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Constraining possible \(\gamma\)-ray burst emission from GW230529 using Swift-BAT and Fermi-GBM

Constraining possible \(\gamma\)-ray burst emission from GW230529 using Swift-BAT and Fermi-GBM

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3056925855

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

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Scope and Contents

Contents

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\(M_{\odot}\). If interpreted as a neutron star-black hole merger, this event has the most symmetric mass ratio detected so far and therefore has a relative...

Alternative Titles

Full title

Constraining possible \(\gamma\)-ray burst emission from GW230529 using Swift-BAT and Fermi-GBM

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Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_3056925855

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3056925855

Other Identifiers

E-ISSN

2331-8422

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