The Virgo O3 run and the impact of the environment

被引：11

作者：

Acernese, F. ^{[1
,2
]}

Agathos, M. ^{[3
]}

Ain, A. ^{[4
]}

Albanesi, S. ^{[5
,6
]}

Allocca, A. ^{[2
,7
]}

Amato, A. ^{[8
]}

Andrade, T. ^{[9
]}

Andres, N. ^{[10
]}

Andres-Carcasona, M. ^{[11
,12
]}

Andric, T. ^{[13
]}

Ansoldi, S. ^{[14
,15
]}

Antier, S. ^{[16
,17
,18
]}

Apostolatos, T. ^{[19
]}

Appavuravther, E. Z. ^{[20
,21
]}

Arene, M. ^{[22
]}

Arnaud, N. ^{[23
,24
]}

Assiduo, M. ^{[25
,26
]}

Melo, S. Assis de Souza ^{[24
]}

Astone, P. ^{[27
]}

Aubin, F. ^{[26
]}

Avgitas, T. ^{[28
]}

Babak, S. ^{[22
]}

Badaracco, F. ^{[29
]}

Bader, M. K. M. ^{[30
]}

Bagnasco, S. ^{[6
]}

Baird, J. ^{[22
]}

Baka, T. ^{[31
]}

Ballardin, G. ^{[24
]}

Baltus, G. ^{[32
]}

Banerjee, B. ^{[13
]}

Barbieri, C. ^{[33
,34
,35
]}

Barneo, P. ^{[9
]}

Barone, F. ^{[2
,36
]}

Barsuglia, M. ^{[22
]}

Barta, D. ^{[37
]}

Basti, A. ^{[4
,38
]}

Bawaj, M. ^{[20
,39
]}

Bazzan, M. ^{[40
,41
]}

Beirnaert, F. ^{[42
]}

Bejger, M. ^{[43
]}

Belahcene, I ^{[23
]}

Benedetto, V ^{[44
]}

Berbel, M. ^{[45
]}

Bernuzzi, S. ^{[3
]}

Bersanetti, D. ^{[46
]}

Bertolini, A. ^{[30
]}

Bhardwaj, U. ^{[17
,18
,30
]}

Bianchi, A. ^{[30
,47
]}

Bini, S. ^{[48
,49
]}

Bischi, M. ^{[25
,26
]}

机构：

[1] Univ Salerno, Dipartimento Farm, I-84084 Salerno, Italy

[2] Complesso Univ Monte S Angelo, Sez Napoli, Ist Nazl Fis Nucl, I-80126 Naples, Italy

[3] Friedrich Schiller Univ Jena, Theoret Phys Inst, D-07743 Jena, Germany

[4] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy

[5] Univ Torino, Dipartimento Fis, I-10125 Turin, Italy

[6] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy

[7] Univ Napoli Federico II, Complesso Univ Monte S Angelo, I-80126 Naples, Italy

[8] Univ Lyon, Univ Claude Bernard Lyon 1, Inst Lumiere Matiere, CNRS, F-69622 Villeurbanne, France

[9] Univ Barcelona, Inst Ciencies Cosmos ICCUB, C Marti i Franques 1, Barcelona 08028, Spain

[10] Univ Savoie Mt Blanc, Lab Annecy Phys Particules, CNRS, IN2P3, F-74000 Annecy, France

[11] Barcelona Inst Sci & Technol, Inst Fis Altes Energies IFAE, E-08193 Barcelona, Spain

[12] ICREA, E-08193 Barcelona, Spain

[13] Gran Sasso Sci Inst GSSI, I-67100 Laquila, Italy

[14] Univ Udine, Dipartimento Sci Matemat Informat & Fis, I-33100 Udine, Italy

[15] Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy

[16] Univ Cote Azur, Observ Cote Azur, CNRS, Artemis, F-06304 Nice, France

[17] Univ Amsterdam, Anton Pannekoek Inst Astron, GRAPPA, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[18] Univ Amsterdam, Inst High Energy Phys, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[19] Natl & Kapodistrian Univ Athens, Sch Sci Bldg,2nd Floor, Panepistimiopolis 15771, Ilissia, Greece

[20] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy

[21] Univ Camerino, Dipartimento Fis, I-62032 Camerino, Italy

[22] Univ Paris, Astroparticule & Cosmol, CNRS, F-75006 Paris, France

[23] Univ Paris Saclay, IJCLab, CNRS IN2P3, F-91405 Orsay, France

[24] European Gravitat Observ EGO, I-56021 Pisa, Italy

[25] Univ Urbino Carlo Bo, I-61029 Urbino, Italy

[26] Ist Nazl Fis Nucl, Sez Firenze, I-50019 Florence, Italy

[27] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy

[28] Univ Lyon, Univ Claude Bernard Lyon 1, CNRS, IP2I Lyon,IN2P3,UMR 5822, F-69622 Villeurbanne, France

[29] Catholic Univ Louvain, B-1348 Louvain La Neuve, Belgium

[30] Nikhef, Sci Pk 105, NL-1098 XG Amsterdam, Netherlands

[31] Univ Utrecht, Inst Gravitat & Subat Phys GRASP, Princetonpl 1, NL-3584 CC Utrecht, Netherlands

[32] Univ Liege, B-4000 Liege, Belgium

[33] Univ Milano Bicocca, I-20126 Milan, Italy

[34] Ist Nazl Fis Nucl, Sez Milano Bicocca, I-20126 Milan, Italy

[35] INAF, Osservatorio Astron Brera Sede Merate, I-23807 Merate, Lecco, Italy

[36] Univ Salerno, Scuola Med Salernitana, Dipartimento Med Chirurg & Odontoiatria, I-84081 Salerno, Italy

[37] RMKI, Wigner RCP, Konkoly Thege Miklos Ut 29-33, H-1121 Budapest, Hungary

[38] Univ Pisa, I-56127 Pisa, Italy

[39] Univ Perugia, I-06123 Perugia, Italy

[40] Univ Padua, Dipartimento Fis & Astron, I-35131 Padua, Italy

[41] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy

[42] Univ Ghent, B-9000 Ghent, Belgium

[43] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, PL-00716 Warsaw, Poland

[44] Univ Sannio, Dipartimento Ingn, I-82100 Benevento, Italy

[45] Univ Autonoma Barcelona, Fac Ciencias, Dept Matemat, Edificio C, Bellaterra 08193, Barcelona, Spain

[46] Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy

[47] Vrije Univ Amsterdam, NL-1081 HV Amsterdam, Netherlands

[48] Univ Trento, Dipartimento Fis, I-38123 Trento, Italy

[49] Trento Inst Fundamental Phys & Applicat, Ist Nazl Fis Nucl, I-38123 Povo, Trento, Italy

[50] Univ Salerno, Dipartimento Fis ER Caianiello, I-84084 Salerno, Italy

来源：

CLASSICAL AND QUANTUM GRAVITY | 2022年 / 39卷 / 23期

基金：

匈牙利科学研究基金会;

关键词：

Advanced Virgo detector; gravitational waves; interferometer; observing run 3; environmental monitoring; environment impact; sensitivity and duty cycle; MONITORING-SYSTEM; ANTENNA;

D O I：

10.1088/1361-6382/ac776a

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Sources of geophysical noise (such as wind, sea waves and earthquakes) or of anthropogenic noise impact ground-based gravitational-wave interferometric detectors, causing transient sensitivity worsening and gaps in data taking. During the one year-long third observing run (O3: from April 01, 2019 to March 27, 2020), the Virgo Collaboration collected a statistically significant dataset, used in this article to study the response of the detector to a variety of environmental conditions. We correlated environmental parameters to global detector performance, such as observation range, duty cycle and control losses. Where possible, we identified weaknesses in the detector that will be used to elaborate strategies in order to improve Virgo robustness against external disturbances for the next data taking period, O4, currently planned to start at the end of 2022. The lessons learned could also provide useful insights for the design of the next generation of ground-based interferometers.

引用

页数：40

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