All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run

Abbott,; and Abbott, B. P.; and Abbott, R.; and Abernathy, T. D.; and Acernese, M. R.; and Ackley, F.; and Adams, K.; and Adams, C.; and Addesso, T.; and Adhikari, P.; and Adya, R. X.; and Affeldt, V. B.; and Agathos, C.; and Agatsuma, M.; and Aggarwal, K.; and Aguiar, N.; and Aiello, O. D.; and Ain, L.; and Ajith, A.; and Allen, P.; and Allocca, B.; and Altin, A.; and Ananyeva, P. A.; and Anderson, A.; and Anderson, S. B.; and Appert, W. G.; 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 Avila-Alvarez, C.; and Babak, A.; and Bacon, S.; and Bader, P.; and Baker, M. K. M.; and Baldaccini, P. T.; and Ballardin, F.; and Ballmer, G.; and Barayoga, S. W.; 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 Bavigadda, C.; and Bazzan, V.; and Beer, M.; and Bejger, C.; and Belahcene, M.; and Belgin, I.; and Bell, M.; 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 Boer, O.; 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 Cannon, M.; and Cao, K. C.; and Cao, H.; and Capano, J.; and Capocasa, C. D.; and Carbognani, E.; and Caride, F.; and Diaz, S.; 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. 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doi:10.1088/1361-6382/aaab76

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.