Details
Originalsprache | Englisch |
---|---|
Aufsatznummer | 8 |
Fachzeitschrift | Astrophysical Journal |
Jahrgang | 925 |
Ausgabenummer | 1 |
Publikationsstatus | Veröffentlicht - 20 Jan. 2022 |
Abstract
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 925, Nr. 1, 8, 20.01.2022.
Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review
}
TY - JOUR
T1 - Results from an Einstein@Home search for continuous gravitational waves from G347.3 at low frequencies in LIGO O2 data
AU - Ming, Jing
AU - Papa, Maria Alessandra
AU - Machenschalk, Bernd
AU - Steltner, Benjamin
AU - Prix, Reinhard
AU - Allen, Bruce
AU - Behnke, Oliver
PY - 2022/1/20
Y1 - 2022/1/20
N2 - We present results of a search for periodic gravitational wave signals with frequency between 20 and 400 Hz, from the neutron star in the supernova remnant G347.3-0.5, using LIGO O2 public data. The search is deployed on the volunteer computing project Einstein@Home, with thousands of participants donating compute cycles to make this endevour possible. We find no significant signal candidate and set the most constraining upper limits to date on the amplitude of gravitational wave signals from the target, corresponding to deformations below \(10^{-6}\) in a large part of the band. At the frequency of best strain sensitivity, near \(166\) Hz, we set 90\%\ confidence upper limits on the gravitational wave intrinsic amplitude of \(h_0^{90\%}\approx 7.0\times10^{-26}\). Over most of the frequency range our upper limits are a factor of 20 smaller than the indirect age-based upper limit.
AB - We present results of a search for periodic gravitational wave signals with frequency between 20 and 400 Hz, from the neutron star in the supernova remnant G347.3-0.5, using LIGO O2 public data. The search is deployed on the volunteer computing project Einstein@Home, with thousands of participants donating compute cycles to make this endevour possible. We find no significant signal candidate and set the most constraining upper limits to date on the amplitude of gravitational wave signals from the target, corresponding to deformations below \(10^{-6}\) in a large part of the band. At the frequency of best strain sensitivity, near \(166\) Hz, we set 90\%\ confidence upper limits on the gravitational wave intrinsic amplitude of \(h_0^{90\%}\approx 7.0\times10^{-26}\). Over most of the frequency range our upper limits are a factor of 20 smaller than the indirect age-based upper limit.
KW - gr-qc
KW - astro-ph.HE
UR - http://www.scopus.com/inward/record.url?scp=85124167732&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ac35cb
DO - 10.3847/1538-4357/ac35cb
M3 - Article
VL - 925
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 1
M1 - 8
ER -