Cleaning the Virgo sampled data for the search of periodic sources of gravitational waves

F. Acernese; M. Alshourbagy; F. Antonucci; S. Aoudia; K.G. Arun; P. Astone; G. Ballardin; F. Barone; M. Barsuglia; T.S. Bauer; M. Beker; S. Bigotta; S. Birindelli; M.A. Bizouard; C. Boccara; F. Bondu; L. Bonelli; L. Bosi; S. Braccini; C. Bradaschia; A. Brillet; V. Brisson; H.J. Bulten; D. Buskulic; G. Cagnoli; E. Calloni; E. Campagna; B. Canuel; F. Carbognani; L. Carbone; F. Cavalier; R. Cavalieri; G. Cella; E.C. Mottin; S. Chatterji; A. Chincarini; F. Cleva; E. Coccia; J. Colas; A. Colla; M. Colombini; C. Corda; A. Corsi; J.P. Coulon; E. Cuoco; S. D'Antonio; A. Dari; V. Dattilo; M. Davier; R. Day; S. Hild; J.F.J. van den Brand

doi:10.1088/0264-9381/26/20/204002

Cleaning the Virgo sampled data for the search of periodic sources of gravitational waves

F. Acernese^*, M. Alshourbagy, F. Antonucci, S. Aoudia, K.G. Arun, P. Astone, G. Ballardin, F. Barone, M. Barsuglia, T.S. Bauer, M. Beker, S. Bigotta, S. Birindelli, M.A. Bizouard, C. Boccara, F. Bondu, L. Bonelli, L. Bosi, S. Braccini, C. BradaschiaA. Brillet, V. Brisson, H.J. Bulten, D. Buskulic, G. Cagnoli, E. Calloni, E. Campagna, B. Canuel, F. Carbognani, L. Carbone, F. Cavalier, R. Cavalieri, G. Cella, E.C. Mottin, S. Chatterji, A. Chincarini, F. Cleva, E. Coccia, J. Colas, A. Colla, M. Colombini, C. Corda, A. Corsi, J.P. Coulon, E. Cuoco, S. D'Antonio, A. Dari, V. Dattilo, M. Davier, R. Day, S. Hild, J.F.J. van den Brand

^*Corresponding author for this work

Research output: Contribution to journal › Article › Academic › peer-review

9 Citations (Web of Science)

Abstract

The cleaning procedure used to produce the data that we analyze for the search of periodic sources of gravitational waves is based on different steps, which are applied to both time and frequency domain data. We have recently improved the procedure, which now consists of different steps. The use of a cleaned procedure is in principle important, since it is aimed to recover at best the observation time from the data by vetoing only times where disturbances act and not entire data chunks. Clearly, the effect of the procedure depends on the nature of the data, and is thus highly related to the detector characteristics in a particular run. We will here describe the whole cleaning chain, by giving details and examples based on the C7 and WSR10 Virgo runs.

Original language	English
Article number	204002
Number of pages	10
Journal	Classical and Quantum Gravity
Volume	26
Issue number	20
DOIs	https://doi.org/10.1088/0264-9381/26/20/204002
Publication status	Published - 21 Oct 2009
Externally published	Yes

Access to Document

10.1088/0264-9381/26/20/204002

Cite this

Acernese, F., Alshourbagy, M., Antonucci, F., Aoudia, S., Arun, K. G., Astone, P., Ballardin, G., Barone, F., Barsuglia, M., Bauer, T. S., Beker, M., Bigotta, S., Birindelli, S., Bizouard, M. A., Boccara, C., Bondu, F., Bonelli, L., Bosi, L., Braccini, S., ... van den Brand, J. F. J. (2009). Cleaning the Virgo sampled data for the search of periodic sources of gravitational waves. Classical and Quantum Gravity, 26(20), Article 204002. https://doi.org/10.1088/0264-9381/26/20/204002

@article{c0925727972947858e7c0d5a6a096c92,

title = "Cleaning the Virgo sampled data for the search of periodic sources of gravitational waves",

abstract = "The cleaning procedure used to produce the data that we analyze for the search of periodic sources of gravitational waves is based on different steps, which are applied to both time and frequency domain data. We have recently improved the procedure, which now consists of different steps. The use of a cleaned procedure is in principle important, since it is aimed to recover at best the observation time from the data by vetoing only times where disturbances act and not entire data chunks. Clearly, the effect of the procedure depends on the nature of the data, and is thus highly related to the detector characteristics in a particular run. We will here describe the whole cleaning chain, by giving details and examples based on the C7 and WSR10 Virgo runs.",

author = "F. Acernese and M. Alshourbagy and F. Antonucci and S. Aoudia and K.G. Arun and P. Astone and G. Ballardin and F. Barone and M. Barsuglia and T.S. Bauer and M. Beker and S. Bigotta and S. Birindelli and M.A. Bizouard and C. Boccara and F. Bondu and L. Bonelli and L. Bosi and S. Braccini and C. Bradaschia and A. Brillet and V. Brisson and H.J. Bulten and D. Buskulic and G. Cagnoli and E. Calloni and E. Campagna and B. Canuel and F. Carbognani and L. Carbone and F. Cavalier and R. Cavalieri and G. Cella and E.C. Mottin and S. Chatterji and A. Chincarini and F. Cleva and E. Coccia and J. Colas and A. Colla and M. Colombini and C. Corda and A. Corsi and J.P. Coulon and E. Cuoco and S. D'Antonio and A. Dari and V. Dattilo and M. Davier and R. Day and S. Hild and {van den Brand}, J.F.J.",

year = "2009",

month = oct,

day = "21",

doi = "10.1088/0264-9381/26/20/204002",

language = "English",

volume = "26",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

publisher = "IOP Publishing Ltd.",

number = "20",

}

Acernese, F, Alshourbagy, M, Antonucci, F, Aoudia, S, Arun, KG, Astone, P, Ballardin, G, Barone, F, Barsuglia, M, Bauer, TS, Beker, M, Bigotta, S, Birindelli, S, Bizouard, MA, Boccara, C, Bondu, F, Bonelli, L, Bosi, L, Braccini, S, Bradaschia, C, Brillet, A, Brisson, V, Bulten, HJ, Buskulic, D, Cagnoli, G, Calloni, E, Campagna, E, Canuel, B, Carbognani, F, Carbone, L, Cavalier, F, Cavalieri, R, Cella, G, Mottin, EC, Chatterji, S, Chincarini, A, Cleva, F, Coccia, E, Colas, J, Colla, A, Colombini, M, Corda, C, Corsi, A, Coulon, JP, Cuoco, E, D'Antonio, S, Dari, A, Dattilo, V, Davier, M, Day, R, Hild, S & van den Brand, JFJ 2009, 'Cleaning the Virgo sampled data for the search of periodic sources of gravitational waves', Classical and Quantum Gravity, vol. 26, no. 20, 204002. https://doi.org/10.1088/0264-9381/26/20/204002

TY - JOUR

T1 - Cleaning the Virgo sampled data for the search of periodic sources of gravitational waves

AU - Acernese, F.

AU - Alshourbagy, M.

AU - Antonucci, F.

AU - Aoudia, S.

AU - Arun, K.G.

AU - Astone, P.

AU - Ballardin, G.

AU - Barone, F.

AU - Barsuglia, M.

AU - Bauer, T.S.

AU - Beker, M.

AU - Bigotta, S.

AU - Birindelli, S.

AU - Bizouard, M.A.

AU - Boccara, C.

AU - Bondu, F.

AU - Bonelli, L.

AU - Bosi, L.

AU - Braccini, S.

AU - Bradaschia, C.

AU - Brillet, A.

AU - Brisson, V.

AU - Bulten, H.J.

AU - Buskulic, D.

AU - Cagnoli, G.

AU - Calloni, E.

AU - Campagna, E.

AU - Canuel, B.

AU - Carbognani, F.

AU - Carbone, L.

AU - Cavalier, F.

AU - Cavalieri, R.

AU - Cella, G.

AU - Mottin, E.C.

AU - Chatterji, S.

AU - Chincarini, A.

AU - Cleva, F.

AU - Coccia, E.

AU - Colas, J.

AU - Colla, A.

AU - Colombini, M.

AU - Corda, C.

AU - Corsi, A.

AU - Coulon, J.P.

AU - Cuoco, E.

AU - D'Antonio, S.

AU - Dari, A.

AU - Dattilo, V.

AU - Davier, M.

AU - Day, R.

AU - Hild, S.

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

PY - 2009/10/21

Y1 - 2009/10/21

N2 - The cleaning procedure used to produce the data that we analyze for the search of periodic sources of gravitational waves is based on different steps, which are applied to both time and frequency domain data. We have recently improved the procedure, which now consists of different steps. The use of a cleaned procedure is in principle important, since it is aimed to recover at best the observation time from the data by vetoing only times where disturbances act and not entire data chunks. Clearly, the effect of the procedure depends on the nature of the data, and is thus highly related to the detector characteristics in a particular run. We will here describe the whole cleaning chain, by giving details and examples based on the C7 and WSR10 Virgo runs.

AB - The cleaning procedure used to produce the data that we analyze for the search of periodic sources of gravitational waves is based on different steps, which are applied to both time and frequency domain data. We have recently improved the procedure, which now consists of different steps. The use of a cleaned procedure is in principle important, since it is aimed to recover at best the observation time from the data by vetoing only times where disturbances act and not entire data chunks. Clearly, the effect of the procedure depends on the nature of the data, and is thus highly related to the detector characteristics in a particular run. We will here describe the whole cleaning chain, by giving details and examples based on the C7 and WSR10 Virgo runs.

U2 - 10.1088/0264-9381/26/20/204002

DO - 10.1088/0264-9381/26/20/204002

M3 - Article

SN - 0264-9381

VL - 26

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 20

M1 - 204002

ER -