The NoEMi (Noise Frequency Event Miner) framework

T. Accadia; F. Acernese; M. Agathos; P. Astone; G. Ballardin; F. Barone; M. Barsuglia; A. Basti; Th 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; 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. P. Coulon; E. Cuoco; S. D'Antonio; V. Dattilo; M. Davier; R. Day; R. De Rosa; G. Debreczeni; W. Del Pozzo; L. Di Fiore; A. Di Lieto; M. Di Paolo Emilio; A. Di Virgilio; A. Dietz; M. Drago; G. Endröczi; V. Fafone; I. Ferrante; F. Fidecaro; I. Fiori; R. Flaminio; L. A. Forte; J. D. Fournier; J. Franc; S. Franco; S. Frasca; F. Frasconi; M. Galimberti; L. Gammaitoni; F. Garufi; M. E. Gáspár; G. Gemme; E. Genin; A. Gennai; A. Giazotto; R. Gouaty; M. Granata; C. Greverie; G. M. Guidi; J. F. Hayau; A. Heidmann; H. Heitmann; P. Hello; G. Hemming; P. Jaranowski; R. J.G. Jonker; M. Kasprzack; I. Kowalska; A. Królak; N. Leroy; N. Letendre; T. G.F. Li; N. Liguori; M. Lorenzini; V. Loriette; G. Losurdo; E. Majorana; I. Maksimovic; V. Malvezzi; N. Man; M. Mantovani; F. Marchesoni; F. Marion; J. Marque; F. Martelli; A. Masserot; C. Michel; L. Milano; Y. Minenkov; M. Mohan; N. Morgado; A. Morgia; S. Mosca; B. Mours; L. Naticchioni; F. Nocera; L. Palladino; C. Palomba; F. Paoletti; R. Paoletti; M. Parisi; A. Pasqualetti; R. Passaquieti; D. Passuello; G. Persichetti; F. Piergiovanni; M. Pietka; L. Pinard; R. Poggiani; M. Prato; G. A. Prodi; M. Punturo; P. Puppo; D. S. Rabeling; I. Racz; P. Rapagnani; V. Re; T. Regimbau; F. Ricci; F. Robinet; A. Rocchi; L. Rolland; R. Romano; D. Rosińska; P. Ruggi; B. Sassolas; D. Sentenac; L. Sperandio; R. Sturani; B. Swinkels; M. Tacca; L. Taffarello; A. P.M. Ter Braack; A. Toncelli; M. Tonelli; O. Torre; E. Tournefier; F. Travasso; G. Vajente; J. F.J. Van Den Brand; C. Van Den Broeck; S. Van Der Putten; M. Vasuth; M. Vavoulidis; G. Vedovato; D. Verkindt; F. Vetrano; A. Viceré; J. Y. Vinet; S. Vitale; H. Vocca; R. L. Ward; M. Was; K. Yamamoto; M. Yvert; A. Zadroźny; J. P. Zendri

doi:10.1088/1742-6596/363/1/012037

The NoEMi (Noise Frequency Event Miner) framework

T. Accadia^*, F. Acernese, M. Agathos, P. Astone, G. Ballardin, F. Barone, M. Barsuglia, A. Basti, Th 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, 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. P. Coulon, E. Cuoco, S. D'Antonio, V. Dattilo, M. Davier, R. Day, R. De Rosa, G. Debreczeni, W. Del Pozzo, L. Di Fiore, A. Di Lieto, M. Di Paolo Emilio, A. Di Virgilio, A. Dietz, M. Drago, G. Endröczi, V. Fafone, I. Ferrante, F. Fidecaro, I. Fiori, R. Flaminio, L. A. Forte, J. D. Fournier, J. Franc, S. Franco, S. Frasca, F. Frasconi, M. Galimberti, L. Gammaitoni, F. Garufi, M. E. Gáspár, G. Gemme, E. Genin, A. Gennai, A. Giazotto, R. Gouaty, M. Granata, C. Greverie, G. M. Guidi, J. F. Hayau, A. Heidmann, H. Heitmann, P. Hello, G. Hemming, P. Jaranowski, R. J.G. Jonker, M. Kasprzack, I. Kowalska, A. Królak, N. Leroy, N. Letendre, T. G.F. Li, N. Liguori, M. Lorenzini, V. Loriette, G. Losurdo, E. Majorana, I. Maksimovic, V. Malvezzi, N. Man, M. Mantovani, F. Marchesoni, F. Marion, J. Marque, F. Martelli, A. Masserot, C. Michel, L. Milano, Y. Minenkov, M. Mohan, N. Morgado, A. Morgia, S. Mosca, B. Mours, L. Naticchioni, F. Nocera, L. Palladino, C. Palomba, F. Paoletti, R. Paoletti, M. Parisi, A. Pasqualetti, R. Passaquieti, D. Passuello, G. Persichetti, F. Piergiovanni, M. Pietka, L. Pinard, R. Poggiani, M. Prato, G. A. Prodi, M. Punturo, P. Puppo, D. S. Rabeling, I. Racz, P. Rapagnani, V. Re, T. Regimbau, F. Ricci, F. Robinet, A. Rocchi, L. Rolland, R. Romano, D. Rosińska, P. Ruggi, B. Sassolas, D. Sentenac, L. Sperandio, R. Sturani, B. Swinkels, M. Tacca, L. Taffarello, A. P.M. Ter Braack, A. Toncelli, M. Tonelli, O. Torre, E. Tournefier, F. Travasso, G. Vajente, J. F.J. Van Den Brand, C. Van Den Broeck, S. Van Der Putten, M. Vasuth, M. Vavoulidis, G. Vedovato, D. Verkindt, F. Vetrano, A. Viceré, J. Y. Vinet, S. Vitale, H. Vocca, R. L. Ward, M. Was, K. Yamamoto, M. Yvert, A. Zadroźny, J. P. Zendri

^*Corresponding author for this work

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

Abstract (may include machine translation)

The data collected by a gravitational wave interferometer are inevitably affected by instrumental artefacts and environmental disturbances. In particular, for continuous gravitational wave (CW) studies it is important to detect narrow-band disturbances (the so-called "noise lines") during science runs, and to help scientists to identify and possibly remove or mitigate their sources. The NoEMi (Noise Frequency Event Miner) framework exploits some of the algorithms implemented for the CW search to identify, on a daily basis, the frequency lines observed in the Virgo science data and in a subset of the environmental sensors, looking for lines that match in frequency. A line tracker algorithm reconstructs the lines over time, and stores them in a database, which is made accesible via a web interface. We describe the workflow of NoEMi, providing examples of its use for the investigation of noise lines in past Virgo runs (VSR2, VSR3) and in the most recent run (VSR4).

Original language	English
Article number	012037
Journal	Journal of Physics: Conference Series
Volume	363
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/363/1/012037
State	Published - 2012
Externally published	Yes
Event	9th Edoardo Amaldi Conference on Gravitational Waves, Amaldi 9 and the 2011 Numerical Relativity - Data Analysis Meeting, NRDA 2011 - Cardiff, United Kingdom Duration: 10 Jul 2011 → 15 Jul 2011

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10.1088/1742-6596/363/1/012037

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., ... Zendri, J. P. (2012). The NoEMi (Noise Frequency Event Miner) framework. Journal of Physics: Conference Series, 363(1), Article 012037. https://doi.org/10.1088/1742-6596/363/1/012037

@article{e678f34bb4b644e6a6c3f80d9274a6e9,

title = "The NoEMi (Noise Frequency Event Miner) framework",

abstract = "The data collected by a gravitational wave interferometer are inevitably affected by instrumental artefacts and environmental disturbances. In particular, for continuous gravitational wave (CW) studies it is important to detect narrow-band disturbances (the so-called {"}noise lines{"}) during science runs, and to help scientists to identify and possibly remove or mitigate their sources. The NoEMi (Noise Frequency Event Miner) framework exploits some of the algorithms implemented for the CW search to identify, on a daily basis, the frequency lines observed in the Virgo science data and in a subset of the environmental sensors, looking for lines that match in frequency. A line tracker algorithm reconstructs the lines over time, and stores them in a database, which is made accesible via a web interface. We describe the workflow of NoEMi, providing examples of its use for the investigation of noise lines in past Virgo runs (VSR2, VSR3) and in the most recent run (VSR4).",

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 Bauer, {Th S.} and M. Bebronne and M. Bejger and Beker, {M. G.} and M. Bitossi and Bizouard, {M. A.} 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 T. Briant and A. Brillet and V. Brisson and T. Bulik and Bulten, {H. J.} 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 Cohadon, {P. F.} and Colacino, {C. N.} and J. Colas and A. Colla and M. Colombini and A. Conte and Coulon, {J. P.} and E. Cuoco and S. D'Antonio and V. Dattilo and M. Davier and R. Day and {De Rosa}, R. and G. Debreczeni and {Del Pozzo}, W. and {Di Fiore}, L. and {Di Lieto}, A. and {Di Paolo Emilio}, M. and {Di Virgilio}, A. and A. Dietz and M. Drago and G. Endr{\"o}czi and V. Fafone and I. Ferrante and F. Fidecaro and I. Fiori and R. Flaminio and Forte, {L. A.} and Fournier, {J. D.} and J. Franc and S. Franco and S. Frasca and F. Frasconi and M. Galimberti and L. Gammaitoni and F. Garufi and G{\'a}sp{\'a}r, {M. E.} and G. Gemme and E. Genin and A. Gennai and A. Giazotto and R. Gouaty and M. Granata and C. Greverie and Guidi, {G. M.} and Hayau, {J. F.} and A. Heidmann and H. Heitmann and P. Hello and G. Hemming and P. Jaranowski and Jonker, {R. J.G.} and M. Kasprzack and I. Kowalska and A. Kr{\'o}lak and N. Leroy and N. Letendre and Li, {T. G.F.} and N. Liguori and M. Lorenzini and V. Loriette and G. Losurdo and E. Majorana and I. Maksimovic and V. Malvezzi and N. Man and M. Mantovani and F. Marchesoni and F. Marion and J. Marque and F. Martelli and A. Masserot and C. Michel and L. Milano and Y. Minenkov and M. Mohan and N. Morgado and A. Morgia and S. Mosca and B. Mours and L. Naticchioni and F. Nocera and L. Palladino and C. Palomba and F. Paoletti and R. Paoletti and M. Parisi and A. Pasqualetti and R. Passaquieti and D. Passuello and G. Persichetti and F. Piergiovanni and M. Pietka and L. Pinard and R. Poggiani and M. Prato and Prodi, {G. A.} and M. Punturo and P. Puppo and Rabeling, {D. S.} and I. Racz and P. Rapagnani and V. Re and T. Regimbau and F. Ricci and F. Robinet and A. Rocchi and L. Rolland and R. Romano and D. Rosi{\'n}ska and P. Ruggi and B. Sassolas and D. Sentenac and L. Sperandio and R. Sturani and B. Swinkels and M. Tacca and L. Taffarello and {Ter Braack}, {A. P.M.} and A. Toncelli and M. Tonelli and O. Torre and E. Tournefier and F. Travasso and G. Vajente and {Van Den Brand}, {J. F.J.} and {Van Den Broeck}, C. and {Van Der Putten}, S. and M. Vasuth and M. Vavoulidis and G. Vedovato and D. Verkindt and F. Vetrano and A. Vicer{\'e} and Vinet, {J. Y.} and S. Vitale and H. Vocca and Ward, {R. L.} and M. Was and K. Yamamoto and M. Yvert and A. Zadro{\'z}ny and Zendri, {J. P.}",

year = "2012",

doi = "10.1088/1742-6596/363/1/012037",

language = "English",

volume = "363",

journal = "Journal of Physics: Conference Series",

issn = "1742-6588",

number = "1",

note = "9th Edoardo Amaldi Conference on Gravitational Waves, Amaldi 9 and the 2011 Numerical Relativity - Data Analysis Meeting, NRDA 2011 ; Conference date: 10-07-2011 Through 15-07-2011",

}

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, T, 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, Coulon, JP, Cuoco, E, D'Antonio, S, Dattilo, V, Davier, M, Day, R, De Rosa, R, Debreczeni, G, Del Pozzo, W, Di Fiore, L, Di Lieto, A, Di Paolo Emilio, M, Di Virgilio, A, Dietz, A, Drago, M, Endröczi, G, Fafone, V, Ferrante, I, Fidecaro, F, Fiori, I, Flaminio, R, Forte, LA, Fournier, JD, Franc, J, Franco, S, Frasca, S, Frasconi, F, Galimberti, M, Gammaitoni, L, Garufi, F, Gáspár, ME, Gemme, G, Genin, E, Gennai, A, Giazotto, A, Gouaty, R, Granata, M, Greverie, C, Guidi, GM, Hayau, JF, Heidmann, A, Heitmann, H, Hello, P, Hemming, G, Jaranowski, P, Jonker, RJG, Kasprzack, M, Kowalska, I, Królak, A, Leroy, N, Letendre, N, Li, TGF, Liguori, N, Lorenzini, M, Loriette, V, Losurdo, G, Majorana, E, Maksimovic, I, Malvezzi, V, Man, N, Mantovani, M, Marchesoni, F, Marion, F, Marque, J, Martelli, F, Masserot, A, Michel, C, Milano, L, Minenkov, Y, Mohan, M, Morgado, N, Morgia, A, Mosca, S, Mours, B, Naticchioni, L, Nocera, F, Palladino, L, Palomba, C, Paoletti, F, Paoletti, R, Parisi, M, Pasqualetti, A, Passaquieti, R, Passuello, D, Persichetti, G, Piergiovanni, F, Pietka, M, Pinard, L, Poggiani, R, Prato, M, Prodi, GA, Punturo, M, Puppo, P, Rabeling, DS, Racz, I, Rapagnani, P, Re, V, Regimbau, T, Ricci, F, Robinet, F, Rocchi, A, Rolland, L, Romano, R, Rosińska, D, Ruggi, P, Sassolas, B, Sentenac, D, Sperandio, L, Sturani, R, Swinkels, B, Tacca, M, Taffarello, L, Ter Braack, APM, Toncelli, A, Tonelli, M, Torre, O, Tournefier, E, Travasso, F, Vajente, G, Van Den Brand, JFJ, Van Den Broeck, C, Van Der Putten, S, Vasuth, M, Vavoulidis, M, Vedovato, G, Verkindt, D, Vetrano, F, Viceré, A, Vinet, JY, Vitale, S, Vocca, H, Ward, RL, Was, M, Yamamoto, K, Yvert, M, Zadroźny, A & Zendri, JP 2012, 'The NoEMi (Noise Frequency Event Miner) framework', Journal of Physics: Conference Series, vol. 363, no. 1, 012037. https://doi.org/10.1088/1742-6596/363/1/012037

TY - JOUR

T1 - The NoEMi (Noise Frequency Event Miner) framework

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, Th 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, 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 - Coulon, J. P.

AU - Cuoco, E.

AU - D'Antonio, S.

AU - Dattilo, V.

AU - Davier, M.

AU - Day, R.

AU - De Rosa, R.

AU - Debreczeni, G.

AU - Del Pozzo, W.

AU - Di Fiore, L.

AU - Di Lieto, A.

AU - Di Paolo Emilio, M.

AU - Di Virgilio, A.

AU - Dietz, A.

AU - Drago, M.

AU - Endröczi, G.

AU - Fafone, V.

AU - Ferrante, I.

AU - Fidecaro, F.

AU - Fiori, I.

AU - Flaminio, R.

AU - Forte, L. A.

AU - Fournier, J. D.

AU - Franc, J.

AU - Franco, S.

AU - Frasca, S.

AU - Frasconi, F.

AU - Galimberti, M.

AU - Gammaitoni, L.

AU - Garufi, F.

AU - Gáspár, M. E.

AU - Gemme, G.

AU - Genin, E.

AU - Gennai, A.

AU - Giazotto, A.

AU - Gouaty, R.

AU - Granata, M.

AU - Greverie, C.

AU - Guidi, G. M.

AU - Hayau, J. F.

AU - Heidmann, A.

AU - Heitmann, H.

AU - Hello, P.

AU - Hemming, G.

AU - Jaranowski, P.

AU - Jonker, R. J.G.

AU - Kasprzack, M.

AU - Kowalska, I.

AU - Królak, A.

AU - Leroy, N.

AU - Letendre, N.

AU - Li, T. G.F.

AU - Liguori, N.

AU - Lorenzini, M.

AU - Loriette, V.

AU - Losurdo, G.

AU - Majorana, E.

AU - Maksimovic, I.

AU - Malvezzi, V.

AU - Man, N.

AU - Mantovani, M.

AU - Marchesoni, F.

AU - Marion, F.

AU - Marque, J.

AU - Martelli, F.

AU - Masserot, A.

AU - Michel, C.

AU - Milano, L.

AU - Minenkov, Y.

AU - Mohan, M.

AU - Morgado, N.

AU - Morgia, A.

AU - Mosca, S.

AU - Mours, B.

AU - Naticchioni, L.

AU - Nocera, F.

AU - Palladino, L.

AU - Palomba, C.

AU - Paoletti, F.

AU - Paoletti, R.

AU - Parisi, M.

AU - Pasqualetti, A.

AU - Passaquieti, R.

AU - Passuello, D.

AU - Persichetti, G.

AU - Piergiovanni, F.

AU - Pietka, M.

AU - Pinard, L.

AU - Poggiani, R.

AU - Prato, M.

AU - Prodi, G. A.

AU - Punturo, M.

AU - Puppo, P.

AU - Rabeling, D. S.

AU - Racz, I.

AU - Rapagnani, P.

AU - Re, V.

AU - Regimbau, T.

AU - Ricci, F.

AU - Robinet, F.

AU - Rocchi, A.

AU - Rolland, L.

AU - Romano, R.

AU - Rosińska, D.

AU - Ruggi, P.

AU - Sassolas, B.

AU - Sentenac, D.

AU - Sperandio, L.

AU - Sturani, R.

AU - Swinkels, B.

AU - Tacca, M.

AU - Taffarello, L.

AU - Ter Braack, A. P.M.

AU - Toncelli, A.

AU - Tonelli, M.

AU - Torre, O.

AU - Tournefier, E.

AU - Travasso, F.

AU - Vajente, G.

AU - Van Den Brand, J. F.J.

AU - Van Den Broeck, C.

AU - Van Der Putten, S.

AU - Vasuth, M.

AU - Vavoulidis, M.

AU - Vedovato, G.

AU - Verkindt, D.

AU - Vetrano, F.

AU - Viceré, A.

AU - Vinet, J. Y.

AU - Vitale, S.

AU - Vocca, H.

AU - Ward, R. L.

AU - Was, M.

AU - Yamamoto, K.

AU - Yvert, M.

AU - Zadroźny, A.

AU - Zendri, J. P.

PY - 2012

Y1 - 2012

N2 - The data collected by a gravitational wave interferometer are inevitably affected by instrumental artefacts and environmental disturbances. In particular, for continuous gravitational wave (CW) studies it is important to detect narrow-band disturbances (the so-called "noise lines") during science runs, and to help scientists to identify and possibly remove or mitigate their sources. The NoEMi (Noise Frequency Event Miner) framework exploits some of the algorithms implemented for the CW search to identify, on a daily basis, the frequency lines observed in the Virgo science data and in a subset of the environmental sensors, looking for lines that match in frequency. A line tracker algorithm reconstructs the lines over time, and stores them in a database, which is made accesible via a web interface. We describe the workflow of NoEMi, providing examples of its use for the investigation of noise lines in past Virgo runs (VSR2, VSR3) and in the most recent run (VSR4).

AB - The data collected by a gravitational wave interferometer are inevitably affected by instrumental artefacts and environmental disturbances. In particular, for continuous gravitational wave (CW) studies it is important to detect narrow-band disturbances (the so-called "noise lines") during science runs, and to help scientists to identify and possibly remove or mitigate their sources. The NoEMi (Noise Frequency Event Miner) framework exploits some of the algorithms implemented for the CW search to identify, on a daily basis, the frequency lines observed in the Virgo science data and in a subset of the environmental sensors, looking for lines that match in frequency. A line tracker algorithm reconstructs the lines over time, and stores them in a database, which is made accesible via a web interface. We describe the workflow of NoEMi, providing examples of its use for the investigation of noise lines in past Virgo runs (VSR2, VSR3) and in the most recent run (VSR4).

UR - http://www.scopus.com/inward/record.url?scp=84862305318&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/363/1/012037

DO - 10.1088/1742-6596/363/1/012037

M3 - Conference article

AN - SCOPUS:84862305318

SN - 1742-6588

VL - 363

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

IS - 1

M1 - 012037

T2 - 9th Edoardo Amaldi Conference on Gravitational Waves, Amaldi 9 and the 2011 Numerical Relativity - Data Analysis Meeting, NRDA 2011

Y2 - 10 July 2011 through 15 July 2011

ER -

The NoEMi (Noise Frequency Event Miner) framework

Abstract (may include machine translation)

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