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author = "Abbott, R. and Abbott, T. D. and Abraham, S. and Acernese, F. and
Ackley, K. and Adams, A. and Adams, C. and Adhikari, R. X. and
Adya, V. B. and Affeldt, C. and Agathos, M. and Agatsuma, K. and
Aggarwal, N. and Aguiar, Odylio Denys de and Aiello, L. and Ain,
A. and Ajith, P. and Akcay, S. and Allen, G. and Allocca, A. and
Altin, P. A. and Amato, A. and Anand, S. and Ananyeva, A. and
Anderson, S. B. and Anderson, W. G. and Angelova, S. V. and
Ansoldi, S. and Antelis, J. M. and Antier, S. and Appert, S. and
Arai, K. and Araya, M. C. and Areeda, J. S. and Ar{\`e}ne, M. and
Arnaud, N. and Aronson, S. M. and Arun, K. G. and Asali, Y. and
Ascenzi, S. and Ashton, G. and Aston, S. M. and Astone, P. and
Aubin, F. and Aufmuth, P. and Aultoneal, K. and Austin, C. and
Avendano, V. and Babak, S. and Badaracco, F. and Bader, M. K. M.
and Bae, S. and Baer, A. M. and Bagnasco, S. and Baird, J. and
Ball, M. and Ballardin, G. and Ballmer, S. W. and Bals, A. and
Balsamo, A. and Baltus, G. and Banagiri, S. and Bankar, D. and
Bankar, R. S. and Barayoga, J. C. and Barbieri, C. and Barish, B.
C. and Barker, D. and Barneo, P. and Barnum, S. and Barone, F. and
Barr, B. and Barsotti, L. and Barsuglia, M. and Barta, D. and
Bartlett, J. and Bartos, I. and Bassiri, R. and Basti, A. and
Bawaj, M. and Bayley, J. C. and Bazzan, M. and Becher, B. R. and
B{\'e}csy, B. and Bedakihale, V. M. and Bejger, M. and Belahcene,
I. and Beniwal, D. and Benjamin, M. G. and Benkel, R. and Bennett,
T. F. and Bentley, J. D. and Bergamin, F. and Berger, B. K. and
Bergmann, G. and Bernuzzi, S. and Berry, C. P. L. and Bersanetti,
D. and Bertolini, A. and Betzwieser, J. and Bhandare, R. and
Bhandari, A. V. and Bhattacharjee, D. and Bidler, J. and Bilenko,
I. A. and Billingsley, G. and Birney, R. and Birnholtz, O. and
Biscans, S. and Bischi, M. and Biscoveanu, S. and Bisht, A. and
Bitossi, M. and Bizouard, M. -A. and Blackburn, J. K. and
Blackman, J. and Blair, C. D. and Blair, D. G. and Blair, R. M.
and Blanch, O. and Bobba, F. and Bode, N. and Boer, M. and
Boetzel, Y. and Bogaert, G. and Boldrini, M. and Bondu, F. and
Bonilla, E. and Bonnand, R. and Booker, P. and Boom, B. A. and
Borhanian, S. and Bork, R. and Boschi, V. and Bose, N. and Bose,
S. and Bossilkov, V. and Boudart, V. and Bouffanais, Y. and Bozzi,
A. and Bradaschia, C. and Brady, P. R. and Bramley, A. and
Branchesi, M. and Brau, J. E. and Breschi, M. and Briant, T. and
Briggs, J. H. and Brighenti, F. and Brillet, A. and Brinkmann, M.
and Brito, R. and Brockill, P. and Brooks, A. F. and Brooks, J.
and Brown, D. D. and Brunett, S. and Bruno, G. and Bruntz, R. and
Buikema, A. and Bulik, T. and Bulten, H. J. and Buonanno, A. and
Buskulic, D. and Byer, R. L. and Cabero, M. and Cadonati, L. and
Caesar, M. and Cagnoli, G. and Cahillane, C. and Bustillo, J. C.
and Callaghan, J. D. and Callister, T. A. and Calloni, E. and
Camp, J. B. and Canepa, M. and Cannon, K. C. and Cao, H. and Cao,
J. and Carapella, G. and Carbognani, F. and Carney, M. F. and
Carpinelli, M. and Carullo, G. and Carver, T. L. and Diaz, J. C.
and Casentini, C. and Caudill, S. and Cavagli{\~A}, M. and
Cavalier, F. and Cavalieri, R. and Cella, G. and
Cerd{\'a}-Dur{\'a}n, P. and Cesarini, E. and Chaibi, W. and
Chakravarti, K. and Chan, C. -L. and Chan, C. and Chandra, K. and
Chanial, P. and Chao, S. and Charlton, P. and Chase, E. A. and
Chassande-Mottin, E. and Chatterjee, D. and Chaturvedi, M. and
Chatziioannou, K. and Chen, A. and Chen, H. Y. and Chen, X. and
Chen, Y. and Cheng, H. -P. and Cheong, C. K. and Chia, H. Y. and
Chiadini, F. and Chierici, R. and Chincarini, A. and Chiummo, A.
and Cho, G. and Cho, H. S. and Cho, M. and Choate, S. and
Christensen, N. and Chu, Q. and Chua, S. and Chung, K. W. and
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Corbitt, T. R. and Cordero-Carri{\'o}n, I. and Corezzi, S. and
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Cortese, S. and Costa, Cesar Augusto and Cotesta, R. and Coughlin,
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Cunningham, L. and Cuoco, E. and Curylo, M. and Dal Canton, T. and
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D'Angelo, B. and Danilishin, S. L. and D'Antonio, S. and Danzmann,
K. and Darsow-Fromm, C. and Dasgupta, A. and Datrier, L. E. H. and
Dattilo, V. and Dave, I. and Davier, M. and Davies, G. S. and
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and D'Emilio, V. and Demos, N. and Denker, T. and Dent, T. and
Depasse, A. and De Pietri, R. and De Rosa, R. and De Rossi, C. and
Desalvo, R. and De Varona, O. and Dhani, A. and Dhurandhar, S. and
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Dietrich, T. and Di Fiore, L. and Difronzo, C. and Di Giorgio, C.
and Di Giovanni, F. and Di Giovanni, M. and Di Girolamo, T. and Di
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and Edy, O. and Effler, A. and Eichholz, J. and Eikenberry, S. S.
and Eisenmann, M. and Eisenstein, R. A. and Ejlli, A. and Errico,
L. and Essick, R. C. and Estell{\'e}s, H. and Estevez, D. and
Etienne, Z. B. and Etzel, T. and Evans, M. and Evans, T. M. and
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Collaboration, (LIGO S and Collaboration), V",
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{} and {} and {} and {} and {} and {} and {} and {} and Ligo,
California Institute of Technology, Pasadena, CA 91125, United
States and Louisiana State University, Baton Rouge, LA 70803,
United States",
title = "All-sky search for long-duration gravitational-wave bursts in the
third Advanced LIGO and Advanced Virgo run",
journal = "Physical Review D",
year = "2021",
volume = "104",
number = "10",
pages = "e102001",
note = "{cited By 0}",
abstract = "After the detection of gravitational waves from compact binary
coalescences, the search for transient gravitational-wave signals
with less well-defined waveforms for which matched filtering is
not well suited is one of the frontiers for gravitational-wave
astronomy. Broadly classified into {"}short{"} less than or
similar to 1 s and {"}long{"} greater than or similar to 1 s
duration signals, these signals are expected from a variety of
astrophysical processes, including non-axisymmetric deformations
in magnetars or eccentric binary black hole coalescences. In this
work, we present a search for long-duration gravitational-wave
transients from Advanced LIGO and Advanced Virgo's third observing
run from April 2019 to March 2020. For this search, we use minimal
assumptions for the sky location, event time, waveform morphology,
and duration of the source. The search covers the range of 2-500 s
in duration and a frequency band of 24-2048 Hz. We find no
significant triggers within this parameter space; we report
sensitivity limits on the signal strength of gravitational waves
characterized by the root-sum-square amplitude h(rss) as a
function of waveform morphology. These hrss limits improve upon
the results from the second observing run by an average factor of
1.8.",
doi = "10.1103/PhysRevD.104.102001",
url = "http://dx.doi.org/10.1103/PhysRevD.104.102001",
issn = "1550-2368 and 1550-7998",
label = "20210628",
language = "en",
targetfile = "abbott_allsky_2021.pdf",
url = "https://www.scopus.com/inward/record.uri?eid=2-s2.0-85108209768\&doi=10.1103%2fPhysRevD.103.122002\&partnerID=40\&md5=2afc88279299b10b56e641010b5e8e79",
urlaccessdate = "27 abr. 2024"
}