GW170814: A three-detector observation of gravitational waves from a binary black hole coalescence
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Cites background or methods or result from "GW170814: A three-detector observat..."
...We evaluate the distance to the host galaxy from the ratio of the Hubble flow velocity of the host 3017 166 km s 1 - (Abbott et al. 2017g) and two current measurements of the Hubble constant (Ade et al. 2016; Riess et al. 2016)....
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...GW170817 is a GW signal from the inspiral of two low-mass compact objects and is the first GW observation consistent with a BNS coalescence (Abbott et al. 2017e, 2017f)....
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...The figure also contains the 90% credible region of the gravitational masses obtained with a restricted or full spin prior (Abbott et al. 2017e)....
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...The detection of GW170817 triggered a campaign of EM follow-up observations which led to the identification of NGC 4993 as the host galaxy of GW170817/GRB170817A (Coulter et al. 2017a, 2017b; Abbott et al. 2017f)....
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...The second coherent search does not assume any particular GW morphology or GRB model (Sutton et al. 2010; Was et al. 2012; Abbott et al. 2017b) and uses the GBM localization of GRB170817A to constrain the sky location of the source....
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Cites background from "GW170814: A three-detector observat..."
...GW170818 is the second BBH observed in triple-coincidence between the two LIGO observatories and Virgo after GW170814 [16]....
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...PE results for four O2 events have been provided for GW170104 in [15], for GW170608 in [17], for GW170814 in [16] and for GW170817 in [18, 95]....
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...Three binary black hole events from O2 have already been published: GW170104 [15], GW170608 [17], and GW170814 [16]....
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...A similar impact of Virgo on the sky localization was already seen for GW170814 [16], reaffirming the importance of a global GW detector network for accurately localizing GW sources [198]....
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...Of these eleven events, seven have been previously reported: the three gravitational-wave events from O1 [1–4]; and from O2, the binary neutron star merger GW170817 [18], and the binary black hole events GW170104 [15], GW170608 [17], and GW170814 [16]....
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References
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