Search for gravitational wave radiation associated with the pulsating tail of the SGR 1806-20 hyperflare of 27 December 2004 using LIGO

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

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Originalspracheundefiniert/unbekannt
FachzeitschriftPhysical Review D
Jahrgang76
Ausgabenummer6
PublikationsstatusVeröffentlicht - 2007

Abstract

We report on a search for gravitational waves from binary black hole inspirals in the data from the second science run of the LIGO interferometers. The search focused on binary systems with component masses between 3 and 20M[sun]. Optimally oriented binaries with distances up to 1 Mpc could be detected with efficiency of at least 9085.6 hours of data that we searched.

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Search for gravitational wave radiation associated with the pulsating tail of the SGR 1806-20 hyperflare of 27 December 2004 using LIGO. / The LIGO Scientific Collaboration.
in: Physical Review D, Jahrgang 76, Nr. 6, 2007.

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

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title = "Search for gravitational wave radiation associated with the pulsating tail of the SGR 1806-20 hyperflare of 27 December 2004 using LIGO",
abstract = "We report on a search for gravitational waves from binary black hole inspirals in the data from the second science run of the LIGO interferometers. The search focused on binary systems with component masses between 3 and 20M[sun]. Optimally oriented binaries with distances up to 1 Mpc could be detected with efficiency of at least 9085.6 hours of data that we searched.",
author = "{The LIGO Scientific Collaboration} and B. Abbott and R. Abbott and R. Adhikari and J. Agresti and P. Ajith and B. Allen and R. Amin and Anderson, {S. B.} and Anderson, {W. G.} and M. Arain and M. Araya and H. Armandula and M. Ashley and S. Aston and Peter Aufmuth and C. Aulbert and Stanislav Babak and S. Ballmer and H. Bantilan and Barish, {B. C.} and C. Barker and D. Barker and B. Barr and P. Barriga and Barton, {M. A.} and K. Bayer and K. Belczynski and J. Betzwieser and Beyersdorf, {P. T.} and B. Bhawal and Bilenko, {I. A.} and G. Billingsley and R. Biswas and E. Black and K. Blackburn and L. Blackburn and S. Bose and Brown, {D. A.} and Y. Chen and K. Danzmann and A. Dietz and T. Fricke and M. Heurs and M. Hewitson and F. Kawazoe and H. L{\"u}ck and H. Vahlbruch and B. Willke and W. Wu and L. Zhang",
year = "2007",
doi = "10.1103/PhysRevD.76.062003",
language = "Undefined/Unknown",
volume = "76",
journal = "Physical Review D",
issn = "1089-4918",
publisher = "American Institute of Physics",
number = "6",

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TY - JOUR

T1 - Search for gravitational wave radiation associated with the pulsating tail of the SGR 1806-20 hyperflare of 27 December 2004 using LIGO

AU - The LIGO Scientific Collaboration

AU - Abbott, B.

AU - Abbott, R.

AU - Adhikari, R.

AU - Agresti, J.

AU - Ajith, P.

AU - Allen, B.

AU - Amin, R.

AU - Anderson, S. B.

AU - Anderson, W. G.

AU - Arain, M.

AU - Araya, M.

AU - Armandula, H.

AU - Ashley, M.

AU - Aston, S.

AU - Aufmuth, Peter

AU - Aulbert, C.

AU - Babak, Stanislav

AU - Ballmer, S.

AU - Bantilan, H.

AU - Barish, B. C.

AU - Barker, C.

AU - Barker, D.

AU - Barr, B.

AU - Barriga, P.

AU - Barton, M. A.

AU - Bayer, K.

AU - Belczynski, K.

AU - Betzwieser, J.

AU - Beyersdorf, P. T.

AU - Bhawal, B.

AU - Bilenko, I. A.

AU - Billingsley, G.

AU - Biswas, R.

AU - Black, E.

AU - Blackburn, K.

AU - Blackburn, L.

AU - Bose, S.

AU - Brown, D. A.

AU - Chen, Y.

AU - Danzmann, K.

AU - Dietz, A.

AU - Fricke, T.

AU - Heurs, M.

AU - Hewitson, M.

AU - Kawazoe, F.

AU - Lück, H.

AU - Vahlbruch, H.

AU - Willke, B.

AU - Wu, W.

AU - Zhang, L.

PY - 2007

Y1 - 2007

N2 - We report on a search for gravitational waves from binary black hole inspirals in the data from the second science run of the LIGO interferometers. The search focused on binary systems with component masses between 3 and 20M[sun]. Optimally oriented binaries with distances up to 1 Mpc could be detected with efficiency of at least 9085.6 hours of data that we searched.

AB - We report on a search for gravitational waves from binary black hole inspirals in the data from the second science run of the LIGO interferometers. The search focused on binary systems with component masses between 3 and 20M[sun]. Optimally oriented binaries with distances up to 1 Mpc could be detected with efficiency of at least 9085.6 hours of data that we searched.

U2 - 10.1103/PhysRevD.76.062003

DO - 10.1103/PhysRevD.76.062003

M3 - Article

VL - 76

JO - Physical Review D

JF - Physical Review D

SN - 1089-4918

IS - 6

ER -

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