Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914

被引：256

作者：

Abbott, B. P.

Abbott, R. ^{[1
]}

Abbott, T. D. ^{[2
]}

Abernathy, M. R. ^{[1
]}

Acernese, F. ^{[3
,4
]}

Ackley, K. ^{[5
]}

Adamo, M. ^{[4
,6
]}

Adams, C. ^{[7
]}

Adams, T. ^{[8
]}

Addesso, P. ^{[3
]}

Adhikari, R. X. ^{[1
]}

Adya, V. B. ^{[9
]}

Affeldt, C. ^{[9
]}

Agathos, M. ^{[10
]}

Agatsuma, K. ^{[10
]}

Aggarwal, N. ^{[11
]}

Aguiar, O. D. ^{[12
]}

Aiello, L. ^{[13
,14
]}

Ain, A. ^{[15
]}

Ajith, P. ^{[16
]}

Allen, B. ^{[9
,17
,18
]}

Allocca, A. ^{[19
,20
]}

Altin, P. A. ^{[21
]}

Anderson, S. B. ^{[1
]}

Anderson, W. G. ^{[17
]}

Arai, K. ^{[1
]}

Araya, M. C. ^{[1
]}

Arceneaux, C. C. ^{[6
]}

Areeda, J. S. ^{[22
]}

Arnaud, N. ^{[23
]}

Arun, K. G. ^{[24
]}

Ascenzi, S. ^{[14
,25
]}

Ashton, G. ^{[26
]}

Ast, M. ^{[27
]}

Aston, S. M. ^{[7
]}

Astone, P. ^{[28
]}

Aufmuth, P. ^{[9
]}

Aulbert, C. ^{[9
]}

Babak, S. ^{[29
]}

Bacon, P. ^{[30
]}

Bader, M. K. M. ^{[10
]}

Baker, P. T. ^{[31
]}

Baldaccini, F. ^{[32
,33
]}

Ballardin, G. ^{[34
]}

Ballmer, S. W. ^{[35
]}

Barayoga, J. C. ^{[1
]}

Barclay, S. E. ^{[36
]}

Barish, B. C. ^{[1
]}

Barker, D. ^{[37
]}

Barone, F. ^{[3
,4
]}

机构：

[1] CALTECH, LIGO, Pasadena, CA 91125 USA

[2] Louisiana State Univ, Baton Rouge, LA 70803 USA

[3] Univ Salerno, I-84084 Salerno, Italy

[4] Complesso Univ Monte S Angelo, Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy

[5] Univ Florida, Gainesville, FL 32611 USA

[6] Univ Mississippi, University, MS 38677 USA

[7] LIGO Livingston Observ, Livingston, LA 70754 USA

[8] Univ Savoie Mont Blanc, Lab Annecy Le Vieux Phys Particules, CNRS IN2P3, F-74941 Annecy Le Vieux, France

[9] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany

[10] Nikhef, Sci Pk, NL-1098 XG Amsterdam, Netherlands

[11] MIT, LIGO, Cambridge, MA 02139 USA

[12] Inst Nacl Pesquisas Espaciais, BR-12227010 Sao Paulo, Brazil

[13] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, I-67100 Laquila, Italy

[14] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, Italy

[15] Inter Univ Ctr Astron & Astrophys, Pune 411007, Maharashtra, India

[16] Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bangalore 560012, Karnataka, India

[17] Univ Wisconsin, Milwaukee, WI 53201 USA

[18] Leibniz Univ Hannover, D-30167 Hannover, Germany

[19] Univ Pisa, I-56127 Pisa, Italy

[20] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy

[21] Australian Natl Univ, GPO Box 4, Canberra, ACT 0200, Australia

[22] Calif State Univ Fullerton, Fullerton, CA 92831 USA

[23] Univ Paris 11, CNRS IN2P3, Univ Paris Saclay, LAL, F-91400 Orsay, France

[24] Chennai Math Inst, Madras 603103, Tamil Nadu, India

[25] Univ Roma Tor Vergata, I-00133 Rome, Italy

[26] Univ Southampton, Southampton SO17 1BJ, Hants, England

[27] Univ Hamburg, D-22761 Hamburg, Germany

[28] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy

[29] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Potsdam, Germany

[30] Univ Paris Diderot, CNRS, CEA Irfu,IN2P3, Observ Paris,Sorbonne Paris Cite,APC,AstroParticu, F-75205 Paris 13, France

[31] Montana State Univ, Bozeman, MT 59717 USA

[32] Univ Perugia, I-06123 Perugia, Italy

[33] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy

[34] European Gravitat Observ, I-56021 Pisa, Italy

[35] Syracuse Univ, Syracuse, NY 13244 USA

[36] Univ Glasgow, SUPA, Glasgow G12 8QQ, Lanark, Scotland

[37] LIGO Hanford Observ, Richland, WA 99352 USA

[38] RMKI, Wigner RCP, Konkoly Thege Miklos Ut 29-33, H-1121 Budapest, Hungary

[39] Columbia Univ, New York, NY 10027 USA

[40] Stanford Univ, Stanford, CA 94305 USA

[41] Univ Padua, Dipartimento Fis & Astron, I-35131 Padua, Italy

[42] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy

[43] CAMK PAN, PL-00716 Warsaw, Poland

[44] Univ Birmingham, Birmingham B15 2TT, W Midlands, England

[45] Univ Genoa, I-16146 Genoa, Italy

[46] Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy

[47] RRCAT, Indore 452013, Madhya Pradesh, India

[48] Moscow MV Lomonosov State Univ, Fac Phys, Moscow 119991, Russia

[49] Univ West Scotland, SUPA, Paisley PA1 2BE, Renfrew, Scotland

[50] Univ Western Australia, Crawley, WA 6009, Australia

来源：

CLASSICAL AND QUANTUM GRAVITY | 2016年 / 33卷 / 13期

基金：

美国国家科学基金会; 匈牙利科学研究基金会; 新加坡国家研究基金会; 澳大利亚研究理事会; 俄罗斯基础研究基金会; 巴西圣保罗研究基金会;

关键词：

gravitational waves; detector characterization; GW150914;

D O I：

10.1088/0264-9381/33/13/134001

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

On 14 September 2015, a gravitational wave signal from a coalescing black hole binary system was observed by the Advanced LIGO detectors. This paper describes the transient noise backgrounds used to determine the significance of the event (designated GW150914) and presents the results of investigations into potential correlated or uncorrelated sources of transient noise in the detectors around the time of the event. The detectors were operating nominally at the time of GW150914. We have ruled out environmental influences and non-Gaussian instrument noise at either LIGO detector as the cause of the observed gravitational wave signal.

引用

页数：34

共 41 条

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