Authors
Richard Abbott, Thomas D Abbott, Fausto Acernese, K Ackley, C Adams, N Adhikari, Rana X Adhikari, VB Adya, C Affeldt, D Agarwal, M Agathos, K Agatsuma, N Aggarwal, OD Aguiar, L Aiello, A Ain, P Ajith, T Akutsu, S Albanesi, A Allocca, PA Altin, A Amato, C Anand, S Anand, A Ananyeva, SB Anderson, WG Anderson, M Ando, T Andrade, N Andres, T Andrić, SV Angelova, S Ansoldi, JM Antelis, S Antier, S Appert, Koji Arai, Koya Arai, Y Arai, S Araki, A Araya, MC Araya, JS Areeda, M Arène, N Aritomi, N Arnaud, SM Aronson, KG Arun, H Asada, Y Asali, G Ashton, Y Aso, M Assiduo, SM Aston, P Astone, F Aubin, C Austin, S Babak, F Badaracco, MKM Bader, C Badger, S Bae, Y Bae, AM Baer, S Bagnasco, Y Bai, L Baiotti, J Baird, R Bajpai, M Ball, G Ballardin, SW Ballmer, A Balsamo, G Baltus, S Banagiri, D Bankar, JC Barayoga, C Barbieri, BC Barish, D Barker, P Barneo, F Barone, B Barr, L Barsotti, M Barsuglia, D Barta, J Bartlett, MA Barton, I Bartos, R Bassiri, A Basti, M Bawaj, JC Bayley, AC Baylor, M Bazzan, B Bécsy, VM Bedakihale, M Bejger, I Belahcene, V Benedetto, D Beniwal, TF Bennett, JD Bentley, M BenYaala, F Bergamin, BK Berger, S Bernuzzi, CPL Berry, D Bersanetti, A Bertolini, J Betzwieser, D Beveridge, R Bhandare, U Bhardwaj, D Bhattacharjee, S Bhaumik, IA Bilenko, G Billingsley, S Bini, R Birney, O Birnholtz, S Biscans, M Bischi, S Biscoveanu, A Bisht, B Biswas, M Bitossi, M-A Bizouard, JK Blackburn, CD Blair, DG Blair, RM Blair, F Bobba, N Bode, M Boer, G Bogaert, M Boldrini, LD Bonavena, François Bondu, E Bonilla, R Bonnand, P Booker, BA Boom, R Bork, V Boschi, N Bose, S Bose, V Bossilkov, V Boudart, Y Bouffanais
Publication date
2021/12/15
Journal
Physical Review D
Volume
104
Issue
12
Pages
122004
Publisher
American Physical Society
Description
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 in gravitational waves …
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