Details
Originalsprache | Englisch |
---|---|
Aufsatznummer | 255 |
Fachzeitschrift | Astrophysical Journal |
Jahrgang | 977 |
Ausgabenummer | 2 |
Publikationsstatus | Veröffentlicht - 18 Dez. 2024 |
Abstract
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.
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Astronomie und Astrophysik
- Erdkunde und Planetologie (insg.)
- Astronomie und Planetologie
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in: Astrophysical Journal, Jahrgang 977, Nr. 2, 255, 18.12.2024.
Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review
}
TY - JOUR
T1 - A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154
AU - The LIGO Scientific Collaboration
AU - The Virgo Collaboration
AU - the 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 - Anderson, S. B.
AU - Anderson, W. G.
AU - Andia, M.
AU - Ando, M.
AU - Andrade, T.
AU - Carlassara, M.
AU - Chakraborty, P.
AU - Danilishin, S.
AU - Danzmann, K.
AU - Dasgupta, A.
AU - Heurs, M.
AU - Johny, N.
AU - Junker, J.
AU - Knust, N.
AU - Lück, H.
AU - Matiushechkina, M.
AU - Vahlbruch, H.
AU - Wilken, D.
AU - Willke, B.
AU - Andric, Tomislav
AU - Bergamin, Fabio
AU - Bisht, Aparna
AU - Bode, Nina
AU - Borchers, Andreas
AU - Brinkmann, Marc
AU - Brockmueller, Eike
AU - Carter, Jonathan Joseph
AU - Ghosh, Shrobana
AU - Hochheim, S.
AU - Kastaun, Wolfgang
AU - Khan, Fawad
AU - Koch, Philip
AU - Kuehn, G.
AU - Kruska, Kristopher
AU - Kringel, Volker
AU - Lehmann, J.
AU - Lough, James
AU - Maciy, R. R.
AU - Ma'arif, M.
AU - Meylahn, Fabian
AU - Nadji, S. L.
AU - Nery, M.
AU - Ohme, F.
AU - Pascale, G.
AU - Schutz, B. F.
AU - Schulte, Bernd Wolfgang
AU - Schneewind, M.
AU - Venneberg, J.
AU - von Wrangel, J.
AU - Wang, Z.
AU - Weinert, Michael
AU - Wellmann, F.
AU - Wu, D. S.
N1 - Publisher Copyright: © 2024. The Author(s). Published by the American Astronomical Society.
PY - 2024/12/18
Y1 - 2024/12/18
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 - http://www.scopus.com/inward/record.url?scp=85213701609&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ad8de0
DO - 10.3847/1538-4357/ad8de0
M3 - Article
AN - SCOPUS:85213701609
VL - 977
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 2
M1 - 255
ER -