Details

Autor(en) / Beteiligte

• Ackley, K
• Anderson, S B
• Ast, M
• Bassiri, R
• Bavigadda, V
• Cagnoli, G
• Caride, S
• Casentini, C
• Cavalier, F
• Charlton, P
• Coccia, E
• Cohadon, P-F
• Cooper, S J
• Corbitt, T R
• Countryman, S T
• Dave, I
• Degallaix, J
• Di Fiore, L
• Eichholz, J
• Etienne, Z
• Evans, M
• Everett, R
• Fletcher, M
• Frei, Z
• Fritschel, P
• Gehrels, N
• Gosselin, M
• Grote, H
• Hall, E D
• Haster, C-J
• Heidmann, A
• Heurs, M
• Hopkins, P
• Huet, D
• Isac, J-M
• Isi, M
• Kang, G
• Kawabe, K
• Keitel, D
• Khazanov, E A
• Kim, Chunglee
• Kim, Y-M
• Klein, B
• Kontos, A
• Kowalska, I
• Kuehn, G
• Lazzaro, C
• Leaci, P
• Leavey, S
• Lee, H K
• Letendre, N
• Li, T G F
• London, L T
• Lück, H
• Maksimovic, I
• Mansell, G L
• Markosyan, A S
• Martynov, D V
• Matone, L
• Meacher, D
• Meidam, J
• Metzdorff, R
• Mittleman, R
• Mow-Lowry, C M
• Naticchioni, L
• Normandin, M E N
• Passaquieti, R
• Pedurand, R
• Perez, C J
• Poggiani, R
• Prasad, J
• Privitera, S
• Rajan, C
• Sadeghian, L
• Samajdar, A
• Scheuer, J
• Schuette, D
• Sequino, V
• Siellez, K
• Sorazu, B
• Srivastava, A K
• Steinlechner, S
• Steinmeyer, D
• Stuver, A L
• Tringali, M C
• Urban, A L
• Viceré, A
• Vinciguerra, S
• Vine, D J
• Vinet, J-Y
• Vorvick, C
• Wade, A R
• Wade, M
• Wang, M
• Weaver, B
• Westphal, T
• Zadro ny, A
• Zangrando, L
• Zhang, T
• Zhu, X J

Titel

All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run

Ist Teil von

• Classical and quantum gravity, 2018-02, Vol.35 (6), p.65009

Ort / Verlag

United States: IOP Publishing

Erscheinungsjahr

2018

Link zum Volltext

Quelle

Alma/SFX Local Collection

Beschreibungen/Notizen

• We present the results of a search for long-duration gravitational wave transients in the data of the LIGO Hanford and LIGO Livingston second generation detectors between September 2015 and January 2016, with a total observational time of 49 d. The search targets gravitational wave transients of 10-500 s duration in a frequency band of 24-2048 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. No significant events were observed. As a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. We also show that the search is sensitive to sources in the Galaxy emitting at least   10−8 M⊙c2 in gravitational waves.