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author = "Abbott, B. P. and Abbott, R. and Abbott, T. D. and Abraham, S. and
Acernese, F. and Ackley, K. and Adams, C. and Adya, V. B. and
Affeldt, C. and Agathos, M. and Agatsuma, K. and Aggarwal, N. and
Aguiar, Odylio Denys de and Aiello, L. and Ain, A. and Ajith, P.
and Allen, G. and Allocca, A. and Aloy, M. A. and Altin, P. A. and
Amato, A. and Ananyeva, A. and Anderson, S. B. and Anderson, W. G.
and Angelova, S. V. and Antier, S. and Appert, S. and Arai, K. and
Araya, M. C. and Areeda, J. S. and Ar{\`e}ne, M. and Arnaud, N.
and Arun, K. G. and Ascenzi, S. and Ashton, G. and Aston, S. M.
and Astone, P. and Aubin, F. and Aufmuth, P. and Aultoneal, K. and
Austin, C. and Avendano, V. and Avila-Alvarez, A. and Babak, S.
and Bacon, P. and Badaracco, F. 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. C. and Barker, D. and Barkett, K. and Barnum, S. and
Barone, F. and Barr, B. and Barsotti, L. and Barsuglia, M. and
Barta, D. and Bartlett, J. and Bartos, I. and Bassiri, R. and
Basti, A. and Bawaj, M. and Bayley, J. C. and Bazzan, M. and
B{\'e}csy, B. and Bejger, M. and Belahcene, I. and Bell, A. S.
and Beniwal, D. and Berger, B. K. and Bergmann, G. and Bernuzzi,
S. and Bero, J. J. and Berry, C. P. L. and Bersanetti, D. and
Bertolini, A. and Betzwieser, J. and Bhandare, R. and Bidler, J.
and Bilenko, I. A. and Bilgili, S. A. and Billingsley, G. and
Birch, J. and Birney, R. and Birnholtz, O. and Biscans, S. and
Biscoveanu, S. and Bisht, A. and Bitossi, M. and Bizouard, M. A.
and Blackburn, J. K. and Blair, C. D. and Blair, D. G. and Blair,
R. M. and Bloemen, S. and Bode, N. and Boer, M. and Boetzel, Y.
and Bogaert, G. and Bondu, F. and Bonilla, E. and Bonnand, R. and
Booker, P. and Boom, B. A. and Booth, C. D. and Bork, R. and
Boschi, V. and Bose, S. and Bossie, K. and Bossilkov, V. and
Bosveld, J. and Bouffanais, Y. and Bozzi, A. and Bradaschia, C.
and Brady, P. R. and Bramley, A. and Branchesi, M. and Brau, J. E.
and Briant, T. and Briggs, J. H. and Brighenti, F. and Brillet, A.
and Brinkmann, M. and Brisson, V. and Brockill, P. and Brooks, A.
F. and Brown, D. D. and Brunett, S. and Buikema, A. and Bulik, T.
and Bulten, H. J. and Buonanno, A. and Buskulic, D. and Buy, C.
and Byer, R. L. and Cabero, M. and Cadonati, L. and Cagnoli, G.
and Cahillane, C. and Calder{\'o}n Bustillo, J. and Callister, T.
A. and Calloni, E. and Camp, J. B. and Campbell, W. A. and Canepa,
M. and Cannon, K. C. and Cao, H. and Cao, J. and Capocasa, E. and
Carbognani, F. and Caride, S. and Carney, M. F. and Carullo, G.
and Casanueva Diaz, J. and Casentini, C. and Caudill, S. and
Cavagli{\~A}, M. and Cavalier, F. and Cavalieri, R. and Cella, G.
and Cerd{\'a}-Dur{\'a}n, P. and Cerretani, G. and Cesarini, E.
and Chaibi, O. and Chakravarti, K. and Chamberlin, S. J. and Chan,
M. and Chao, S. and Charlton, P. and Chase, E. A. and
Chassande-Mottin, E. and Chatterjee, D. and Chaturvedi, M. and
Cheeseboro, B. D. and Chen, H. Y. and Chen, X. and Chen, Y. and
Cheng, H. -P. and Cheong, C. K. and Chia, H. Y. and Chincarini, A.
and Chiummo, A. and Cho, G. and Cho, H. S. and Cho, M. and
Christensen, N. and Chu, Q. and Chua, S. and Chung, K. W. and
Chung, S. and Ciani, G. and Ciobanu, A. A. and Ciolfi, R. and
Cipriano, F. and Cirone, A. and Clara, F. and Clark, J. A. and
Clearwater, P. and Cleva, F. and Cocchieri, C. and Coccia, E. and
Cohadon, P. -F. and Cohen, D. and Colgan, R. and Colleoni, M. and
Collette, C. G. and Collins, C. and Cominsky, L. R. and Constancio
J{\'u}nior, M{\'a}rcio and Conti, L. and Cooper, S. J. and
Corban, P. and Corbitt, T. R. and Cordero-Carri{\'o}n, I. and
Corley, K. R. and Cornish, N. and Corsi, A. and Cortese, S. and
Costa, C{\'e}sar Augusto and Cotesta, R. and Coughlin, M. W. and
Coughlin, S. B. and Coulon, J. -P. and Countryman, S. T. and
Couvares, P. and Covas, P. B. and Cowan, E. E. and Coward, D. M.
and Cowart, M. J. and Coyne, D. C. and Coyne, R. and Creighton, J.
D. E. and Creighton, T. D. and Cripe, J. and Croquette, M. and
Crowder, S. G. and Cullen, T. J. and Cumming, A. and Cunningham,
L. and Cuoco, E. and Canton, T. D. and D{\'a}lya, G. and
Danilishin, S. L. and D'antonio, S. and Danzmann, K. and Dasgupta,
A. and Da Silva Costa, C. F. and Datrier, L. E. H. and Dattilo, V.
and Dave, I. and Davier, M. and Davis, D. and Daw, E. J. and
Debra, D. and Deenadayalan, M. and Degallaix, J. and De Laurentis,
M. and Del{\'e}glise, S. and Del Pozzo, W. and Demarchi, L. M.
and Demos, N. and Dent, T. and De Pietri, R. and Derby, J. and De
Rosa, R. and De Rossi, C. and Desalvo, R. and De Varona, O. and
Dhurandhar, S. and D{\'{\i}}az, M. C. and Dietrich, T. and Di
Fiore, L. and Di Giovanni, M. and Di Girolamo, T. and Di Lieto, A.
and Ding, B. and Di Pace, S. and Di Palma, I. and Di Renzo, F. and
Dmitriev, A. and Doctor, Z. and Donovan, F. and Dooley, K. L. and
Doravari, S. and Dorrington, I. and Downes, T. P. and Drago, M.
and Driggers, J. C. and Du, Z. and Ducoin, J. -G. and Dupej, P.
and Dvorkin, I. and Dwyer, S. E. and Easter, P. J. and Edo, T. B.
and Edwards, M. C. and Effler, A. and Ehrens, P. and Eichholz, J.
and Eikenberry, S. S. and Eisenmann, M. and Eisenstein, R. A. and
Essick, R. C. and Estelles, H. and Estevez, D. and Etienne, Z. B.
and Etzel, T. and Evans, M. and Evans, T. M. and Fafone, V. and
Fair, H. and Fairhurst, S. and Fan, X. and Farinon, S. and Farr,
B. and Farr, W. M. and Fauchon-Jones, E. J. and Favata, M. and
Fays, M. and Fazio, M. and Fee, C. and Feicht, J. and Fejer, M. M.
and Feng, F. and Fernandez-Galiana, A. and Ferrante, I. and
Ferreira, Elvis Camilo and Ferreira, Tabata Aira and Ferrini, F.
and Fidecaro, F. and Fiori, I. and Fiorucci, D. and Fishbach, M.
and Fisher, R. P. and Fishner, J. M. and Fitz-Axen, M. and
Flaminio, R. and Fletcher, M. and Flynn, E. and Fong, H. and Font,
J. A. and Forsyth, P. W. F. and Fournier, J. -D. and Frasca, S.
and Frasconi, F. and Frei, Z. and Freise, A. and Frey, R. and
Frey, V. and Fritschel, P. and Frolov, V. V. and Fulda, P. and
Fyffe, M. and Gabbard, H. A. and Gadre, B. U. and Gaebel, S. M.
and Gair, J. R. and Gammaitoni, L. and Ganija, M. R. and Gaonkar,
S. G. and Garcia, A. and Garc{\'{\i}}a-Quir{\'o}s, C. and
Garufi, F. and Gateley, B. and Gaudio, S. and Gaur, G. and
Gayathri, V. and Gemme, G. and Genin, E. and Gennai, A. and
George, D. and George, J. and Gergely, L. and Germain, V. and
Ghonge, S. and Ghosh, A. and Ghosh, A. and Ghosh, S. and
Giacomazzo, B. and Giaime, J. A. and Giardina, K. D. and Giazotto,
A. and Gill, K. and Giordano, G. and Glover, L. and Godwin, P. and
Goetz, E. and Goetz, R. and Goncharov, B. and Gonz{\'a}lez, G.
and Gonzalez Castro, J. M. and Gopakumar, A. and Gorodetsky, M. L.
and Gossan, S. E. and Gosselin, M. and Gouaty, R. and Grado, A.
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and Grunewald, S. and Gruning, P. and Guidi, G. M. and Gulati, H.
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and Gustafson, R. and Haegel, L. and Halim, O. and Hall, B. R. and
Hall, E. D. and Hamilton, E. Z. and Hammond, G. and Haney, M. and
Hanke, M. M. and Hanks, J. and Hanna, C. and Hannuksela, O. A. and
Hanson, J. and Hardwick, T. and Haris, K. and Harms, J. and Harry,
G. M. and Harry, I. W. and Haster, C. -J. and Haughian, K. and
Hayes, F. J. and Healy, J. and Heidmann, A. and Heintze, M. C. and
Heitmann, H. and Hello, P. and Hemming, G. and Hendry, M. and
Heng, I. S. and Hennig, J. and Heptonstall, A. W. and Hernandez
Vivanco, F. and Heurs, M. and Hild, S. and Hinderer, T. and Hoak,
D. and Hochheim, S. and Hofman, D. and Holgado, A. M. and Holland,
N. A. and Holt, K. and Holz, D. E. and Hopkins, P. and Horst, C.
and Hough, J. and Howell, E. J. and Hoy, C. G. and Hreibi, A. and
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S. and Huttner, S. H. and Huynh-Dinh, T. and Idzkowski, B. and
Iess, A. and Ingram, C. and Inta, R. and Intini, G. and Irwin, B.
and Isa, H. N. and Isac, J. -M. and Isi, M. and Iyer, B. R. and
Izumi, K. and Jacqmin, T. and Jadhav, S. J. and Jani, K. and
Janthalur, N. N. and Jaranowski, P. and Jenkins, A. C. and Jiang,
J. and Johnson, D. S. and Jones, A. W. and Jones, D. I. and Jones,
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C. V. and Kalogera, V. and Kamai, B. and Kandhasamy, S. and Kang,
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S. and Katsavounidis, E. and Katzman, W. and Kaufer, S. and
Kawabe, K. and Keerthana, N. V. and K{\'e}f{\'e}lian, F. and
Keitel, D. and Kennedy, R. and Key, J. S. and Khalili, F. Y. and
Khan, H. and Khan, I. and Khan, S. and Khan, Z. and Khazanov, E.
A. and Khursheed, M. and Kijbunchoo, N. and Kim, C. and Kim, J. C.
and Kim, K. and Kim, W. and Kim, W. S. and Kim, Y. -M. and
Kimball, C. and King, E. J. and King, P. J. and Kinley-Hanlon, M.
and Kirchhoff, R. and Kissel, J. S. and Kleybolte, L. and Klika,
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and Kowalska, I. and Kozak, D. B. and Kringel, V. and Krishnendu,
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affiliation = "{} and {} and {} and {} and {} and {} and {} and {} and {} and {}
and {} and {} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {} and {} and {} and {} and {} and {} and {} and {}
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Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {} and {} and {} and {} and {} and {} and {} and {}
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{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Search for the isotropic stochastic background using data from
Advanced LIGO's second observing run",
journal = "Physical Review D",
year = "2019",
volume = "100",
number = "6",
pages = "e061101",
abstract = "The stochastic gravitational-wave background is a superposition of
sources that are either too weak or too numerous to detect
individually. In this study, we present the results from a
cross-correlation analysis on data from Advanced LIGO's second
observing run (O2), which we combine with the results of the first
observing run (O1). We do not find evidence for a stochastic
background, so we place upper limits on the normalized energy
density in gravitational waves at the 95% credible level of
{\"{\I}}GW<6.0{\~A}10-8 for a frequency-independent (flat)
background and {\"{\I}}GW<4.8{\~A}10-8 at 25 Hz for a
background of compact binary coalescences. The upper limit
improves over the O1 result by a factor of 2.8. Additionally, we
place upper limits on the energy density in an isotropic
background of scalar- and vector-polarized gravitational waves,
and we discuss the implication of these results for models of
compact binaries and cosmic string backgrounds. Finally, we
present a conservative estimate of the correlated broadband noise
due to the magnetic Schumann resonances in O2, based on
magnetometer measurements at both the LIGO Hanford and LIGO
Livingston observatories. We find that correlated noise is well
below the O2 sensitivity. © 2019 American Physical Society.
American Physical Society.",
doi = "10.1103/PhysRevD.100.061101",
url = "http://dx.doi.org/10.1103/PhysRevD.100.061101",
issn = "1550-2368 and 1550-7998",
label = "isi 2019-10-21
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language = "en",
targetfile = "abbott_search.pdf",
url = "https://www.scopus.com/inward/record.uri?eid=2-s2.0-85072995802\&doi=10.1103%2fPhysRevD.100.061101\&partnerID=40\&md5=8ca9cb2e119894bfcabb5524104a8cbb",
urlaccessdate = "27 abr. 2024"
}