The Broadband Counterpart of the Short GRB 200522A at z = 0.5536: A Luminous Kilonova or a Collimated Outflow with a Reverse Shock?-Reference-Cited by-同舟云学术

The Broadband Counterpart of the Short GRB 200522A at z = 0.5536: A Luminous Kilonova or a Collimated Outflow with a Reverse Shock?

Published:2021-01-15 Issue:2 Volume:906 Page:127
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Fong W.^ORCID,Laskar T.^ORCID,Rastinejad J.^ORCID,Escorial A. Rouco^ORCID,Schroeder G.^ORCID,Barnes J.^ORCID,Kilpatrick C. D.^ORCID,Paterson K.^ORCID,Berger E.^ORCID,Metzger B. D.^ORCID,Dong Y.^ORCID,Nugent A. E.^ORCID,Strausbaugh R.^ORCID,Blanchard P. K.^ORCID,Goyal A.^ORCID,Cucchiara A.,Terreran G.^ORCID,Alexander K. D.^ORCID,Eftekhari T.^ORCID,Fryer C.^ORCID,Margalit B.^ORCID,Margutti R.^ORCID,Nicholl M.^ORCID

Funder

National Science Foundation

Space Telescope Science Institute

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/abc74a/pdf

Reference234 articles.

1. Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

2. Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA