Search for gravitational waves from Scorpius X-1 in the first Advanced
LIGO observing run with a hidden Markov model

Abbott,; and Abbott, B. P.; and Abbott, R.; and Acernese, D.; and Ackley, F.; and Adams, K.; and Adams, C.; and Addesso, T.; and Adhikari, P.; and Adya, R. X.; and Affeldt, V. B.; and Afrough, C.; and Agarwal, M.; and Agatsuma, B.; and Aggarwal, K.; and Aguiar, N.; and Aiello, O. D.; and Ain, L.; and Ajith, A.; and Allen, P.; and Allen, B.; and Allocca, G.; and Almoubayyed, A.; and Altin, H.; and Amato, P. A.; and Ananyeva, A.; and Anderson, A.; and Anderson, S. B.; and Antier, W. G.; and Appert, S.; and Arai, S.; and Araya, K.; and Areeda, M. C.; and Arnaud, J. S.; and Arun, N.; and Ascenzi, K. G.; and Ashton, S.; and Ast, G.; and Aston, M.; and Astone, S. M.; and Aufmuth, P.; and Aulbert, P.; and AultONeal, C.; and Avila-Alvarez, K.; and Babak, A.; and Bacon, S.; and Bader, P.; and Bae, M. K. M.; and Baker, S.; and Baldaccini, P. T.; and Ballardin, F.; and Ballmer, G.; and Banagiri, S. W.; and Barayoga, S.; and Barclay, J. C.; and Barish, S. E.; and Barker, B. C.; and Barone, D.; and Barr, F.; and Barsotti, B.; and Barsuglia, L.; and Barta, M.; and Bartlett, D.; and Bartos, J.; and Bassiri, I.; and Basti, R.; and Batch, A.; and Baune, J. C.; and Bawaj, C.; and Bazzan, M.; and Becsy, M.; and Beer, B.; and Bejger, C.; and Belahcene, M.; and Bell, I.; and Berger, A. S.; and Bergmann, B. K.; and Berry, G.; and Bersanetti, C. P. L.; and Bertolini, D.; and Etienne, A.; and Betzwieser, Z. B.; and Bhagwat, J.; and Bhandare, S.; and Bilenko, R.; and Billingsley, I. A.; and Billman, G.; and Birch, C. R.; and Birney, J.; and Birnholtz, R.; and Biscans, O.; and Bisht, S.; and Bitossi, A.; and Biwer, M.; and Bizouard, C.; and Blackburn, M. A.; and Blackman, J. K.; and Blair, J.; and Blari, C. D.; and Blair, D. G.; and Bloemen, R. M.; and Bock, S.; and Bode, O.; and Boer, N.; and Bogaert, M.; and Bohe, G.; and Bondu, A.; and Bonnand, F.; and Boom, R.; and Bork, B. A.; and Boschi, R.; and Bose, V.; and Bouffanais, S.; and Bozzi, Y.; and Bradaschia, A.; and Brady, C.; and Braginsky, P. R.; and Branchesi, V. B.; and Brau, M.; and Briant, J. E.; and Brillet, T.; and Brinkmann, A.; and Brisson, M.; and Brockill, V.; and Broida, P.; and Brooks, J. E.; and Brown, A. F.; and Brown, D. A.; and Brown, D. D.; and Brunett, N. M.; and Buchanan, S.; and Buikema, C. C.; and Bulik, A.; and Bulten, T.; and Buonanno, H. J.; and Buskulic, A.; and Buy, D.; and Byer, C.; and Cabero, R. L.; and Cadonati, M.; and Cagnoli, L.; and Cahillane, G.; and Bustillo, C.; Calderon and Callister, J.; and Calloni, T. A.; and Camp, E.; and Canepa, J. B.; and Canizares, M.; and Cannon, P.; and Cao, C.; and Cao, H.; and Capano, J.; and Capocasa, C. D.; and Carbognani, E.; and Caride, F.; and Carney, S.; and Diaz, M. F.; Casanueva and Casentini, J.; and Caudill, C.; and Cavaglia, S.; and Cavalier, M.; and Cavalieri, F.; and Cella, R.; and Cepeda, G.; and Baiardi, C. B.; Cerboni and Cerretani, L.; and Cesarini, G.; and Chamberlin, E.; and Chan, S. J.; and Chao, M.; and Charlton, S.; and Chassande-Mottin, P.; and Chatterjee, E.; and Cheeseboro, D.; and Chen, B. D.; and Chen, H. Y.; and Cheng, Y.; and Chincarini, H. -. P.; and Chiummo, A.; and Chmiel, A.; and Cho, T.; and Cho, H. S.; and Chow, M.; and Christensen, J. H.; and Chu, N.; and Chua, Q.; and Chua, A. J. K.; and Chung, S.; and Chung, A. K. W.; and Ciani, S.; and Ciolfi, G.; and Cirelli, R.; and Cirone, C. E.; and Clara, A.; and Clark, F.; and Cleva, J. A.; and Cocchieri, F.; and Coccia, C.; and Cohadon, E.; and Colla, P. -. F.; and Collette, A.; and Cominsky, C. G.; and Constancio, R.; J. r.,; and Conti, M.; and Cooper, L.; and Corban, S. J.; and Corbitt, P.; and Corley, T. R.; and Cornish, K. R.; and Corsi, N.; and Cortese, A.; and Costa, S.; and Coughlin, C. A.; and Coughlin, M. W.; and Coulon, S. B.; and Countryman, J. -. P.; and Couvares, S. T.; and Covas, P.; and Cowan, P. B.; and Coward, E. E.; and Cowart, D. M.; and Coyne, M. J.; and Coyne, D. C.; and Creighton, R.; and Creighton, J. D. E.; and Cripe, T. D.; and Crowder, J.; and Cullen, S. G.; and Cumming, T. J.; and Cunningham, A.; and Cuoco, L.; and Dal Canton, E.; and Danilishin, T.; and D'Antonio, S. L.; and Danzmann, S.; and Dasgupta, K.; and Costa, A.; Da Silva and Dattilo, C. F.; and Dave, V.; and Davier, I.; and Davies, M.; and Davis, G. S.; and Daw, D.; and Day, E. J.; and De, B.; and Debra, S.; and Deelman, D.; and Degallaix, E.; and De Laurentis, J.; and Deleglise, M.; and Del Pozzo, S.; and Denker, W.; and Dent, T.; and Dergachev, T.; and De Rosa, V.; and DeRosa, R.; and DeSalvo, R. T.; and Devenson, R.; and Devine, J.; and Dhurandhar, R. C.; and Diaz, S.; and Di Fiore, M. C.; and Di Giovanni, L.; and Di Girolamo, M.; and Di Lieto, T.; and Di Pace, A.; and Di Palma, S.; and Di Renzo, I.; and Doctor, F.; and Dolique, Z.; and Donovan, V.; and Dooley, F.; and Doravari, K. L.; and Dorrington, S.; and Douglas, I.; and Alvarez, R.; Dovale and Downes, M.; and Drago, T. P.; and Drever, M.; and Driggers, R. W. P.; and Du, J. C.; and Ducrot, Z.; and Duncan, M.; and Dwyer, J.; and Edo, S. E.; and Edwards, T. B.; and Effler, M. C.; and Eggenstein, A.; and Ehrens, H. -. B.; and Eichholz, P.; and Eikenberry, J.; and Essick, S. S.; and Etzel, R. C.; and Evans, T.; and Evans, M.; and Factourovich, T. M.; and Fafone, M.; and Fair, V.; and Fairhurst, H.; and Fan, S.; and Farinon, X.; and Farr, S.; and Farr, B.; and Fauchon-Jones, W. M.; and Favata, E. J.; and Fays, M.; and Fehrmann, M.; and Feicht, H.; and Fejer, J.; and Fernandez-Galiana, M. M.; and Ferrante, A.; and Ferreira, I.; and Ferrini, E. C.; and Fidecaro, F.; and Fiori, F.; and Fiorucci, I.; and Fisher, D.; and Flaminio, R. P.; and Fletcher, R.; and Fong, M.; and Forsyth, H.; and Forsyth, P. W. F.; and Fournier, S. S.; and Frasca, J. -. D.; and Frasconi, S.; and Frei, F.; and Freise, Z.; and Frey, A.; and Frey, R.; and Fries, V.; and Fritschel, E. M.; and Frolov, P.; and Fulda, V. V.; and Fyffe, P.; and Gabbard, M.; and Gabel, H.; and Gadre, M.; and Gaebel, B. U.; and Gair, S. M.; and Gammaitoni, J. R.; and Ganija, L.; and Gaonkar, M. R.; and Garufi, S. G.; and Gaudio, F.; and Gaur, S.; and Gayathri, G.; and Gehrels, V.; and Gemme, N.; and Genin, G.; and Gennai, E.; and George, A.; and George, D.; and Gergely, J.; and Germain, L.; and Ghonge, V.; and Ghosh, S.; Abhirup and Ghosh,; Archisman and Ghosh,; and Giaime, S.; and Giardina, J. A.; and Giazotto, K. D.; and Gill, A.; and Glover, K.; and Goetz, L.; and Goetz, E.; and Gomes, R.; and Gonzalez, S.; and Castro, G.; Gonzalez and Gopakumar, J. M.; and Gorodetsky, A.; and Gossan, M. L.; and Gosselin, S. E.; and Gouaty, M.; and Grado, R.; and Graef, A.; and Granata, C.; and Grant, M.; and Gras, A.; and Gray, S.; and Greco, C.; and Green, G.; and Groot, A. 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doi:10.1103/PhysRevD.95.122003

Results are presented from a semicoherent search for continuous gravitational waves from the brightest low-mass X-ray binary, Scorpius X-1, using data collected during the first Advanced LIGO observing run. The search combines a frequency domain matched filter (Bessel-weighted F-statistic) with a hidden Markov model to track wandering of the neutron star spin frequency. No evidence of gravitational waves is found in the frequency range 60-650 Hz. Frequentist 95\% confidence strain upper limits, h(0)(95\%) = 4.0 x 10(-25), 8.3 x 10(-25), and 3.0 x 10(-25) for electromagnetically restricted source orientation, unknown polarization, and circular polarization, respectively, are reported at 106 Hz. They are <= 10 times higher than the theoretical torque-balance limit at 106 Hz.

Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model

Abbott;B. P. and Abbott;R. and Abbott;D. and Acernese;F. and Ackley;K. and Adams;C. and Adams;T. and Addesso;P. and Adhikari;R. X. and Adya;V. B. and Affeldt;C. and Afrough;M. and Agarwal;B. and Agatsuma;K. and Aggarwal;N. and Aguiar;O. D. and Aiello;L. and Ain;A. and Ajith;P. and Allen;B. and Allen;G. and Allocca;A. and Almoubayyed;H. and Altin;P. A. and Amato;A. and Ananyeva;A. and Anderson;S. B. and Anderson;W. G. and Antier;S. and Appert;S. and Arai;K. and Araya;M. C. and Areeda;J. S. and Arnaud;N. and Arun;K. G. and Ascenzi;S. and Ashton;G. and Ast;M. and Aston;S. M. and Astone;P. and Aufmuth;P. and Aulbert;C. and AultONeal;K. and Avila-Alvarez;A. and Babak;S. and Bacon;P. and Bader;M. K. M. and Bae;S. and Baker;P. T. and Baldaccini;F. and Ballardin;G. and Ballmer;S. W. and Banagiri;S. and Barayoga;J. C. and Barclay;S. E. and Barish;B. 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2017-01-01

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	Anno di pubblicazione
	
				2017
			
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				PHYSICAL REVIEW D
			
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				https://dx.doi.org/10.1103/PhysRevD.95.122003
			
	ID tipologia loginMiur
	
				262
			
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Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model

2017-01-01

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Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model

2017-01-01

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