We present the results of a search for long-duration gravitational wave transients in the data of the LIGO Hanford and LIGO Livingston second generation detectors between September 2015 and January 2016, with a total observational time of 49 d. The search targets gravitational wave transients of 10-500 s duration in a frequency band of 24-2048 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. No significant events were observed. As a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. We also show that the search is sensitive to sources in the Galaxy emitting at least similar to 10-8 M(circle dot)c(2) in gravitational waves.
All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run / Abbott, Bp; Abbott, R; Abbott, Td; Abernathy, Mr; Acernese, F; Ackley, K; Adams, C; Adams, T; Addesso, P; Adhikari, Rx; Adya, Vb; Affeldt, C; Agathos, M; Agatsuma, K; Aggarwal, N; Aguiar, Od; Aiello, L; Ain, A; Ajith, P; Allen, B; Allocca, A; Altin, Pa; Ananyeva, A; Anderson, Sb; Anderson, Wg; Appert, S; Arai, K; Araya, Mc; Areeda, Js; Arnaud, N; Arun, Kg; Ascenzi, S; Ashton, G; Ast, M; Aston, Sm; Astone, P; Aufmuth, P; Aulbert, C; Avila-Alvarez, A; Babak, S; Bacon, P; Bader, Mkm; Baker, Pt; Baldaccini, F; Ballardin, G; Ballmer, Sw; Barayoga, Jc; Barclay, Se; Barish, Bc; Barker, D; Barone, F; Barr, B; Barsotti, L; Barsuglia, M; Barta, D; Bartlett, J; Bartos, I; Bassiri, R; Basti, A; Batch, Jc; Baune, C; Bavigadda, V; Bazzan, M; Beer, C; Bejger, M; Belahcene, I; Belgin, M; Bell, As; Berger, Bk; Bergmann, G; Berry, Cpl; Bersanetti, D; Bertolini, A; Betzwieser, J; Bhagwat, S; Bhandare, R; Bilenko, Ia; Billingsley, G; Billman, Cr; Birch, J; Birney, R; Birnholtz, O; Biscans, S; Bisht, A; Bitossi, M; Biwer, C; Bizouard, Ma; Blackburn, Jk; Blackman, J; Blair, Cd; Blair, Dg; Blair, Rm; Bloemen, S; Bock, O; Boer, M; Bogaert, G; Bohe, A; Bondu, F; Bonnand, R; Boom, Ba; Bork, R; Boschi, V; Bose, S; Bouffanais, Y; Bozzi, A; Bradaschia, C; Brady, Pr; Braginsky, Vb; Branchesi, M; Brau, Je; Briant, T; Brillet, A; Brinkmann, M; Brisson, V; Brockill, P; Broida, Je; Brooks, Af; Brown, Da; Brown, Dd; Brown, Nm; Brunett, S; Buchanan, Cc; Buikema, A; Bulik, T; Bulten, Hj; Buonanno, A; Buskulic, D; Buy, C; Byer, Rl; Cabero, M; Cadonati, L; Cagnoli, G; Cahillane, C; Bustillo, Jc; Callister, Ta; Calloni, E; Camp, Jb; Canepa, M; Cannon, Kc; Cao, H; Cao, J; Capano, Cd; Capocasa, E; Carbognani, F; Caride, S; Diaz, Jc; Casentini, C; Caudill, S; Cavaglia, M; Cavalier, F; Cavalieri, R; Cella, G; Cepeda, Cb; Baiardi, Lc; Cerretani, G; Cesarini, E; Chamberlin, Sj; Chan, M; Chao, S; Charlton, P; Chassande-Mottin, E; Cheeseboro, Bd; Chen, Hy; Chen, Y; Cheng, Hp; Chincarini, A; Chiummo, A; Chmiel, T; Cho, Hs; Cho, M; Chow, Jh; Christensen, N; Chu, Q; Chua, Ajk; Chua, S; Chung, S; Ciani, G; Clara, F; Clark, Ja; Cleva, F; Cocchieri, C; Coccia, E; Cohadon, Pf; Colla, A; Collette, Cg; Cominsky, L; Constancio, M; Conti, L; Cooper, Sj; Corbitt, Tr; Cornish, N; Corsi, A; Cortese, S; Costa, Ca; Coughlin, Mw; Coughlin, Sb; Coulon, Jp; Countryman, St; Couvares, P; Covas, Pb; Cowan, Ee; Coward, Dm; Cowart, Mj; Coyne, Dc; Coyne, R; Creighton, Jde; Creighton, Td; Cripe, J; Crowder, Sg; Cullen, Tj; Cumming, A; Cunningham, L; Cuoco, E; Dal Canton, T; Danilishin, Sl; D'Antonio, S; Danzmann, K; Dasgupta, A; Costa, Cfd; Dattilo, V; Dave, I; Davier, M; Davies, Gs; Davis, D; Daw, Ej; Day, B; Day, R; De, S; Debra, D; Debreczeni, G; Degallaix, J; De Laurentis, M; Deleglise, S; Del Pozzo, W; Denker, T; Dent, T; Dergachev, V; De Rosa, R; Derosa, Rt; Desalvo, R; Devine, Rc; Dhurandhar, S; Diaz, Mc; Di Fiore, L; Di Girolamo, T; 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[10.1088/1361-6382/aaab76]
All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run
Abbott, BP; Abbott, R; Abbott, TD; Abernathy, MR; Acernese, F; Ackley, K; Adams, C; Adams, T; Addesso, P; Adhikari, RX; Adya, VB; Affeldt, C; Agathos, M; Agatsuma, K; Aggarwal, N; Aguiar, OD; Aiello, L; Ain, A; Ajith, P; Allen, B; Allocca, A; Altin, PA; Ananyeva, A; Anderson, SB; Anderson, WG; Appert, S; Arai, K; Araya, MC; Areeda, JS; Arnaud, N; Arun, KG; Ascenzi, S; Ashton, G; Ast, M; Aston, SM; Astone, P; Aufmuth, P; Aulbert, C; Avila-Alvarez, A; Babak, S; Bacon, P; Bader, MKM; Baker, PT; Baldaccini, F; Ballardin, G; Ballmer, SW; Barayoga, JC; Barclay, SE; Barish, BC; Barker, D; Barone, F; Barr, B; Barsotti, L; Barsuglia, M; Barta, D; Bartlett, J; Bartos, I; Bassiri, R; Basti, A; Batch, JC; Baune, C; Bavigadda, V; Bazzan, M; Beer, C; Bejger, M; Belahcene, I; Belgin, M; Bell, AS; Berger, BK; Bergmann, G; Berry, CPL; Bersanetti, D; Bertolini, A; Betzwieser, J; Bhagwat, S; Bhandare, R; Bilenko, IA; Billingsley, G; Billman, CR; Birch, J; Birney, R; Birnholtz, O; Biscans, S; Bisht, A; Bitossi, M; Biwer, C; Bizouard, MA; Blackburn, JK; Blackman, J; Blair, CD; Blair, DG; Blair, RM; Bloemen, S; Bock, O; Boer, M; Bogaert, G; Bohe, A; Bondu, F; Bonnand, R; Boom, BA; Bork, R; Boschi, V; Bose, S; Bouffanais, Y; Bozzi, A; Bradaschia, C; Brady, PR; Braginsky, VB; Branchesi, M; Brau, JE; Briant, T; Brillet, A; Brinkmann, M; Brisson, V; Brockill, P; Broida, JE; Brooks, AF; Brown, DA; Brown, DD; Brown, NM; Brunett, S; Buchanan, CC; Buikema, A; Bulik, T; Bulten, HJ; Buonanno, A; Buskulic, D; Buy, C; Byer, RL; Cabero, M; Cadonati, L; Cagnoli, G; Cahillane, C; Bustillo, JC; Callister, TA; Calloni, E; Camp, JB; Canepa, M; Cannon, KC; Cao, H; Cao, J; Capano, CD; Capocasa, E; Carbognani, F; Caride, S; Diaz, JC; Casentini, C; Caudill, S; Cavaglia, M; Cavalier, F; Cavalieri, R; Cella, G; Cepeda, CB; Baiardi, LC; Cerretani, G; Cesarini, E; Chamberlin, SJ; Chan, M; Chao, S; Charlton, P; Chassande-Mottin, E; Cheeseboro, BD; Chen, HY; Chen, Y; Cheng, HP; Chincarini, A; Chiummo, A; Chmiel, T; Cho, HS; Cho, M; Chow, JH; Christensen, N; Chu, Q; Chua, AJK; Chua, S; Chung, S; Ciani, G; Clara, F; Clark, JA; Cleva, F; Cocchieri, C; Coccia, E; Cohadon, PF; Colla, A; Collette, CG; Cominsky, L; Constancio, M; Conti, L; Cooper, SJ; Corbitt, TR; Cornish, N; Corsi, A; Cortese, S; Costa, CA; Coughlin, MW; Coughlin, SB; Coulon, JP; Countryman, ST; Couvares, P; Covas, PB; Cowan, EE; Coward, DM; Cowart, MJ; Coyne, DC; Coyne, R; Creighton, JDE; Creighton, TD; Cripe, J; Crowder, SG; Cullen, TJ; Cumming, A; Cunningham, L; Cuoco, E; Dal Canton, T; Danilishin, SL; D'Antonio, S; Danzmann, K; Dasgupta, A; Costa, CFD; Dattilo, V; Dave, I; Davier, M; Davies, GS; Davis, D; Daw, EJ; Day, B; Day, R; De, S; DeBra, D; Debreczeni, G; Degallaix, J; De Laurentis, M; Deleglise, S; Del Pozzo, W; Denker, T; Dent, T; Dergachev, V; De Rosa, R; DeRosa, RT; DeSalvo, R; Devine, RC; Dhurandhar, S; Diaz, MC; Di Fiore, L; Di Girolamo, T; Di Lieto, A; Di Pace, S; Di Palma, I; Di Virgilio, A; Doctor, Z; Dolique, V; Donovan, F; 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2018-01-01
Abstract
We present the results of a search for long-duration gravitational wave transients in the data of the LIGO Hanford and LIGO Livingston second generation detectors between September 2015 and January 2016, with a total observational time of 49 d. The search targets gravitational wave transients of 10-500 s duration in a frequency band of 24-2048 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. No significant events were observed. As a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. We also show that the search is sensitive to sources in the Galaxy emitting at least similar to 10-8 M(circle dot)c(2) in gravitational waves.
Citazione
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[10.1088/1361-6382/aaab76]
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Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione.
