Noise subtraction from KAGRA O3GK data using Independent Component Analysis

被引：0

作者：

Abe, H. ^{[1
]}

Akutsu, T. ^{[2
,3
]}

Ando, M. ^{[4
,5
]}

Araya, A. ^{[6
]}

Aritomi, N. ^{[4
]}

Asada, H. ^{[7
]}

Aso, Y. ^{[8
,9
]}

Bae, S. ^{[10
]}

Bae, Y. ^{[11
]}

Bajpai, R. ^{[12
]}

Cannon, K. ^{[5
]}

Cao, Z. ^{[13
]}

Capocasa, E. ^{[2
]}

Chan, M. ^{[14
]}

Chen, C. ^{[15
,16
,17
]}

Chen, D. ^{[8
]}

Chen, K. ^{[18
]}

Chen, Y. ^{[16
]}

Chiang, C-Y ^{[19
]}

Chu, Y-K ^{[19
]}

Eguchi, S. ^{[14
]}

Eisenmann, M. ^{[2
]}

Enomoto, Y. ^{[4
]}

Flaminio, R. ^{[2
,20
]}

Fong, H. K. ^{[5
]}

Fujii, Y. ^{[21
]}

Fujikawa, Y. ^{[22
]}

Fujimoto, Y. ^{[23
]}

Fukunaga, I. ^{[23
]}

Gao, D. ^{[24
]}

Ge, G-G ^{[24
]}

Ha, S. ^{[25
]}

Hadiputrawan, I. P. W. ^{[18
]}

Haino, S. ^{[19
]}

Han, W-B ^{[26
]}

Hasegawa, K. ^{[27
]}

Hattori, K. ^{[28
]}

Hayakawa, H. ^{[29
]}

Hayama, K. ^{[14
]}

Himemoto, Y. ^{[30
]}

Hirata, N. ^{[2
]}

Hirose, C. ^{[22
]}

Ho, T-C ^{[18
]}

Hsieh, B-H ^{[27
]}

Hsieh, H-F ^{[17
]}

Hsiung, C. ^{[15
]}

Huang, H-Y ^{[19
]}

Huang, P. ^{[24
]}

Huang, Y-C ^{[16
]}

Huang, Y-J ^{[19
]}

机构：

[1] Tokyo Inst Technol, Grad Sch Sci, Meguro Ku, Tokyo 1528551, Japan

[2] NAOJ, Gravitat Wave Sci Project, Mitaka, Tokyo 1818588, Japan

[3] NAOJ, Adv Technol Ctr, Mitaka, Tokyo 1818588, Japan

[4] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan

[5] Univ Tokyo, Res Ctr Early Universe RESCEU, Bunkyo Ku, Tokyo 1130033, Japan

[6] Univ Tokyo, Earthquake Res Inst, Bunkyo Ku, Tokyo 1130032, Japan

[7] Hirosaki Univ, Dept Math & Phys, Gravitat Wave Sci Project, Hirosaki, Aomori 0368561, Japan

[8] NAOJ, Kamioka Branch, Kamioka Cho, Hida City, Gifu 5061205, Japan

[9] Grad Univ Adv Studies SOKENDAI, Mitaka, Tokyo 1818588, Japan

[10] KISTI, Daejeon 34141, South Korea

[11] Natl Inst Math Sci, Daejeon 34047, South Korea

[12] Grad Univ Adv Studies SOKENDAI, Sch High Energy Accelerator Sci, Tsukuba, Ibaraki 3050801, Japan

[13] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China

[14] Fukuoka Univ, Dept Appl Phys, Fukuoka, Fukuoka 8140180, Japan

[15] Tamkang Univ, Dept Phys, New Taipei 25137, Taiwan

[16] Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan

[17] Natl Tsing Hua Univ, Inst Astron, Hsinchu 30013, Taiwan

[18] Natl Cent Univ, Dept Phys, Ctr High Energy & High Field Phys, Taoyuan 32001, Taiwan

[19] Acad Sinica, Inst Phys, Taipei 11529, Taiwan

[20] Univ Grenoble Alpes, LAPP, Univ Savoie Mt Blanc, CNRS,IN2P3, F-74941 Annecy, France

[21] Univ Tokyo, Dept Astron, Mitaka, Tokyo 1818588, Japan

[22] Niigata Univ, Fac Engn, Nishi Ku, Niigata, Niigata 9502181, Japan

[23] Osaka City Univ, Grad Sch Sci, Dept Phys, Sumiyoshi Ku, Osaka, Osaka 5588585, Japan

[24] Chinese Acad Sci, Innovat Acad Precis Measurement Sci & Technol APM, State Key Lab Magnet Resonance & Atom & Mol Phys, Wuhan 430071, Peoples R China

[25] UNIST, Dept Phys, Ulsan 44919, South Korea

[26] Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China

[27] Univ Tokyo, ICRR, KAGRA Observ, Kashiwa, Chiba 2778582, Japan

[28] Univ Toyama, Fac Sci, Toyama, Toyama 9308555, Japan

[29] Univ Tokyo, ICRR, KAGRA Observ, Kamioka Cho, Hida City, Gifu 5061205, Japan

[30] Nihon Univ, Coll Ind Technol, Narashino, Chiba 2758575, Japan

[31] Chungnam Natl Univ, Dept Astron & Space Sci, Daejeon 34134, South Korea

[32] Aoyama Gakuin Univ, Dept Phys Sci, Sagamihara, Kanagawa 2525258, Japan

[33] Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China

[34] Univ Toyama, Grad Sch Sci & Engn, Toyama, Toyama 9308555, Japan

[35] Osaka City Univ, Nambu Yoichiro Inst Theoret & Expt Phys NITEP, Sumiyoshi Ku, Osaka, Osaka 5588585, Japan

[36] Ewha Womans Univ, Dept Phys, Seoul 03760, South Korea

[37] Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China

[38] Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing, Peoples R China

[39] Univ Tokyo, ICRR, Kashiwa, Chiba 2778582, Japan

[40] Myongji Univ, Dept Phys, Yongin 17058, South Korea

[41] Inje Univ, Dept Comp Simulat, Gimhae 50834, Gyeongsangnam D, South Korea

[42] High Energy Accelerator Res Org KEK, IPNS, Tsukuba, Ibaraki 3050801, Japan

[43] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales

[44] Inst Fis Teor CA, C Nicolas Cabrera 13-15, Madrid 1315, Spain

[45] Nagoya Univ, Dept Phys, Chikusa Ku, Nagoya, Aichi 4648602, Japan

[46] Natl Cheng Kung Univ, Dept Phys, Tainan 701, Taiwan

[47] Wuhan Univ, Sch Phys & Technol, Wuhan 430072, Hubei, Peoples R China

[48] Natl Ctr High Performance Comp, Natl Appl Res Labs, Hsinchu Sci Pk, Hsinchu 30076, Taiwan

[49] Natl Taiwan Normal Univ, Sect 4, Dept Phys, Taipei 116, Taiwan

[50] Univ Roma La Sapienza, INFN, I-00185 Rome, Italy

来源：

CLASSICAL AND QUANTUM GRAVITY | 2023年 / 40卷 / 08期

基金：

新加坡国家研究基金会;

关键词：

gravitational wave; data analysis; noise subtraction; independent component analysis; SEPARATION;

D O I：

10.1088/1361-6382/acc0cb

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

During April 7-21 2020, KAGRA conducted its first scientific observation in conjunction with the GEO600 detector. The dominant noise sources during this run were found to be suspension control noise in the low-frequency range and acoustic noise in the mid-frequency range. In this study, we show that their contributions in the observational data can be reduced by a signal processing method called independent component analysis (ICA). The model of ICA is extended from that studied in the initial KAGRA data analysis to account for frequency dependence, while the linearity and stationarity of the coupling between the interferometer and the noise sources are still assumed. We identify optimal witness sensors in the application of ICA, leading to successful mitigation of these two dominant contributions. We also analyze the stability of the transfer functions for the entire two weeks of data to investigate the applicability of the proposed subtraction method in gravitational wave searches.

引用

页数：24

共 50 条

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Aritomi, N.
Asada, H.
Aso, Y.
Bae, S.
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