gravitational-wave transients with Advanced LIGO and Advanced Virgo</span></a></h3><span>The LIGO Scientific Collaboration and the Virgo Collaboration</span>, <span class="date">8 Feb 2016</span>, <span class="journal">In: <a rel="Journal" href="#" class="link"><span>Living Reviews in Relativity.</span></a></span> <span class="volume">19</span>, <span class="pages">p. 1-39</span> <span class="numberofpages">39 p.</span><p class="type"><span class="type_family">Research output<span class="type_family_sep">: </span></span><span class="type_classification_parent">Contribution to journal<span class="type_parent_sep"> › </span></span><span class="type_classification">Review Article</span><span class="type_classification"><span class="type_parent_sep"> › </span>Research</span><span class="type_classification"><span class="type_parent_sep"> › </span>peer-review</span></p></div> <div class="rendering rendering_researchoutput rendering_researchoutput_publicationattacheddocumentsportalrenderer rendering_contributiontojournal rendering_publicationattacheddocumentsportalrenderer rendering_contributiontojournal_publicationattacheddocumentsportalrenderer"><div class="open-access">Open Access</div><div class="files">File</div></div> </div> <div class="publication-metrics" aria-label="Publication metrics section"> <div class="metrics-container"> <div class="metrics-wrap metrics-top one"> <div class="metric scopus-citations"> <a target="_blank" href="http://www.scopus.com/inward/citedby.url?scp=84959257630&partnerID=8YFLogxK" aria-label="Source: Scopus: 450"> <span class="count">450</span> </a> <span class="label">Citations (Scopus)</span> </div> </div> <div class="metrics-wrap metrics-bottom one"> <div class="metric metric-altmetric"> <div data-badge-popover="top" data-badge-type="donut" data-doi="10.1007/lrr-2016-1" data-hide-no-mentions="true" data-link-target='_blank' class="altmetric-embed"></div> </div> </div> </div> </div> </li> </ul> </div> <div class="footer"> </div> </div> </section> <section class="page-section content-relation-section publication-projects"> <div class="container"> <div class="header"> <h2 class="section-title" id="related-projects-title"> <i class="icon icon-projects" aria-hidden="true"></i> <span class="title"> Projects </span> </h2> <div class="content-trends"> <button rel="toggle-project-chart" data-year-url="/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3/projects/?projectStartYear=" aria-label="Projects per year" class="chart-toggler" aria-expanded="false"> <span class="title"> Projects per year <img src="/assets/gizmo-expand-61f33ba7afaffaa77611abfb62f97a9e.svg" aria-hidden="true" alt="" class="expand" /> <img src="/assets/gizmo-contract-7adbcd523b1972d72d537e479dd74798.svg" aria-hidden="true" alt="" class="contract" /> </span> <span class="inline-trend-graph"> <span class="year year-start">2011</span> <span class="trend-graph-wrapper"> <span class="bar" style="height: 100%;"> <span aria-expanded="false" role="tooltip">2011</span> </span> </span> <span class="year year-end">2018</span> </span> </button> <ul class="content-statistics"> <li class=""> <a class="portal_link count increment-counter" aria-label="1 Finished" href="/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3/projects/?status=FINISHED"><span> 1 </span></a> <span class="label">Finished</span> </li> </ul> <div class="flex-break"></div> <div class="chart-container" id="chart-content-projects-by-year" style="display: none;" aria-hidden="true" tabindex="-1"> <p class="legend">Projects per year</p> <div class="chart-wrapper"> <canvas></canvas> </div> </div> <table id="project-container-table" class="sr-only" aria-hidden="true"></table> <script> $("#chart-content-projects-by-year").contentChart({ toggle: "button[rel='toggle-project-chart']", title: "Projects per year", labels: [2011], values: [1], tableContainer : $('#project-container-table'), }); </script> </div> </div> <div class="relation-list relation-list-projects"> <ul class="list-results"> <li class="list-result-item"> <div class="result-container"> <div class="rendering rendering_upmproject rendering_short rendering_upmproject_short"><h3 class="title"><a rel="UPMProject" href="https://research.monash.edu/en/projects/arc-centre-of-excellence-for-particle-physics-at-the-tera-scale" class="link"><span>ARC Centre of Excellence for Particle Physics at the Tera-Scale</span></a></h3><p><a rel="Person" href="https://research.monash.edu/en/persons/csaba-balazs" class="link person"><span>Balazs, C.</span></a>, Barberio, E., Bell, N., Gherghetta, T., Limosani, A., Sevior, M., Taylor, G., Thomas, A., Varvell, K., Volkas, R., Williams, A. G., Yabsley, B., Young, R. D., Clarke, A., Jakobs, C., Kruse, M., Meroni, C., Parker, M. & Trodden, M.</p><p class="fundings"><a rel="UEOExternalOrganisation" href="#" class="link"><span>Australian Research Council (ARC)</span></a></p><p class="period"><span class="date">1/01/11</span> → <span class="date">31/12/18</span></p><p class="type"><span class="type_family">Project<span class="type_family_sep">: </span></span><span class="type_classification">Research</span></p></div> </div> </li> </ul> </div> <div class="footer"> </div> </div> </section> <section class="page-section cite"> <div class="container"> <section class="publication-cite" aria-labelledby="publications-cite-title"> <h2 class="subheader" id="publications-cite-title">Cite this</h2> <ul class="tabs has-overflow-navigation" role="tablist" aria-label="Cite this"> <li class="selected" role="tab" id="tab-0" aria-controls="cite-apa" tabindex="-1" aria-selected="false" > APA </li> <li class="" role="tab" id="tab-1" aria-controls="cite-author" tabindex="-1" aria-selected="false" > Author </li> <li class="" role="tab" id="tab-2" aria-controls="cite-BIBTEX" tabindex="-1" aria-selected="false" > BIBTEX </li> <li class="" role="tab" id="tab-3" aria-controls="cite-harvard" tabindex="-1" aria-selected="false" > Harvard </li> <li class="" role="tab" id="tab-4" aria-controls="cite-standard" tabindex="-1" aria-selected="false" > Standard </li> <li class="" role="tab" id="tab-5" aria-controls="cite-RIS" tabindex="-1" aria-selected="false" > RIS </li> <li class="" role="tab" id="tab-6" aria-controls="cite-vancouver" tabindex="-1" aria-selected="false" > Vancouver </li> </ul> <div class="tab-container"> <div id="cite-apa" class="tab selected" role="tabpanel" aria-labelledby="tab-0" tabindex="-1" aria-hidden="true"> <div class="rendering rendering_researchoutput rendering_researchoutput_apa rendering_contributiontojournal rendering_apa rendering_contributiontojournal_apa">the KAGRA Collaboration, The LIGO Scientific Collaboration, & Virgo Collaboration (2018). <a rel="ContributionToJournal" href="https://research.monash.edu/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3" class="link"><span>Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA</span></a>. <a rel="Journal" href="#" class="link"><span><em>Living Reviews in Relativity</em></span></a>, <em>21</em>(1), Article 3. <a onclick="window.open(this.href, '_blank','noopener,noreferrer'); return false;" href="https://doi.org/10.1007/s41114-018-0012-9" class="link"><span>https://doi.org/10.1007/s41114-018-0012-9</span></a></div> </div> <div id="cite-author" class="tab " role="tabpanel" aria-labelledby="tab-1" tabindex="-1" aria-hidden="true"> <div class="rendering rendering_researchoutput rendering_researchoutput_author rendering_contributiontojournal rendering_author rendering_contributiontojournal_author">the KAGRA Collaboration ; The LIGO Scientific Collaboration ; Virgo Collaboration. / <a rel="ContributionToJournal" href="https://research.monash.edu/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3" class="link"><span><strong>Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA</strong></span></a>. In: <a rel="Journal" href="#" class="link"><span>Living Reviews in Relativity</span></a>. 2018 ; Vol. 21, No. 1.</div> </div> <div id="cite-BIBTEX" class="tab " role="tabpanel" aria-labelledby="tab-2" tabindex="-1" aria-hidden="true"> <div class="rendering rendering_researchoutput rendering_researchoutput_bibtex rendering_contributiontojournal rendering_bibtex rendering_contributiontojournal_bibtex"><div>@article{6bc15ecfff314b6da655dfab40606543,</div><div> title = "Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA",</div><div> abstract = "We present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron star systems, which are the most promising targets for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90 % credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5–20deg2 requires at least three detectors of sensitivity within a factor of ∼ 2 of each other and with a broad frequency bandwidth. When all detectors, including KAGRA and the third LIGO detector in India, reach design sensitivity, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.",</div><div> keywords = "Data analysis, Electromagnetic counterparts, Gravitational waves, Gravitational-wave detectors",</div><div> author = "Abbott, {B. P.} and R. Abbott and Abbott, {T. D.} and Abernathy, {M. R.} and F. Acernese and K. Ackley and C. Adams and T. Adams and P. Addesso and Adhikari, {R. X.} and Adya, {V. B.} and C. Affeldt and M. Agathos and K. Agatsuma and N. Aggarwal and Aguiar, {O. D.} and L. Aiello and A. Ain and P. Ajith and T. Akutsu and B. Allen and A. Allocca and Altin, {P. A.} and A. Ananyeva and Anderson, {S. B.} and Anderson, {W. G.} and M. Ando and S. Appert and K. Arai and A. Araya and Araya, {M. C.} and Areeda, {J. S.} and N. Arnaud and Arun, {K. G.} and H. Asada and S. Ascenzi and G. Ashton and Y. Aso and M. Ast and Aston, {S. M.} and P. Astone and S. Atsuta and P. Aufmuth and C. Aulbert and A. Avila-Alvarez and K. Awai and S. Babak and P. Bacon and Bader, {M. K.M.} and L. Baiotti and Baker, {P. T.} and F. Baldaccini and G. Ballardin and Ballmer, {S. W.} and Barayoga, {J. C.} and Barclay, {S. E.} and Barish, {B. C.} and D. Barker and F. Barone and B. Barr and L. Barsotti and M. Barsuglia and D. Barta and J. Bartlett and Barton, {M. A.} and I. Bartos and R. Bassiri and A. Basti and Batch, {J. C.} and C. Baune and V. Bavigadda and M. Bazzan and B. B{\'e}csy and C. Beer and M. Bejger and I. Belahcene and M. Belgin and Bell, {A. S.} and Berger, {B. K.} and G. Bergmann and Berry, {C. P.L.} and D. Bersanetti and A. Bertolini and J. Betzwieser and S. Bhagwat and R. Bhandare and Bilenko, {I. A.} and G. Billingsley and Billman, {C. R.} and J. Birch and R. Birney and O. Birnholtz and S. Biscans and A. Bisht and M. Bitossi and C. Biwer and Bizouard, {M. A.} and Blackburn, {J. K.} and J. Blackman and Blair, {C. D.} and Blair, {D. G.} and Blair, {R. M.} and S. Bloemen and O. Bock and M. Boer and G. Bogaert and A. Bohe and F. Bondu and R. Bonnand and Boom, {B. A.} and R. Bork and V. Boschi and S. Bose and Y. Bouffanais and A. Bozzi and C. Bradaschia and Brady, {P. R.} and Braginsky, {V. B.} and M. Branchesi and Brau, {J. E.} and T. Briant and A. Brillet and M. Brinkmann and V. Brisson and P. Brockill and Broida, {J. E.} and Brooks, {A. F.} and Brown, {D. A.} and Brown, {D. D.} and Brown, {N. M.} and S. Brunett and Buchanan, {C. C.} and A. Buikema and T. Bulik and Bulten, {H. J.} and A. Buonanno and D. Buskulic and C. Buy and Byer, {R. L.} and M. Cabero and L. Cadonati and G. Cagnoli and C. Cahillane and J. Calder{\'o}n Bustillo and Callister, {T. A.} and E. Calloni and Camp, {J. B.} and Cannon, {K. C.} and H. Cao and J. Cao and Capano, {C. D.} and E. Capocasa and F. Carbognani and S. Caride and J. Casanueva Diaz and C. Casentini and S. Caudill and M. Cavagli{\`a} and F. Cavalier and R. Cavalieri and G. Cella and Cepeda, {C. B.} and L. Cerboni Baiardi and G. Cerretani and E. Cesarini and Chamberlin, {S. J.} and M. Chan and S. Chao and P. Charlton and E. Chassande-Mottin and Cheeseboro, {B. D.} and Chen, {H. Y.} and Y. Chen and Cheng, {H. P.} and A. Chincarini and A. Chiummo and T. Chmiel and Cho, {H. S.} and M. Cho and Chow, {J. H.} and N. Christensen and Q. Chu and Chua, {A. J.K.} and S. Chua and S. Chung and G. Ciani and F. Clara and Clark, {J. A.} and F. Cleva and C. Cocchieri and E. Coccia and Cohadon, {P. F.} and A. Colla and Collette, {C. G.} and L. Cominsky and M. Constancio and L. Conti and Cooper, {S. J.} and Corbitt, {T. R.} and N. Cornish and A. Corsi and S. Cortese and Costa, {C. A.} and Coughlin, {M. W.} and Coughlin, {S. B.} and Coulon, {J. P.} and Countryman, {S. T.} and P. Couvares and Covas, {P. B.} and Cowan, {E. E.} and Coward, {D. M.} and Cowart, {M. J.} and Coyne, {D. C.} and R. Coyne and Creighton, {J. D.E.} and Creighton, {T. D.} and J. Cripe and Crowder, {S. G.} and Cullen, {T. J.} and A. Cumming and L. Cunningham and E. Cuoco and Canton, {T. Dal} and Danilishin, {S. L.} and S. D{\textquoteright}Antonio and K. Danzmann and A. Dasgupta and {Da Silva Costa}, {C. F.} and V. Dattilo and I. Dave and M. Davier and Davies, {G. S.} and D. Davis and Daw, {E. J.} and B. Day and R. Day and S. De and D. DeBra and G. Debreczeni and J. Degallaix and {De Laurentis}, M. and S. Del{\'e}glise and {Del Pozzo}, W. and T. Denker and T. Dent and V. Dergachev and Lasky, {P D} and Y Levin and S. Qiu and L. Sammut and Smith, {R. J.E.} and E Thrane and C Whittle and Zhu, {X. J.} and {the KAGRA Collaboration} and {The LIGO Scientific Collaboration} and {Virgo Collaboration}",</div><div> year = "2018",</div><div> month = dec,</div><div> day = "1",</div><div> doi = "10.1007/s41114-018-0012-9",</div><div> language = "English",</div><div> volume = "21",</div><div> journal = "Living Reviews in Relativity",</div><div> issn = "1433-8351",</div><div> publisher = "SpringerOpen",</div><div> number = "1",</div><p>}</p></div> </div> <div id="cite-harvard" class="tab " role="tabpanel" aria-labelledby="tab-3" tabindex="-1" aria-hidden="true"> <div class="rendering rendering_researchoutput rendering_researchoutput_harvard rendering_contributiontojournal rendering_harvard rendering_contributiontojournal_harvard">the KAGRA Collaboration, The LIGO Scientific Collaboration & Virgo Collaboration 2018, '<a rel="ContributionToJournal" href="https://research.monash.edu/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3" class="link harvard_title"><span>Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA</span></a>', <a rel="Journal" href="#" class="link"><span><em>Living Reviews in Relativity</em></span></a>, vol. 21, no. 1, 3. <a onclick="window.open(this.href, '_blank','noopener,noreferrer'); return false;" href="https://doi.org/10.1007/s41114-018-0012-9" class="link"><span>https://doi.org/10.1007/s41114-018-0012-9</span></a></div> </div> <div id="cite-standard" class="tab " role="tabpanel" aria-labelledby="tab-4" tabindex="-1" aria-hidden="true"> <div class="rendering rendering_researchoutput rendering_researchoutput_standard rendering_contributiontojournal rendering_standard rendering_contributiontojournal_standard"><a rel="ContributionToJournal" href="https://research.monash.edu/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3" class="link"><span><strong>Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA.</strong></span></a> / the KAGRA Collaboration; The LIGO Scientific Collaboration; Virgo Collaboration. <br />In: <a rel="Journal" href="#" class="link"><span>Living Reviews in Relativity</span></a>, Vol. 21, No. 1, 3, 01.12.2018.<p class="type"><span class="type_family">Research output<span class="type_family_sep">: </span></span><span class="type_classification_parent">Contribution to journal<span class="type_parent_sep"> › </span></span><span class="type_classification">Review Article</span><span class="type_classification"><span class="type_parent_sep"> › </span>Other</span><span class="type_classification"><span class="type_parent_sep"> › </span>peer-review</span></p></div> </div> <div id="cite-RIS" class="tab " role="tabpanel" aria-labelledby="tab-5" tabindex="-1" aria-hidden="true"> <div class="rendering rendering_researchoutput rendering_researchoutput_ris rendering_contributiontojournal rendering_ris rendering_contributiontojournal_ris"><p>TY - JOUR</p><p>T1 - Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA</p><p>AU - Abbott, B. P.</p><p>AU - Abbott, R.</p><p>AU - Abbott, T. D.</p><p>AU - Abernathy, M. R.</p><p>AU - Acernese, F.</p><p>AU - Ackley, K.</p><p>AU - Adams, C.</p><p>AU - Adams, T.</p><p>AU - Addesso, P.</p><p>AU - Adhikari, R. X.</p><p>AU - Adya, V. B.</p><p>AU - Affeldt, C.</p><p>AU - Agathos, M.</p><p>AU - Agatsuma, K.</p><p>AU - Aggarwal, N.</p><p>AU - Aguiar, O. D.</p><p>AU - Aiello, L.</p><p>AU - Ain, A.</p><p>AU - Ajith, P.</p><p>AU - Akutsu, T.</p><p>AU - Allen, B.</p><p>AU - Allocca, A.</p><p>AU - Altin, P. A.</p><p>AU - Ananyeva, A.</p><p>AU - Anderson, S. B.</p><p>AU - Anderson, W. G.</p><p>AU - Ando, M.</p><p>AU - Appert, S.</p><p>AU - Arai, K.</p><p>AU - Araya, A.</p><p>AU - Araya, M. C.</p><p>AU - Areeda, J. S.</p><p>AU - Arnaud, N.</p><p>AU - Arun, K. G.</p><p>AU - Asada, H.</p><p>AU - Ascenzi, S.</p><p>AU - Ashton, G.</p><p>AU - Aso, Y.</p><p>AU - Ast, M.</p><p>AU - Aston, S. M.</p><p>AU - Astone, P.</p><p>AU - Atsuta, S.</p><p>AU - Aufmuth, P.</p><p>AU - Aulbert, C.</p><p>AU - Avila-Alvarez, A.</p><p>AU - Awai, K.</p><p>AU - Babak, S.</p><p>AU - Bacon, P.</p><p>AU - Bader, M. K.M.</p><p>AU - Baiotti, L.</p><p>AU - Baker, P. T.</p><p>AU - Baldaccini, F.</p><p>AU - Ballardin, G.</p><p>AU - Ballmer, S. W.</p><p>AU - Barayoga, J. C.</p><p>AU - Barclay, S. E.</p><p>AU - Barish, B. C.</p><p>AU - Barker, D.</p><p>AU - Barone, F.</p><p>AU - Barr, B.</p><p>AU - Barsotti, L.</p><p>AU - Barsuglia, M.</p><p>AU - Barta, D.</p><p>AU - Bartlett, J.</p><p>AU - Barton, M. A.</p><p>AU - Bartos, I.</p><p>AU - Bassiri, R.</p><p>AU - Basti, A.</p><p>AU - Batch, J. C.</p><p>AU - Baune, C.</p><p>AU - Bavigadda, V.</p><p>AU - Bazzan, M.</p><p>AU - Bécsy, B.</p><p>AU - Beer, C.</p><p>AU - Bejger, M.</p><p>AU - Belahcene, I.</p><p>AU - Belgin, M.</p><p>AU - Bell, A. S.</p><p>AU - Berger, B. K.</p><p>AU - Bergmann, G.</p><p>AU - Berry, C. P.L.</p><p>AU - Bersanetti, D.</p><p>AU - Bertolini, A.</p><p>AU - Betzwieser, J.</p><p>AU - Bhagwat, S.</p><p>AU - Bhandare, R.</p><p>AU - Bilenko, I. A.</p><p>AU - Billingsley, G.</p><p>AU - Billman, C. R.</p><p>AU - Birch, J.</p><p>AU - Birney, R.</p><p>AU - Birnholtz, O.</p><p>AU - Biscans, S.</p><p>AU - Bisht, A.</p><p>AU - Bitossi, M.</p><p>AU - Biwer, C.</p><p>AU - Bizouard, M. A.</p><p>AU - Blackburn, J. K.</p><p>AU - Blackman, J.</p><p>AU - Blair, C. D.</p><p>AU - Blair, D. G.</p><p>AU - Blair, R. M.</p><p>AU - Bloemen, S.</p><p>AU - Bock, O.</p><p>AU - Boer, M.</p><p>AU - Bogaert, G.</p><p>AU - Bohe, A.</p><p>AU - Bondu, F.</p><p>AU - Bonnand, R.</p><p>AU - Boom, B. A.</p><p>AU - Bork, R.</p><p>AU - Boschi, V.</p><p>AU - Bose, S.</p><p>AU - Bouffanais, Y.</p><p>AU - Bozzi, A.</p><p>AU - Bradaschia, C.</p><p>AU - Brady, P. R.</p><p>AU - Braginsky, V. B.</p><p>AU - Branchesi, M.</p><p>AU - Brau, J. E.</p><p>AU - Briant, T.</p><p>AU - Brillet, A.</p><p>AU - Brinkmann, M.</p><p>AU - Brisson, V.</p><p>AU - Brockill, P.</p><p>AU - Broida, J. E.</p><p>AU - Brooks, A. F.</p><p>AU - Brown, D. A.</p><p>AU - Brown, D. D.</p><p>AU - Brown, N. M.</p><p>AU - Brunett, S.</p><p>AU - Buchanan, C. C.</p><p>AU - Buikema, A.</p><p>AU - Bulik, T.</p><p>AU - Bulten, H. J.</p><p>AU - Buonanno, A.</p><p>AU - Buskulic, D.</p><p>AU - Buy, C.</p><p>AU - Byer, R. L.</p><p>AU - Cabero, M.</p><p>AU - Cadonati, L.</p><p>AU - Cagnoli, G.</p><p>AU - Cahillane, C.</p><p>AU - Calderón Bustillo, J.</p><p>AU - Callister, T. A.</p><p>AU - Calloni, E.</p><p>AU - Camp, J. B.</p><p>AU - Cannon, K. C.</p><p>AU - Cao, H.</p><p>AU - Cao, J.</p><p>AU - Capano, C. D.</p><p>AU - Capocasa, E.</p><p>AU - Carbognani, F.</p><p>AU - Caride, S.</p><p>AU - Casanueva Diaz, J.</p><p>AU - Casentini, C.</p><p>AU - Caudill, S.</p><p>AU - Cavaglià, M.</p><p>AU - Cavalier, F.</p><p>AU - Cavalieri, R.</p><p>AU - Cella, G.</p><p>AU - Cepeda, C. B.</p><p>AU - Cerboni Baiardi, L.</p><p>AU - Cerretani, G.</p><p>AU - Cesarini, E.</p><p>AU - Chamberlin, S. J.</p><p>AU - Chan, M.</p><p>AU - Chao, S.</p><p>AU - Charlton, P.</p><p>AU - Chassande-Mottin, E.</p><p>AU - Cheeseboro, B. D.</p><p>AU - Chen, H. Y.</p><p>AU - Chen, Y.</p><p>AU - Cheng, H. P.</p><p>AU - Chincarini, A.</p><p>AU - Chiummo, A.</p><p>AU - Chmiel, T.</p><p>AU - Cho, H. S.</p><p>AU - Cho, M.</p><p>AU - Chow, J. H.</p><p>AU - Christensen, N.</p><p>AU - Chu, Q.</p><p>AU - Chua, A. J.K.</p><p>AU - Chua, S.</p><p>AU - Chung, S.</p><p>AU - Ciani, G.</p><p>AU - Clara, F.</p><p>AU - Clark, J. A.</p><p>AU - Cleva, F.</p><p>AU - Cocchieri, C.</p><p>AU - Coccia, E.</p><p>AU - Cohadon, P. F.</p><p>AU - Colla, A.</p><p>AU - Collette, C. G.</p><p>AU - Cominsky, L.</p><p>AU - Constancio, M.</p><p>AU - Conti, L.</p><p>AU - Cooper, S. J.</p><p>AU - Corbitt, T. R.</p><p>AU - Cornish, N.</p><p>AU - Corsi, A.</p><p>AU - Cortese, S.</p><p>AU - Costa, C. A.</p><p>AU - Coughlin, M. W.</p><p>AU - Coughlin, S. B.</p><p>AU - Coulon, J. P.</p><p>AU - Countryman, S. T.</p><p>AU - Couvares, P.</p><p>AU - Covas, P. B.</p><p>AU - Cowan, E. E.</p><p>AU - Coward, D. M.</p><p>AU - Cowart, M. J.</p><p>AU - Coyne, D. C.</p><p>AU - Coyne, R.</p><p>AU - Creighton, J. D.E.</p><p>AU - Creighton, T. D.</p><p>AU - Cripe, J.</p><p>AU - Crowder, S. G.</p><p>AU - Cullen, T. J.</p><p>AU - Cumming, A.</p><p>AU - Cunningham, L.</p><p>AU - Cuoco, E.</p><p>AU - Canton, T. Dal</p><p>AU - Danilishin, S. L.</p><p>AU - D’Antonio, S.</p><p>AU - Danzmann, K.</p><p>AU - Dasgupta, A.</p><p>AU - Da Silva Costa, C. F.</p><p>AU - Dattilo, V.</p><p>AU - Dave, I.</p><p>AU - Davier, M.</p><p>AU - Davies, G. S.</p><p>AU - Davis, D.</p><p>AU - Daw, E. J.</p><p>AU - Day, B.</p><p>AU - Day, R.</p><p>AU - De, S.</p><p>AU - DeBra, D.</p><p>AU - Debreczeni, G.</p><p>AU - Degallaix, J.</p><p>AU - De Laurentis, M.</p><p>AU - Deléglise, S.</p><p>AU - Del Pozzo, W.</p><p>AU - Denker, T.</p><p>AU - Dent, T.</p><p>AU - Dergachev, V.</p><p>AU - Lasky, P D</p><p>AU - Levin, Y</p><p>AU - Qiu, S.</p><p>AU - Sammut, L.</p><p>AU - Smith, R. J.E.</p><p>AU - Thrane, E</p><p>AU - Whittle, C</p><p>AU - Zhu, X. J.</p><p>AU - the KAGRA Collaboration</p><p>AU - The LIGO Scientific Collaboration</p><p>AU - Virgo Collaboration</p><p>PY - 2018/12/1</p><p>Y1 - 2018/12/1</p><p>N2 - We present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron star systems, which are the most promising targets for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90 % credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5–20deg2 requires at least three detectors of sensitivity within a factor of ∼ 2 of each other and with a broad frequency bandwidth. When all detectors, including KAGRA and the third LIGO detector in India, reach design sensitivity, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.</p><p>AB - We present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron star systems, which are the most promising targets for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90 % credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5–20deg2 requires at least three detectors of sensitivity within a factor of ∼ 2 of each other and with a broad frequency bandwidth. When all detectors, including KAGRA and the third LIGO detector in India, reach design sensitivity, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.</p><p>KW - Data analysis</p><p>KW - Electromagnetic counterparts</p><p>KW - Gravitational waves</p><p>KW - Gravitational-wave detectors</p><p>UR - http://www.scopus.com/inward/record.url?scp=85046034556&partnerID=8YFLogxK</p><p>U2 - 10.1007/s41114-018-0012-9</p><p>DO - 10.1007/s41114-018-0012-9</p><p>M3 - Review Article</p><p>AN - SCOPUS:85046034556</p><p>SN - 1433-8351</p><p>VL - 21</p><p>JO - Living Reviews in Relativity</p><p>JF - Living Reviews in Relativity</p><p>IS - 1</p><p>M1 - 3</p><p>ER - </p></div> </div> <div id="cite-vancouver" class="tab " role="tabpanel" aria-labelledby="tab-6" tabindex="-1" aria-hidden="true"> <div class="rendering rendering_researchoutput rendering_researchoutput_vancouver rendering_contributiontojournal rendering_vancouver rendering_contributiontojournal_vancouver">the KAGRA Collaboration, The LIGO Scientific Collaboration, Virgo Collaboration. <span class="title"><a rel="ContributionToJournal" href="https://research.monash.edu/en/publications/prospects-for-observing-and-localizing-gravitational-wave-transie-3" class="link"><span>Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA</span></a></span>. <a rel="Journal" href="#" class="link"><span>Living Reviews in Relativity</span></a>. 2018 Dec 1;21(1):3. doi: 10.1007/s41114-018-0012-9</div> </div> <script> $(function() { $(".tab-container .rendering a:not([href^='http://dx.doi.org'])").contents().unwrap(); 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Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA - Monash University