@article{a41f64f73878491787541c4498367e4a,
title = "All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run",
abstract = " This paper presents the results of a search for generic short-duration gravitational-wave transients in data from the third observing run of Advanced LIGO and Advanced Virgo. Transients with durations of milliseconds to a few seconds in the 24--4096 Hz frequency band are targeted by the search, with no assumptions made regarding the incoming signal direction, polarization or morphology. Gravitational waves from compact binary coalescences that have been identified by other targeted analyses are detected, but no statistically significant evidence for other gravitational wave bursts is found. Sensitivities to a variety of signals are presented. These include updated upper limits on the source rate-density as a function of the characteristic frequency of the signal, which are roughly an order of magnitude better than previous upper limits. This search is sensitive to sources radiating as little as $\sim$10$^{-10} M_{\odot} c^2$ in gravitational waves at $\sim$70 Hz from a distance of 10~kpc, with 50\% detection efficiency at a false alarm rate of one per century. The sensitivity of this search to two plausible astrophysical sources is estimated: neutron star f-modes, which may be excited by pulsar glitches, as well as selected core-collapse supernova models. ",
keywords = "gr-qc, astro-ph.HE",
author = "{Virgo Collaboration} and C. Adams and Adhikari, {R. X.} and Blair, {C. D.} and S. Bose and H. Cao and C. Chen and Chen, {H. Y.} and J. Chen and X. Chen and Chen, {Y. -R.} and N. Christensen and Clark, {J. A.} and Collette, {C. G.} and L. Conti and Cullen, {T. J.} and Davis, {M. C.} and DeMarchi, {L. M.} and B. Ding and M. Gosselin and A. Grant and Y. Guo and J. Healy and G-Z Huang and H-Y Huang and Y-C Huang and Huang, {Y. -J.} and James, {A. L.} and K. Janssens and Jin, {H. -B.} and Jones, {D. I.} and Jonker, {R. J. G.} and T. Kaur and S. Khan and Kim, {W. S.} and Kim, {Y. -M.} and J. Lee and K. Lee and Li, {A. K. Y.} and B. Li and J. Li and Li, {K. L.} and Li, {T. G. F.} and X. Li and Liu, {G. C.} and J. Liu and K. Liu and X. Liu and A. Malik and M. Mantovani and Martin, {R. M.} and C. Michel and B. Miller and Ng, {S. W. S.} and C. Nguyen and P. Nguyen and T. Nguyen and H. Pan and M. Pinto and Richardson, {J. W.} and K. Ryan and M. Sakellariadou and Sanchez, {L. E.} and Sanders, {J. R.} and P. Schmidt and Sengupta, {A. S.} and P. Sharma and N. Singh and Smith, {R. J. E.} and K. Soni and V. Sordini and H. Sun and L. Sun and M. Thomas and P. Thomas and D. Tsai and D. Tsai and K. Turbang and Broeck, {C. Van Den} and T. Vo and S. Walsh and Wang, {J. Z.} and Wang, {J. Z.} and Wang, {W. H.} and White, {D. D.} and C. Wu and Wu, {D. S.} and H. Wu and S. Wu and L. Xiao and W-R Xu and L. Yang and Y. Yang and Z. Yang and H. Zhang and J. Zhang and L. Zhang and T. Zhang and Y. Zhang and C. Zhao and G. Zhao and Y. Zhao and Z. Zhou and Zhu, {X. J.} and Kevin Turbang",
note = "Funding Information: This material is based upon work supported by NSF\u2019s LIGO Laboratory which is a major facility fully funded by the National Science Foundation. The authors also gratefully acknowledge the support of Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Netherlands Organization for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the Spanish Agencia Estatal de Investigaci\u00F3n, the Vicepresid\u00E8ncia i Conselleria d\u2019Innovaci\u00F3, Recerca i Turisme and the Conselleria d\u2019Educaci\u00F3 i Universitat del Govern de les Illes Balears, the Conselleria d\u2019Innovaci\u00F3, Universitats, Ci\u00E8ncia i Societat Digital de la Generalitat Valenciana and the CERCA Programme Generalitat de Catalunya, Spain, the National Science Centre of Poland and the Foundation for Polish Science (FNP), the Swiss National Science Foundation (SNSF), the Russian Foundation for Basic Research, the Russian Science Foundation, the European Commission, the European Regional Development Funds (ERDF), the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the French Lyon Institute of Origins (LIO), the Belgian Fonds de la Recherche Scientifique (FRS-FNRS), Actions de Recherche Concert\u00E9es (ARC) and Fonds Wetenschappelijk Onderzoek\u2014Vlaanderen (FWO), Belgium, the Paris \u00CEle-de-France Region, the National Research, Development and Innovation Office Hungary (NKFIH), the National Research Foundation of Korea, the Natural Science and Engineering Research Council Canada, Canadian Foundation for Innovation (CFI), the Brazilian Ministry of Science, Technology, and Innovations, the International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), the Research Grants Council of Hong Kong, the National Natural Science Foundation of China (NSFC), the Leverhulme Trust, the Research Corporation, the Ministry of Science and Technology (MOST), Taiwan, the United States Department of Energy, and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, INFN and CNRS for provision of computational resources. This work was supported by MEXT, JSPS Leading-edge Research Infrastructure Program, JSPS Grant-in-Aid for Specially Promoted Research 26000005(Kajita 2014\u20132018), JSPS Grant-in-Aid for Scientific Research on Innovative Areas 2905: Grants No. JP17H06358, No. JP17H06361, and No. JP17H06364, JSPS Core-to-Core Program A. Advanced Research Networks, JSPS Grant-in-Aid for Scientific Research (S) Grants No. 17H06133 and No. 20H05639, JSPS Grant-in-Aid for Transformative Research Areas (A) 20A203: Grant No. JP20H05854, the joint research program of the Institute for Cosmic Ray Research, University of Tokyo, National Research Foundation (NRF) and Computing Infrastructure Project of KISTI-GSDC in Korea, Academia Sinica (AS), AS Grid Center (ASGC) and the Ministry of Science and Technology (MoST) in Taiwan under grants including Grant No. AS-CDA-105-M06, Advanced Technology Center (ATC) of NAOJ, Mechanical Engineering Center of KEK. Publisher Copyright: {\textcopyright} 2021 us.",
year = "2021",
month = dec,
day = "23",
doi = "10.1103/PhysRevD.104.122004",
language = "English",
volume = "104",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "12",
}