TY - JOUR
T1 - A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154
AU - LIGO Scientific Collaboration, Virgo Collaboration and KAGRA Collaboration
AU - Abac, A. G.
AU - Abbott, R.
AU - Abouelfettouh, I.
AU - Acernese, F.
AU - Ackley, K.
AU - Adhicary, S.
AU - Adhikari, N.
AU - Adhikari, R. X.
AU - Adkins, V. K.
AU - Agarwal, D.
AU - Agathos, M.
AU - Aghaei Abchouyeh, M.
AU - Aguiar, O. D.
AU - Aguilar, I.
AU - Aiello, L.
AU - Ain, A.
AU - Ajith, P.
AU - Akutsu, T.
AU - Albanesi, S.
AU - Alfaidi, R. A.
AU - Al-Jodah, A.
AU - Alléné, C.
AU - Allocca, A.
AU - Al-Shammari, S.
AU - Altin, P. A.
AU - Alvarez-Lopez, S.
AU - Amato, A.
AU - Amez-Droz, L.
AU - Amorosi, A.
AU - Amra, C.
AU - Ananyeva, A.
AU - Caudill, S.
AU - Gupta, P.
AU - Hannuksela, O. A.
AU - Kuijer, P.
AU - Pang, P. T.H.
AU - Puecher, A.
AU - Van Den Broeck, C.
AU - Baka, Tomek
AU - Dooney, Tom
AU - Gadre, Bhooshan Uday
AU - Janquart, Justin
AU - Kalaghatgi, Chinmay
AU - Lopez, Melissa
AU - Meijer, Quirijn
AU - Narola, Harsh
AU - Roy, Soumen
AU - Schmidt, Stefano
AU - van der Sluys, Marc
AU - Maliyamveettil Kunjumuhammed, Haris
N1 - Publisher Copyright:
© 2024. The Author(s). Published by the American Astronomical Society.
PY - 2024/12/20
Y1 - 2024/12/20
N2 - The magnetar SGR 1935+2154 is the only known Galactic source of fast radio bursts (FRBs). FRBs from SGR 1935 +2154 were first detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME)/FRB and the Survey for Transient Astronomical Radio Emission 2 in 2020 April, after the conclusion of the LIGO, Virgo, and KAGRA Collaborations’ O3 observing run. Here, we analyze four periods of gravitational wave (GW) data from the GEO600 detector coincident with four periods of FRB activity detected by CHIME/FRB, as well as X-ray glitches and X-ray bursts detected by NICER and NuSTAR close to the time of one of the FRBs. We do not detect any significant GW emission from any of the events. Instead, using a short-duration GW search (for bursts <1 s) we derive 50% (90%) upper limits of 1048 (1049) erg for GWs at 300 Hz and 1049 (1050) erg at 2 kHz, and constrain the GW-to-radio energy ratio to <1014−1016. We also derive upper limits from a long-duration search for bursts with durations between 1 and 10 s. These represent the strictest upper limits on concurrent GW emission from FRBs.
AB - The magnetar SGR 1935+2154 is the only known Galactic source of fast radio bursts (FRBs). FRBs from SGR 1935 +2154 were first detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME)/FRB and the Survey for Transient Astronomical Radio Emission 2 in 2020 April, after the conclusion of the LIGO, Virgo, and KAGRA Collaborations’ O3 observing run. Here, we analyze four periods of gravitational wave (GW) data from the GEO600 detector coincident with four periods of FRB activity detected by CHIME/FRB, as well as X-ray glitches and X-ray bursts detected by NICER and NuSTAR close to the time of one of the FRBs. We do not detect any significant GW emission from any of the events. Instead, using a short-duration GW search (for bursts <1 s) we derive 50% (90%) upper limits of 1048 (1049) erg for GWs at 300 Hz and 1049 (1050) erg at 2 kHz, and constrain the GW-to-radio energy ratio to <1014−1016. We also derive upper limits from a long-duration search for bursts with durations between 1 and 10 s. These represent the strictest upper limits on concurrent GW emission from FRBs.
UR - https://www.scopus.com/pages/publications/85213701609
U2 - 10.3847/1538-4357/ad8de0
DO - 10.3847/1538-4357/ad8de0
M3 - Article
AN - SCOPUS:85213701609
SN - 0004-637X
VL - 977
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 20
ER -