Blackburn, L. and Cadonati, L. and Caride, L. and Caudill, S. and Chatterji, S. and Christensen, N. and Dalrymple, J. and Desai, S. and Di Credico, A. and Ely, G. and Garofoli, J. and Goggin, L. and González, G. and Gouaty, R. and Gray, C. and Gretarsson, A. and Hoak, D. and Isogai, T. and Katsavounidis, E. and Kissel, J. and Klimenko, S. and Mercer, R. A. and Mohapatra, S. and Mukherjee, S. and Raab, F. and Riles, K. and Saulson, P. and Schofield, R. and Shawhan, P. and Slutsky, J. and Smith, J. R. and Stone, R. and Vorvick, C. and Zanolin, M. and Zotov, N. and Zweizig, J. (2008) The LSC glitch group: monitoring noise transients during the fifth LIGO science run. Classical and Quantum Gravity, 25 (18). Art. No. 184004. ISSN 0264-9381 http://resolver.caltech.edu/CaltechAUTHORS:BLAcqg08
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The LIGO Scientific Collaboration (LSC) glitch group is part of the LIGO detector characterization effort. It consists of data analysts and detector experts who, during and after science runs, collaborate for a better understanding of noise transients in the detectors. Goals of the glitch group during the fifth LIGO science run (S5) included (1) offline assessment of the detector data quality, with focus on noise transients, (2) veto recommendations for astrophysical analysis and (3) feedback to the commissioning team on anomalies seen in gravitational wave and auxiliary data channels. Other activities included the study of auto-correlation of triggers from burst searches, stationarity of the detector noise and veto studies. The group identified causes for several noise transients that triggered false alarms in the gravitational wave searches; the times of such transients were identified and vetoed from the data generating the LSC astrophysical results.
|Additional Information:||Copyright © Institute of Physics and IOP Publishing Limited 2008. Received 4 April 2008, in final form 16 June 2008. Published 2 September 2008. Print publication: Issue 18 (21 September 2008). LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation and operates under cooperative agreement PHY-0107417. We would like to thank the Bonneville Power Administration, particularly Mike Viles, for providing and interpreting records of power grid events. We are grateful to all members of the LIGO Scientific Collaboration for feedback and support for our work and especially to all the operators and members from the commissioning team who tirelessly worked for two long years to ensure a high duty cycle and good sensitivity during the fifth LIGO science run. This paper was assigned LIGO document number P080016.|
|Subject Keywords:|| Abbott B et al (LIGO Scientific Collaboration) 2007 LIGO: The laser interferometer gravitational-wave observatory Preprint arXiv:0711.3041  Mukherjee S (for the LIGO Scientific Collaboration) 2007 Class. Quantum Grav. 24 S701  Zweizig J 1999 LIGO Technical Document G990079-35  McNabb J et al 2004 Class. Quantum Grav. 21 S1705  Klimenko S et al 2004 Class. Quantum Grav. 21 S1685  Klimenko S 2005 LIGO Technical Document G050192-00-Z  Mukherjee S 2006 Class. Quantum Grav. 20 S925  LIGO Scientific Collaboration 2007 Technical Document T-070109-01-Z  Chatterji S, Blackburn L, Martin G and Katsavounidis E 2004 Class. Quantum Grav. 21 S1809  Chatterji S 2005 PhD Thesis MIT  Sylvestre J 2002 Phys. Rev. D 66 102004  Christensen N (for the LIGO Scientific Collaboration) 2005 Class. Quantum Grav. 22 S1059  Christensen N, Shawhan P and Gonzalez G (for the LIGO Scientific Collaboration) 2004 Class. Quantum Grav. 20 S1747  Cadonati L and Katsavounidis E (for the LIGO Scientific Collaboration’s Bursts Working Group) 2003 Class. Quantum Grav. 20 S633  Di Credico A (for the LIGO Scientific Collaboration) 2005 Class. Quantum Grav. 22 S1051  Abbott B et al (LIGO Scientific Collaboration) 2007 Class. Quantum Grav. 24 5343  Gouaty R (for the LIGO Scientific Collaboration) 2008 Preprint arXiv:0805.2412|
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|Deposited On:||08 Sep 2008 21:03|
|Last Modified:||26 Dec 2012 10:16|
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