All-sky search for periodic gravitational waves in the O1 LIGO data

Abbott,; and Abbott, B. P.; and Abbott, R.; and Acernese, T. 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 Altin, A.; 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 Ascenzi, N.; and Ashton, S.; and Ast, G.; and Aston, M.; and Astone, S. M.; and Aufmuth, R.; 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 Betzwieser, A.; 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 Blair, 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 Canister, J.; and Calloni, T. A.; and Camp, E.; and Canizares, J. B.; and Cannon, P.; and Cao, K. 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, I.; and Caudil, C.; and Cavaglia, S.; and Cavalier, M.; and Cavalieri, F.; and Cella, R.; and Cepeda, G.; and Baiardi, C. 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doi:10.1103/PhysRevD.96.062002

We report on an all-sky search for periodic gravitational waves in the frequency band 20-475 Hz and with a frequency time derivative in the range of [-1.0, +0.1] x 10(-8) Hz/s. Such a signal 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, O1. No periodic gravitational wave signals were observed, and upper limits were placed on their strengths. The lowest upper limits on worst-case (linearly polarized) strain amplitude h(0) are similar to 4 x 10(-25) near 170 Hz. For a circularly polarized source (most favorable orientation), the smallest upper limits obtained are similar to 1.5 x 10(-25). These upper limits refer to all sky locations and the entire range of frequency derivative values. For a population-averaged ensemble of sky locations and stellar orientations, the lowest upper limits obtained for the strain amplitude are similar to 2.5 x 10(-25).