The panchromatic afterglow of GW170817: the full uniform data set, modeling, comparison with previous results, and implications
S Makhathini, KP Mooley, M Brightman… - The Astrophysical …, 2021 - iopscience.iop.org
We present the full panchromatic afterglow light-curve data of GW170817, including new
radio data as well as archival optical and X-ray data, between 0.5 and 940 days post …
radio data as well as archival optical and X-ray data, between 0.5 and 940 days post …
Afterglow constraints on the viewing angle of binary neutron star mergers and determination of the Hubble constant
One of the key properties of any binary is its viewing angle (ie, inclination), θ obs. In binary
neutron star (BNS) mergers it is of special importance due to the role that it plays in the …
neutron star (BNS) mergers it is of special importance due to the role that it plays in the …
The potential role of binary neutron star merger afterglows in multimessenger cosmology
S Mastrogiovanni, R Duque… - Astronomy & …, 2021 - aanda.org
Binary neutron star mergers offer a new and independent means of measuring the Hubble
constant H 0 by combining the gravitational-wave inferred source luminosity distance with its …
constant H 0 by combining the gravitational-wave inferred source luminosity distance with its …