Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/101199
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dc.contributor.authorAbbott, B.P.-
dc.contributor.authorLIGO Scientific Collaboration-
dc.contributor.authorVirgo Collaboration-
dc.contributor.authorAbbott, R.-
dc.contributor.authorAbbott, T.D.-
dc.contributor.authorAbernathy, M.R.-
dc.contributor.authorAcernese, F.-
dc.contributor.authorAckley, K.-
dc.contributor.authorAdams, C.-
dc.contributor.authorAdams, T.-
dc.contributor.authorAddesso, P.-
dc.contributor.authorAdhikari, R.X.-
dc.contributor.authorAdya, V.B.-
dc.contributor.authorAffeldt, C.-
dc.contributor.authorAgathos, M.-
dc.contributor.authorAgatsuma, K.-
dc.contributor.authorAggarwal, N.-
dc.contributor.authorAguiar, O.D.-
dc.contributor.authorAiello, L.-
dc.contributor.authorAin, A.-
dc.contributor.authoret al.-
dc.date.issued2016-
dc.identifier.citationPhysical Review D: Particles, Fields, Gravitation and Cosmology, 2016; 93(12):122004-1-122004-20-
dc.identifier.issn1550-7998-
dc.identifier.issn1550-2368-
dc.identifier.urihttp://hdl.handle.net/2440/101199-
dc.descriptionPublished 7 June 2016-
dc.description.abstractThe gravitational-wave signal GW150914 was first identified on September 14, 2015, by searches for short-duration gravitational-wave transients. These searches identify time-correlated transients in multiple detectors with minimal assumptions about the signal morphology, allowing them to be sensitive to gravitational waves emitted by a wide range of sources including binary black hole mergers. Over the observational period from September 12 to October 20, 2015, these transient searches were sensitive to binary black hole mergers similar to GW150914 to an average distance of ∼600  Mpc. In this paper, we describe the analyses that first detected GW150914 as well as the parameter estimation and waveform reconstruction techniques that initially identified GW150914 as the merger of two black holes. We find that the reconstructed waveform is consistent with the signal from a binary black hole merger with a chirp mass of ∼30  M⊙ and a total mass before merger of ∼70  M⊙ in the detector frame.-
dc.description.statementofresponsibilityB. P. Abbott ... S. E. Hollitt ... D. J. Hosken ... E. J. King ... J. Munch ... D. J. Ottaway ... P. J. Veitch ... et al. (The LIGO Scientific Collaboration and the Virgo Collaboration)-
dc.language.isoen-
dc.publisherAmerican Physical Society-
dc.rights© 2016 American Physical Society-
dc.titleObserving gravitational-wave transient GW150914 with minimal assumptions-
dc.typeJournal article-
dc.identifier.doi10.1103/PhysRevD.93.122004-
dc.relation.grantARC-
pubs.publication-statusPublished-
Appears in Collections:Aurora harvest 3
IPAS publications

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