We present Fermi Gamma-ray Burst Monitor (Fermi-GBM) and Swift Burst Alert Telescope (Swift-BAT) searches for gamma-ray/X-ray counterparts to gravitational-wave (GW) candidate events identified during the third observing run of the Advanced LIGO and Advanced Virgo detectors. Using Fermi-GBM onboard triggers and subthreshold gamma-ray burst (GRB) candidates found in the Fermi-GBM ground analyses, the Targeted Search and the Untargeted Search, we investigate whether there are any coincident GRBs associated with the GWs. We also search the Swift-BAT rate data around the GW times to determine whether a GRB counterpart is present. No counterparts are found. Using both the Fermi-GBM Targeted Search and the Swift-BAT search, we calculate flux upper limits and present joint upper limits on the gamma-ray luminosity of each GW. Given these limits, we constrain theoretical models for the emission of gamma rays from binary black hole mergers.

A Joint Fermi-GBM and Swift-BAT Analysis of Gravitational-wave Candidates from the Third Gravitational-wave Observing Run / C. Fletcher, J. Wood, R. Hamburg, P. Veres, C.M. Hui, E. Bissaldi, M.S. Briggs, E. Burns, W.H. Cleveland, M.M. Giles, A. Goldstein, B.A. Hristov, D. Kocevski, S. Lesage, B. Mailyan, C. Malacaria, S. Poolakkil, A. von Kienlin, C.A. Wilson-Hodge, M. Crnogor?evi?, J. Delaunay, A. Tohuvavohu, R. Caputo, S.B. Cenko, S. Laha, T. Parsotan, R. Abbott, H. Abe, F. Acernese, K. Ackley, N. Adhikari, R.X. Adhikari, V.K. Adkins, V.B. Adya, C. Affeldt, D. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O.D. Aguiar, L. Aiello, A. Ain, P. Ajith, T. Akutsu, S. Albanesi, R.A. Alfaidi, A. Allocca, P.A. Altin, A. Amato, C. Anand, S. Anand, A. Ananyeva, S.B. Anderson, W.G. Anderson, M. Ando, T. Andrade, N. Andres, M. Andres-Carcasona, T. Andri?, S.V. Angelova, S. Ansoldi, J.M. Antelis, S. Antier, T. Apostolatos, E.Z. Appavuravther, S. Appert, S.K. Apple, K. Arai, A. Araya, M.C. 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A Joint Fermi-GBM and Swift-BAT Analysis of Gravitational-wave Candidates from the Third Gravitational-wave Observing Run

B. Haskell
Membro del Collaboration Group
;
2024

Abstract

We present Fermi Gamma-ray Burst Monitor (Fermi-GBM) and Swift Burst Alert Telescope (Swift-BAT) searches for gamma-ray/X-ray counterparts to gravitational-wave (GW) candidate events identified during the third observing run of the Advanced LIGO and Advanced Virgo detectors. Using Fermi-GBM onboard triggers and subthreshold gamma-ray burst (GRB) candidates found in the Fermi-GBM ground analyses, the Targeted Search and the Untargeted Search, we investigate whether there are any coincident GRBs associated with the GWs. We also search the Swift-BAT rate data around the GW times to determine whether a GRB counterpart is present. No counterparts are found. Using both the Fermi-GBM Targeted Search and the Swift-BAT search, we calculate flux upper limits and present joint upper limits on the gamma-ray luminosity of each GW. Given these limits, we constrain theoretical models for the emission of gamma rays from binary black hole mergers.
Settore PHYS-05/A - Astrofisica, cosmologia e scienza dello spazio
2024
27-mar-2024
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/1107828
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