Noise monitor tools and their application to Virgo data

T. Accadia; F. Acernese; M. Agathos; P. Astone; G. Ballardin; F. Barone; M. Barsuglia; A. Basti; T.S. Bauer; M. Bebronne; M. Bejger; M.G. Beker; M. Bitossi; M.A. Bizouard; M. Blom; F. Bondu; L. Bonelli; R. Bonnand; V. Boschi; L. Bosi; B. Bouhou; S. Braccini; C. Bradaschia; M. Branchesi; G.C.T. Briant; A. Brillet; V. Brisson; T. Bulik; H.J. Bulten; D. Buskulic; C. Buy; E. Calloni; B. Canuel; F. Carbognani; F. Cavalier; R. Cavalieri; G. Cella; E. Cesarini; O. Chaibi; E. Chassande-Mottin; A. Chincarini; A. Chiummo; F. Cleva; E. Coccia; P.F. Cohadon; C.N. Colacino; J. Colas; A. Colla; M. Colombini; A. Conte; J.F.J. van den Brand; S. Hild

doi:10.1088/1742-6596/363/1/012024

Noise monitor tools and their application to Virgo data

T. Accadia^*, F. Acernese, M. Agathos, P. Astone, G. Ballardin, F. Barone, M. Barsuglia, A. Basti, T.S. Bauer, M. Bebronne, M. Bejger, M.G. Beker, M. Bitossi, M.A. Bizouard, M. Blom, F. Bondu, L. Bonelli, R. Bonnand, V. Boschi, L. BosiB. Bouhou, S. Braccini, C. Bradaschia, M. Branchesi, G.C.T. Briant, A. Brillet, V. Brisson, T. Bulik, H.J. Bulten, D. Buskulic, C. Buy, E. Calloni, B. Canuel, F. Carbognani, F. Cavalier, R. Cavalieri, G. Cella, E. Cesarini, O. Chaibi, E. Chassande-Mottin, A. Chincarini, A. Chiummo, F. Cleva, E. Coccia, P.F. Cohadon, C.N. Colacino, J. Colas, A. Colla, M. Colombini, A. Conte, J.F.J. van den Brand, S. Hild

^*Corresponding author for this work

Research output: Contribution to journal › Conference article in journal › Academic › peer-review

2 Citations (Web of Science)

Abstract

The understanding of noise in interferometric gravitational wave detectors is fundamental in terms of both enabling prompt reactions in the mitigation of noise disturbances and in the establishment of appropriate data-cleaning strategies. Monitoring tools to perform online and offline noise analysis in areas such as transient signal detection, line identification algorithms and coherence are used to characterise the Virgo detector noise. In this paper, we describe the framework into which these tools are integrated - the Noise Monitor Application Programming Interface (NMAPI) - and provide examples of its application.

Original language	English
Article number	012024
Number of pages	10
Journal	Journal of Physics: Conference Series
Volume	363
DOIs	https://doi.org/10.1088/1742-6596/363/1/012024
Publication status	Published - 2012
Externally published	Yes

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10.1088/1742-6596/363/1/012024Licence: CC BY

Cite this

Accadia, T., Acernese, F., Agathos, M., Astone, P., Ballardin, G., Barone, F., Barsuglia, M., Basti, A., Bauer, T. S., Bebronne, M., Bejger, M., Beker, M. G., Bitossi, M., Bizouard, M. A., Blom, M., Bondu, F., Bonelli, L., Bonnand, R., Boschi, V., ... Hild, S. (2012). Noise monitor tools and their application to Virgo data. Journal of Physics: Conference Series, 363, [012024]. https://doi.org/10.1088/1742-6596/363/1/012024

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title = "Noise monitor tools and their application to Virgo data",

abstract = "The understanding of noise in interferometric gravitational wave detectors is fundamental in terms of both enabling prompt reactions in the mitigation of noise disturbances and in the establishment of appropriate data-cleaning strategies. Monitoring tools to perform online and offline noise analysis in areas such as transient signal detection, line identification algorithms and coherence are used to characterise the Virgo detector noise. In this paper, we describe the framework into which these tools are integrated - the Noise Monitor Application Programming Interface (NMAPI) - and provide examples of its application.",

author = "T. Accadia and F. Acernese and M. Agathos and P. Astone and G. Ballardin and F. Barone and M. Barsuglia and A. Basti and T.S. Bauer and M. Bebronne and M. Bejger and M.G. Beker and M. Bitossi and M.A. Bizouard and M. Blom and F. Bondu and L. Bonelli and R. Bonnand and V. Boschi and L. Bosi and B. Bouhou and S. Braccini and C. Bradaschia and M. Branchesi and G.C.T. Briant and A. Brillet and V. Brisson and T. Bulik and H.J. Bulten and D. Buskulic and C. Buy and E. Calloni and B. Canuel and F. Carbognani and F. Cavalier and R. Cavalieri and G. Cella and E. Cesarini and O. Chaibi and E. Chassande-Mottin and A. Chincarini and A. Chiummo and F. Cleva and E. Coccia and P.F. Cohadon and C.N. Colacino and J. Colas and A. Colla and M. Colombini and A. Conte and {van den Brand}, J.F.J. and S. Hild",

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Accadia, T, Acernese, F, Agathos, M, Astone, P, Ballardin, G, Barone, F, Barsuglia, M, Basti, A, Bauer, TS, Bebronne, M, Bejger, M, Beker, MG, Bitossi, M, Bizouard, MA, Blom, M, Bondu, F, Bonelli, L, Bonnand, R, Boschi, V, Bosi, L, Bouhou, B, Braccini, S, Bradaschia, C, Branchesi, M, Briant, GCT, Brillet, A, Brisson, V, Bulik, T, Bulten, HJ, Buskulic, D, Buy, C, Calloni, E, Canuel, B, Carbognani, F, Cavalier, F, Cavalieri, R, Cella, G, Cesarini, E, Chaibi, O, Chassande-Mottin, E, Chincarini, A, Chiummo, A, Cleva, F, Coccia, E, Cohadon, PF, Colacino, CN, Colas, J, Colla, A, Colombini, M, Conte, A, van den Brand, JFJ & Hild, S 2012, 'Noise monitor tools and their application to Virgo data', Journal of Physics: Conference Series, vol. 363, 012024. https://doi.org/10.1088/1742-6596/363/1/012024

TY - JOUR

T1 - Noise monitor tools and their application to Virgo data

AU - Accadia, T.

AU - Acernese, F.

AU - Agathos, M.

AU - Astone, P.

AU - Ballardin, G.

AU - Barone, F.

AU - Barsuglia, M.

AU - Basti, A.

AU - Bauer, T.S.

AU - Bebronne, M.

AU - Bejger, M.

AU - Beker, M.G.

AU - Bitossi, M.

AU - Bizouard, M.A.

AU - Blom, M.

AU - Bondu, F.

AU - Bonelli, L.

AU - Bonnand, R.

AU - Boschi, V.

AU - Bosi, L.

AU - Bouhou, B.

AU - Braccini, S.

AU - Bradaschia, C.

AU - Branchesi, M.

AU - Briant, G.C.T.

AU - Brillet, A.

AU - Brisson, V.

AU - Bulik, T.

AU - Bulten, H.J.

AU - Buskulic, D.

AU - Buy, C.

AU - Calloni, E.

AU - Canuel, B.

AU - Carbognani, F.

AU - Cavalier, F.

AU - Cavalieri, R.

AU - Cella, G.

AU - Cesarini, E.

AU - Chaibi, O.

AU - Chassande-Mottin, E.

AU - Chincarini, A.

AU - Chiummo, A.

AU - Cleva, F.

AU - Coccia, E.

AU - Cohadon, P.F.

AU - Colacino, C.N.

AU - Colas, J.

AU - Colla, A.

AU - Colombini, M.

AU - Conte, A.

AU - van den Brand, J.F.J.

AU - Hild, S.

PY - 2012

Y1 - 2012

N2 - The understanding of noise in interferometric gravitational wave detectors is fundamental in terms of both enabling prompt reactions in the mitigation of noise disturbances and in the establishment of appropriate data-cleaning strategies. Monitoring tools to perform online and offline noise analysis in areas such as transient signal detection, line identification algorithms and coherence are used to characterise the Virgo detector noise. In this paper, we describe the framework into which these tools are integrated - the Noise Monitor Application Programming Interface (NMAPI) - and provide examples of its application.

AB - The understanding of noise in interferometric gravitational wave detectors is fundamental in terms of both enabling prompt reactions in the mitigation of noise disturbances and in the establishment of appropriate data-cleaning strategies. Monitoring tools to perform online and offline noise analysis in areas such as transient signal detection, line identification algorithms and coherence are used to characterise the Virgo detector noise. In this paper, we describe the framework into which these tools are integrated - the Noise Monitor Application Programming Interface (NMAPI) - and provide examples of its application.

U2 - 10.1088/1742-6596/363/1/012024

DO - 10.1088/1742-6596/363/1/012024

M3 - Conference article in journal

SN - 1742-6588

VL - 363

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

M1 - 012024

ER -