PARAMETER ESTIMATION FOR BINARY NEUTRON-STAR COALESCENCES WITH REALISTIC NOISE DURING THE ADVANCED LIGO ERA

PARAMETER ESTIMATION FOR BINARY NEUTRON-STAR COALESCENCES WITH REALISTIC NOISE DURING THE ADVANCED LIGO ERA

Advanced ground-based gravitational-wave (GW) detectors begin operation imminently. Their intended goal is not only to make the first direct detection of GWs, but also to make inferences about the source systems. Binary neutron-star mergers are among the most promising sources. We investigate the pe...

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Bibliographic Details
Main Authors: Berry, Christopher P. L. (Author), Mandel, Ilya (Author), Middleton, Hannah (Author), Singer, Leo P. (Author), Urban, Alex L. (Author), Vecchio, Alberto (Author), Vitale, Salvatore (Contributor), Cannon, Kipp (Author), Farr, Ben (Author), Farr, Will M. (Author), Graff, Philip B. (Author), Hanna, Chad (Author), Haster, Carl-Johan (Author), Pankow, Chris (Author), Price, Larry R. (Author), Sidery, Trevor (Author), Veitch, John (Author), Ray Pitambar Mohapatra, Satyanarayan (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), Mohapatra, Satya (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-09-01T20:22:52Z.
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