Constraining Possible γ-Ray Burst Emission from GW230529 Using Swift-BAT and Fermi-GBM

GW230529 is the first compact binary coalescence detected by the LIGO–Virgo–KAGRA collaboration with at least one component mass confidently in the lower mass gap, corresponding to the range 3–5 M _⊙ . If interpreted as a neutron star–black hole merger, this event has the most symmetric mass ratio d...

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मुख्य लेखकों:	Samuele Ronchini, Suman Bala, Joshua Wood, James Delaunay, Simone Dichiara, Jamie A. Kennea, Tyler Parsotan, Gayathri Raman, Aaron Tohuvavohu, Naresh Adhikari, Narayana P. Bhat, Sylvia Biscoveanu, Elisabetta Bissaldi, Eric Burns, Sergio Campana, Koustav Chandra, William H. Cleveland, Sarah Dalessi, Massimiliano De Pasquale, Juan García-Bellido, Claudio Gasbarra, Misty M. Giles, Ish Gupta, Dieter Hartmann, Boyan A. Hristov, Michelle C. Hui, Rahul Kashyap, Daniel Kocevski, Bagrat Mailyan, Christian Malacaria, Hiroyuki Nakano, Giacomo Principe, Oliver J. Roberts, Bangalore Sathyaprakash, Lijing Shao, Eleonora Troja, Péter Veres, Colleen A. Wilson-Hodge
स्वरूप:	Artigo
भाषा:	Inglês
प्रकाशित:	IOP Publishing 2024-01-01
श्रृंखला:	The Astrophysical Journal Letters
विषय:	High energy astrophysics Gamma-ray astronomy Gamma-ray bursts Gravitational waves
ऑनलाइन पहुंच:	https://doi.org/10.3847/2041-8213/ad5d74
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