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dc.rights.license© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society-
dc.contributor.authorKostrzewa Rutkowska, Z.-
dc.contributor.authorJonker, P. G.-
dc.contributor.authorHodgkin, S. T.-
dc.contributor.authorEappachen, D.-
dc.contributor.authorHarrison, D. L.-
dc.contributor.authorKoposov, S. E.-
dc.contributor.authorRixon, G.-
dc.contributor.authorWyrzykowski, L.-
dc.contributor.authorYoldas, A.-
dc.contributor.authorBreedt, E.-
dc.contributor.authorDelgado, A.-
dc.contributor.authorVan Leeuwen, M.-
dc.contributor.authorWevers, T.-
dc.contributor.authorBurgess, P. W.-
dc.contributor.authorDe Angeli, D.-
dc.contributor.authorEvans, D. W.-
dc.contributor.authorOsborne, Paul-
dc.contributor.authorRiello, M.-
dc.contributor.otherUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737-
dc.date.accessioned2021-04-09T10:57:02Z-
dc.date.available2021-04-09T10:57:02Z-
dc.date.issued2020-02-13-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society 493(3): 3264–3273(2020)es
dc.identifier.issn0035-8711-
dc.identifier.otherhttps://academic.oup.com/mnras/article/493/3/3264/5735445-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/206-
dc.descriptionhttps://gaia.esac.esa.int/gost/ The GOST only provides a forecast of the time when targets cross the Gaia Focal Plane based on the scanning law of Gaia. However, it does not take into account operational activities preventing nominal observations nor the gaps between CCDs on the Focal Plane. Hence, the real number of scans may differ from the predictions.es
dc.description.abstractThe recent discoveries of gravitational wave events and in one case also its electromagnetic (EM) counterpart allow us to study the Universe in a novel way. The increased sensitivity of the LIGO and Virgo detectors has opened the possibility for regular detections of EM transient events from mergers of stellar remnants. Gravitational wave sources are expected to have sky localization up to a few hundred square degrees, thus Gaia as an all-sky multi-epoch photometric survey has the potential to be a good tool to search for the EM counterparts. In this paper, we study the possibility of detecting EM counterparts to gravitational wave sources using the Gaia Science Alerts system. We develop an extension to current used algorithms to find transients and test its capabilities in discovering candidate transients on a sample of events from the observation periods O1 and O2 of LIGO and Virgo. For the gravitational wave events from the current run O3, we expect that about 16 (25) per cent should fall in sky regions observed by Gaia 7 (10) d after gravitational wave. The new algorithm will provide about 21 candidates per day from the whole sky.es
dc.description.sponsorshipZKR acknowledges funding from the Netherlands Research School for Astronomy (NOVA). ZKR, PGJ, and DE acknowledge support from European Research Council Consolidator Grant 647208. LW acknowledges Polish NCN HARMONIA grant No. 2018/30/M/ST9/00311. TWis funded in part by European Research Council grant 320360 and by European Commission grant 730980. This publication is based upon work from COST Action MW-Gaia CA18104 supported by COST (European Cooperation in Science and Technology). Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for HighPerformance Computing at the University of Utah. The SDSS web site is www.sdss.org.SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofisica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut fur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-Planck-Institut fur Astrophysik (MPA Garching), Max-Planck-Institut fur Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatario Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University. The Pan-STARRS1 Surveys (PS1) and the PS1 public science archive have been made possible through contributions by the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, the Queen's University Belfast, the HarvardSmithsonian Center forAstrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science FoundationGrant No. AST-1238877, theUniversity of Maryland, Eotvos Lorand University (ELTE), the Los Alamos National Laboratory, and the Gordon and Betty Moore Foundation;With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737).es
dc.language.isoenges
dc.publisherOxford Academics: Blackwell Publishinges
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectGravitational waveses
dc.subjectTransientses
dc.subjectMethods: observationales
dc.subjectSurveyses
dc.titleElectromagnetic counterparts to gravitational wave events from Gaiaes
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcidKoposov, S. E. [0000-0003-2644-135X]-
dc.contributor.orcidHarrison, D. [0000-0001-8687-6588]-
dc.contributor.orcidWyrzykowski, L. [0000-0002-9658-6151]-
dc.contributor.orcidKoposov, S. [0000-0003-2644-135X]-
dc.contributor.orcidBreedt, E. [0000-0001-6180-3438]-
dc.identifier.doi10.1093/mnras/staa436-
dc.identifier.e-issn1365-2966-
dc.contributor.funderEuropean Research Council (ERC)-
dc.contributor.funderNational Science Centre, Poland (NCN)-
dc.contributor.funderEuropean Commission (EC)-
dc.contributor.funderNational Aeronautics and Space Administration (NASA)-
dc.description.peerreviewedPeer reviewes
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501-
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/FP7/320360-
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/H2020/647208-
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