dc.creatorAbbot, B. P.
dc.creatorGalbany, Lluis
dc.creatorRazza, A.
dc.date.accessioned2017-03-28T20:37:03Z
dc.date.accessioned2019-04-26T01:12:01Z
dc.date.available2017-03-28T20:37:03Z
dc.date.available2019-04-26T01:12:01Z
dc.date.created2017-03-28T20:37:03Z
dc.date.issued2016
dc.identifierThe Astrophysical Journal Supplement Series, 225:8 (15pp), 2016 July
dc.identifier10.3847/0067-0049/225/1/8
dc.identifierhttp://repositorio.uchile.cl/handle/2250/143363
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/2447446
dc.description.abstractThis Supplement provides supporting material for Abbott et al. (2016a). We briefly summarize past electromagnetic (EM) follow-up efforts as well as the organization and policy of the current EM follow-up program. We compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow-up observations that were performed in the different bands
dc.languageen
dc.publisherIOP
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
dc.sourceThe Astrophysical Journal Supplement Series
dc.subjectGravitational waves
dc.subjectMethods: observational
dc.titleSupplement: " Localization and Broadband Follow-Up of the Gravitational-Wave Transient GW150914” (2016, ApJL, 826, L13)
dc.typeArtículos de revistas


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