We report on a new all-sky search for periodic gravitational waves in the frequency band 475-2000 Hz and with a frequency time derivative in the range of [-1.0, +0.1] x 10(-8) Hz/s. Potential signals could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. This search uses the data from Advanced LIGO's first observational run 01. No gravitational-wave signals were observed, and upper limits were placed on their strengths. For completeness, results from the separately published low-frequency search 20-475 Hz are included as well. Our lowest upper limit on worst-case (linearly polarized) strain amplitude h 0 is similar to 4 x 10(-25) near 170 Hz, while at the high end of our frequency range, we achieve a worst-case upper limit of 1.3 x 10(-24) . For a circularly polarized source (most favorable orientation), the smallest upper limit obtained is similar to 1.5 x 10(-25)
Full band all-sky search for periodic gravitational waves in the O1 LIGO data / Abbott, Bp; Abbott, R; Abbott, Td; Acernese, F; Ackley, K; Adams, C; Adams, T; Addesso, P; Adhikari, Rx; Adya, Vb; Affeldt, C; Afrough, M; Agarwal, B; Agathos, M; Agatsuma, K; Aggarwal, N; Aguiar, Od; Aiello, L; Ain, A; Allen, B; Allen, G; Allocca, A; Altin, Pa; Amato, A; Ananyeva, A; Anderson, Sb; Anderson, Wg; Angelova, Sv; Antier, S; Appert, S; Arai, K; Araya, Mc; Areeda, Js; Arnaud, N; Ascenzi, S; Ashton, G; Ast, M; Aston, Sm; Astone, P; Atallah, Dv; Aufmuth, P; Aulbert, C; Aultoneal, K; Austin, C; Avila-Alvarez, A; Babak, S; Bacon, P; Bader, Mkm; Bae, S; Baker, Pt; Baldaccini, F; Ballardin, G; Ballmer, Sw; Banagiri, S; Barayoga, Jc; Barclay, Se; Barish, Bc; Barker, D; Barkett, K; Barone, F; Barr, B; Barsotti, L; Barsuglia, M; Barta, D; Bartlett, J; Bartos, I; Bassiri, R; Basti, A; Batch, Jc; Bawaj, M; Bayley, Jc; Bazzan, M; Becsy, B; Beer, C; Bejger, M; Belahcene, I; Bell, As; Berger, Bk; Bergmann, G; Bero, Jj; 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; Biscoveanu, S; Bisht, A; Bitossi, M; Biwer, C; Bizouard, Ma; Blackburn, Jk; Blackman, J; Blair, Cd; Blair, Dg; Blair, Rm; Bloemen, S; Bock, O; Bode, N; Boer, M; Bogaert, G; Bohe, A; Bondu, F; Bonilla, E; Bonnand, R; Boom, Ba; Bork, R; Boschi, V; Bose, S; Bossie, K; Bouffanais, Y; Bozzi, A; Bradaschia, C; Brady, Pr; Branchesi, M; Brau, Je; Briant, T; Brillet, A; Brinkmann, M; Brisson, V; Brockill, P; Broida, Je; Brooks, Af; Brown, Da; Brown, Dd; 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; Canizares, P; Cannon, Kc; Cao, H; Cao, J; Capano, Cd; Capocasa, E; Carbognani, F; Caride, S; Carney, Mf; Diaz, Jc; Casentini, C; Caudill, S; Cavaglia, M; Cavalier, F; Cavalieri, R; Cella, G; Cepeda, Cb; Cerda-Duran, P; Cerretani, G; Cesarini, E; Chamberlin, Sj; Chan, M; Chao, S; Charlton, P; Chase, E; Chassande-Mottin, E; Chatterjee, D; Cheeseboro, Bd; Chen, Hy; Chen, X; Chen, Y; Cheng, Hp; Chia, Hy; Chincarini, A; Chiummo, A; Chmiel, T; Cho, Hs; Cho, M; Chow, Jh; Christensen, N; Chu, Q; Chua, Ajk; Chua, S; Chung, Akw; Chung, S; Ciani, G; Ciecielag, P; Ciolfi, R; Cirelli, Ce; Cirone, A; Clara, F; Clark, Ja; Clearwater, P; Cleva, F; Cocchieri, C; Coccia, E; Cohadon, Pf; Cohen, D; Colla, A; Collette, Cg; Cominsky, Lr; Constancio, M; Conti, L; Cooper, Sj; Corban, P; Corbitt, Tr; Cordero-Carrion, I; Corley, Kr; Cornish, N; Corsi, A; Cortese, S; Costa, Ca; Coughlin, Et; 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; Dalya, G; Danilishin, Sl; D'Antonio, S; 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[10.1103/PhysRevD.97.102003]
Full band all-sky search for periodic gravitational waves in the O1 LIGO data
Abbott, BP; Abbott, R; Abbott, TD; Acernese, F; Ackley, K; Adams, C; Adams, T; Addesso, P; Adhikari, RX; Adya, VB; Affeldt, C; Afrough, M; Agarwal, B; Agathos, M; Agatsuma, K; Aggarwal, N; Aguiar, OD; Aiello, L; Ain, A; Allen, B; Allen, G; Allocca, A; Altin, PA; Amato, A; Ananyeva, A; Anderson, SB; Anderson, WG; Angelova, SV; Antier, S; Appert, S; Arai, K; Araya, MC; Areeda, JS; Arnaud, N; Ascenzi, S; Ashton, G; Ast, M; Aston, SM; Astone, P ;Atallah, DV; Aufmuth, P; Aulbert, C; AultONeal, K; Austin, C; Avila-Alvarez, A; Babak, S; Bacon, P; Bader, MKM; Bae, S; Baker, PT; Baldaccini, F; Ballardin, G; Ballmer, SW; Banagiri, S; Barayoga, JC; Barclay, SE; Barish, BC; Barker, D; Barkett, K; Barone, F; Barr, B; Barsotti, L; Barsuglia, M; Barta, D; Bartlett, J; Bartos, I; Bassiri, R; Basti, A; Batch, JC; Bawaj, M; Bayley, JC; Bazzan, M; Becsy, B; Beer, C; Bejger, M; Belahcene, I; Bell, AS; Berger, BK; Bergmann, G; Bero, JJ; Berry, CPL; Bersanetti, D; Bertolini, A; Betzwieser, J; Bhagwat, S; Bhandare, R; 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Chamberlin, SJ; Chan, M; Chao, S; Charlton, P; Chase, E; Chassande-Mottin, E; Chatterjee, D; Cheeseboro, BD; Chen, HY; Chen, X; Chen, Y; Cheng, HP; Chia, HY; Chincarini, A; Chiummo, A; Chmiel, T; Cho, HS; Cho, M; Chow, JH; Christensen, N; Chu, Q; Chua, AJK; Chua, S; Chung, AKW; Chung, S; Ciani, G; Ciecielag, P; Ciolfi, R; Cirelli, CE; Cirone, A; Clara, F; Clark, JA; Clearwater, P; Cleva, F; Cocchieri, C; Coccia, E; Cohadon, PF; Cohen, D; Colla, A; Collette, CG; Cominsky, LR; Constancio, M; Conti, L; Cooper, SJ; Corban, P; Corbitt, TR; Cordero-Carrion, I; Corley, KR; Cornish, N; Corsi, A; Cortese, S; Costa, CA; Coughlin, ET; 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; Dalya, G; Danilishin, SL; D'Antonio, S; Danzmann, K; Dasgupta, A; Costa, CFD; Dattilo, V; Dave, I; Davier, M; Davis, D; 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2018
Abstract
We report on a new all-sky search for periodic gravitational waves in the frequency band 475-2000 Hz and with a frequency time derivative in the range of [-1.0, +0.1] x 10(-8) Hz/s. Potential signals could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. This search uses the data from Advanced LIGO's first observational run 01. No gravitational-wave signals were observed, and upper limits were placed on their strengths. For completeness, results from the separately published low-frequency search 20-475 Hz are included as well. Our lowest upper limit on worst-case (linearly polarized) strain amplitude h 0 is similar to 4 x 10(-25) near 170 Hz, while at the high end of our frequency range, we achieve a worst-case upper limit of 1.3 x 10(-24) . For a circularly polarized source (most favorable orientation), the smallest upper limit obtained is similar to 1.5 x 10(-25)
Citazione
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[10.1103/PhysRevD.97.102003]
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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.
