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The LSC glitch group: monitoring noise transients during the fifth LIGO science run

dc.contributor.authorBlackburn, L.en_US
dc.contributor.authorCadonati, L.en_US
dc.contributor.authorCaride, S.en_US
dc.contributor.authorCaudill, S.en_US
dc.contributor.authorChatterji, S.en_US
dc.contributor.authorChristensen, N.en_US
dc.contributor.authorDalrymple, J.en_US
dc.contributor.authorDesai, S.en_US
dc.contributor.authorDi Credico, A.en_US
dc.contributor.authorEly, G.en_US
dc.contributor.authorGarofoli, J.en_US
dc.contributor.authorGoggin, L. M.en_US
dc.contributor.authorGonzalez, G.en_US
dc.contributor.authorGouaty, R.en_US
dc.contributor.authorGray, C.en_US
dc.contributor.authorGretarsson, A. M.en_US
dc.contributor.authorHoak, D.en_US
dc.contributor.authorIsogai, T.en_US
dc.contributor.authorKatsavounidis, E.en_US
dc.contributor.authorKissel, J. S.en_US
dc.contributor.authorKlimenko, S.en_US
dc.contributor.authorMercer, R. A.en_US
dc.contributor.authorMohapatra, S.en_US
dc.contributor.authorMukherjee, S.en_US
dc.contributor.authorRaab, F.en_US
dc.contributor.authorRiles, Keithen_US
dc.contributor.authorSaulson, P. R.en_US
dc.contributor.authorSchofield, R.en_US
dc.contributor.authorShawhan, P.en_US
dc.contributor.authorSlutsky, J.en_US
dc.contributor.authorSmith, J. R.en_US
dc.contributor.authorStone, R.en_US
dc.contributor.authorVorvick, C.en_US
dc.contributor.authorZanolin, M.en_US
dc.contributor.authorZotov, N.en_US
dc.contributor.authorZweizig, J.en_US
dc.date.accessioned2009-10-08T15:31:27Z
dc.date.available2009-10-08T15:31:27Z
dc.date.issued2008en_US
dc.identifier.citationBlackburn, L; Cadonati, L; Caride, S; Caudill, S; Chatterji, S; Christensen, N; Dalrymple, J; Desai, S; Credico, A Di; Ely, G; Garofoli, J; Goggin, L; Gonzalez, G; Gouaty, R; Gray, C; Gretarsson, A; Hoak, D; Isogai, T; Katsavounidis, E; Kissel, J; Klimenko, S; Mercer, R A; Mohapatra, S; Mukherjee, S; Raab, F; Riles, K; Saulson, P; Schofield, R; Shawhan, P; Slutsky, J; Smith, J R; Stone, R; Vorvick, C; Zanolin, M; Zotov, N; Zweizig, J (2008). "The LSC glitch group: monitoring noise transients during the fifth LIGO science run." Classical and Quantum Gravity 25(18):184004 (10pp). <http://hdl.handle.net/2027.42/64156>en_US
dc.identifier.issn0264-9381en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/64156
dc.description.abstract"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."en_US
dc.format.extent1098279 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.titleThe LSC glitch group: monitoring noise transients during the fifth LIGO science runen_US
dc.typeArticleen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/64156/1/cqg8_18_184004.pdf
dc.identifier.doihttp://dx.doi.org/10.1088/0264-9381/25/18/184004en_US
dc.identifier.sourceClassical and Quantum Gravityen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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