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All-sky search for periodic gravitational waves in the full S5 LIGO data

Abadie, J. ; Abbott, B. P. ; Abbott, R. ; Abbott, T. D. ; Abernathy, M. ; Accadia, T. ; Acernese, F. ; Adams, C. ; Adhikari, R. and Affeldt, C. , et al. (2012) In Physical Review D (Particles, Fields, Gravitation and Cosmology) 85(2).
Abstract
We report on an all-sky search for periodic gravitational waves in the frequency band 50-800 Hz and with the frequency time derivative in the range of 0 through -6 x 10(-9) Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. After recent improvements in the search program that yielded a 10x increase in computational efficiency, we have searched in two years of data collected during LIGO's fifth science run and have obtained the most sensitive all-sky upper limits on gravitational-wave strain to date. Near 150 Hz our upper limit on worst-case linearly polarized strain amplitude h(0) is 1 x 10(-24), while at the high end of our frequency range we achieve a worst-case... (More)
We report on an all-sky search for periodic gravitational waves in the frequency band 50-800 Hz and with the frequency time derivative in the range of 0 through -6 x 10(-9) Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. After recent improvements in the search program that yielded a 10x increase in computational efficiency, we have searched in two years of data collected during LIGO's fifth science run and have obtained the most sensitive all-sky upper limits on gravitational-wave strain to date. Near 150 Hz our upper limit on worst-case linearly polarized strain amplitude h(0) is 1 x 10(-24), while at the high end of our frequency range we achieve a worst-case upper limit of 3.8 x 10(-24) for all polarizations and sky locations. These results constitute a factor of 2 improvement upon previously published data. A new detection pipeline utilizing a loosely coherent algorithm was able to follow up weaker outliers, increasing the volume of space where signals can be detected by a factor of 10, but has not revealed any gravitational-wave signals. The pipeline has been tested for robustness with respect to deviations from the model of an isolated neutron star, such as caused by a low-mass or long-period binary companion. (Less)
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organization
publishing date
type
Contribution to journal
publication status
published
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in
Physical Review D (Particles, Fields, Gravitation and Cosmology)
volume
85
issue
2
publisher
American Physical Society
external identifiers
  • wos:000298989700001
  • scopus:84863011766
ISSN
1550-2368
DOI
10.1103/PhysRevD.85.022001
language
English
LU publication?
yes
id
312fabfa-ae74-4621-a5f1-74cc0957de4b (old id 2361616)
date added to LUP
2016-04-01 11:06:37
date last changed
2023-01-02 18:44:44
@article{312fabfa-ae74-4621-a5f1-74cc0957de4b,
  abstract     = {{We report on an all-sky search for periodic gravitational waves in the frequency band 50-800 Hz and with the frequency time derivative in the range of 0 through -6 x 10(-9) Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. After recent improvements in the search program that yielded a 10x increase in computational efficiency, we have searched in two years of data collected during LIGO's fifth science run and have obtained the most sensitive all-sky upper limits on gravitational-wave strain to date. Near 150 Hz our upper limit on worst-case linearly polarized strain amplitude h(0) is 1 x 10(-24), while at the high end of our frequency range we achieve a worst-case upper limit of 3.8 x 10(-24) for all polarizations and sky locations. These results constitute a factor of 2 improvement upon previously published data. A new detection pipeline utilizing a loosely coherent algorithm was able to follow up weaker outliers, increasing the volume of space where signals can be detected by a factor of 10, but has not revealed any gravitational-wave signals. The pipeline has been tested for robustness with respect to deviations from the model of an isolated neutron star, such as caused by a low-mass or long-period binary companion.}},
  author       = {{Abadie, J. and Abbott, B. P. and Abbott, R. and Abbott, T. D. and Abernathy, M. and Accadia, T. and Acernese, F. and Adams, C. and Adhikari, R. and Affeldt, C. and Ajith, P. and Allen, B. and Allen, G. S. and Ceron, E. Amador and Amariutei, D. and Amin, R. S. and Anderson, S. B. and Anderson, W. G. and Arai, K. and Arain, M. A. and Araya, M. C. and Aston, S. M. and Astone, P. and Atkinson, D. and Aufmuth, P. and Aulbert, C. and Aylott, B. E. and Babak, S. and Baker, P. and Ballardin, G. and Ballmer, S. and Barker, D. and Barone, F. and Barr, B. and Barriga, P. and Barsotti, L. and Barsuglia, M. and Barton, M. A. and Bartos, I. and Bassiri, R. and Bastarrika, M. and Basti, A. and Batch, J. and Bauchrowitz, J. and Bauer, Th S. and Bebronne, M. and Behnke, B. and Beker, M. G. and Bell, A. S. and Belletoile, A. and Belopolski, I. and Benacquista, M. and Berliner, J. M. and Bertolini, A. and Betzwieser, J. and Beveridge, N. and Beyersdorf, P. T. and Bilenko, I. A. and Billingsley, G. and Birch, J. and Biswas, R. and Bitossi, M. and Bizouard, M. A. and Black, E. and Blackburn, J. K. and Blackburn, L. and Blair, D. and Bland, B. and Blom, M. and Bock, O. and Bodiya, T. P. and Bogan, C. and Bondarescu, R. and Bondu, F. and Bonelli, L. and Bonnand, R. and Bork, R. and Born, M. and Boschi, V. and Bose, S. and Bosi, L. and Bouhou, B. and Braccini, S. and Bradaschia, C. and Brady, P. R. and Braginsky, V. B. and Branchesi, M. and Brau, J. E. and Breyer, J. and Briant, T. and Bridges, D. O. and Brillet, A. and Brinkmann, M. and Brisson, V. and Britzger, M. and Brooks, A. F. and Brown, D. A. and Brummit, A. and Bulik, T. and Bulten, H. J. and Buonanno, A. and Burguet-Castell, J. and Burmeister, O. and Buskulic, D. and Buy, C. and Byer, R. L. and Cadonati, L. and Cagnoli, G. and Calloni, E. and Camp, J. B. and Campsie, P. and Cannizzo, J. and Cannon, K. and Canuel, B. and Cao, J. and Capano, C. D. and Carbognani, F. and Caride, S. and Caudill, S. and Cavaglia, M. and Cavalier, F. and Cavalieri, R. and Cella, G. and Cepeda, C. and Cesarini, E. and Chaibi, O. and Chalermsongsak, T. and Chalkley, E. and Charlton, P. and Chassande-Mottin, E. and Chelkowski, S. and Chen, Y. and Chincarini, A. and Chiummo, A. and Cho, H. and Christensen, N. and Chua, S. S. Y. and Chung, C. T. Y. and Chung, S. and Ciani, G. and Clara, F. and Clark, D. E. and Clark, J. and Clayton, J. H. and Cleva, F. and Coccia, E. and Cohadon, P. -F. and Colacino, C. N. and Colas, J. and Colla, A. and Colombini, M. and Conte, A. and Conte, R. and Cook, D. and Corbitt, T. R. and Cordier, M. and Cornish, N. and Corsi, A. and Costa, C. A. and Coughlin, M. and Coulon, J. -P. and Couvares, P. and Coward, D. M. and Coyne, D. C. and Creighton, J. D. E. and Creighton, T. D. and Cruise, A. M. and Cumming, A. and Cunningham, L. and Cuoco, E. and Cutler, R. M. and Dahl, K. and Danilishin, S. L. and Dannenberg, R. and D'Antonio, S. and Danzmann, K. and Dattilo, V. and Daudert, B. and Daveloza, H. and Davier, M. and Davies, G. and Daw, E. J. and Day, R. and Dayanga, T. and De Rosa, R. and Debra, D. and Debreczeni, G. and Degallaix, J. and Del Pozzo, W. and del Prete, M. and Dent, T. and Dergachev, V. and DeRosa, R. and DeSalvo, R. and Dhurandhar, S. and Di Fiore, L. and DiGuglielmo, J. and Di Lieto, A. and Di Palma, I. and Di Paolo Emilio, M. and Di Virgilio, A. and Diaz, M. and Dietz, A. and Donovan, F. and Dooley, K. L. and Dorsher, S. and Drago, M. and Drever, R. W. P. and Driggers, J. C. and Du, Z. and Dumas, J. -C. and Dwyer, S. and Eberle, T. and Edgar, M. and Edwards, M. and Effler, A. and Ehrens, P. and Endroczi, G. and Engel, R. and Etzel, T. and Evans, K. and Evans, M. and Evans, T. and Factourovich, M. and Fafone, V. and Fairhurst, S. and Fan, Y. and Farr, B. F. and Farr, W. and Fazi, D. and Fehrmann, H. and Feldbaum, D. and Ferrante, I. and Fidecaro, F. and Finn, L. S. and Fiori, I. and Fisher, R. P. and Flaminio, R. and Flanigan, M. and Foley, S. and Forsi, E. and Forte, L. A. and Fotopoulos, N. and Fournier, J. -D. and Franc, J. and Frasca, S. and Frasconi, F. and Frede, M. and Frei, M. and Frei, Z. and Freise, A. and Frey, R. and Fricke, T. T. and Friedrich, D. and Fritschel, P. and Frolov, V. V. and Fulda, P. J. and Fyffe, M. and Galimberti, M. and Gammaitoni, L. and Ganija, M. R. and Garcia, J. and Garofoli, J. A. and Garufi, F. and Gaspar, M. E. and Gemme, G. and Geng, R. and Genin, E. and Gennai, A. and Gergely, L. A. and Ghosh, S. and Giaime, J. A. and Giampanis, S. and Giardina, K. D. and Giazotto, A. and Gill, C. and Goetz, E. and Goggin, L. M. and Gonzalez, G. and Gorodetsky, M. L. and Gossler, S. and Gouaty, R. and Graef, C. and Granata, M. and Grant, A. and Gras, S. and Gray, C. and Gray, N. and Greenhalgh, R. J. S. and Gretarsson, A. M. and Greverie, C. and Grosso, R. and Grote, H. and Grunewald, S. and Guidi, G. M. and Guido, C. and Gupta, R. and Gustafson, E. K. and Gustafson, R. and Ha, T. and Hage, B. and Hallam, J. M. and Hammer, D. and Hammond, G. and Hanks, J. and Hanna, C. and Hanson, J. and Harms, J. and Harry, G. M. and Harry, I. W. and Harstad, E. D. and Hartman, M. T. and Haughian, K. and Hayama, K. and Hayau, J. -F. and Hayler, T. and Heefner, J. and Heidmann, A. and Heintze, M. C. and Heitmann, H. and Hello, P. and Hendry, M. A. and Heng, I. S. and Heptonstall, A. W. and Herrera, V. and Hewitson, M. and Hild, S. and Hoak, D. and Hodge, K. A. and Holt, K. and Hong, T. and Hooper, S. and Hosken, D. J. and Hough, J. and Howell, E. J. and Hughey, B. and Husa, S. and Huttner, S. H. and Huynh-Dinh, T. and Ingram, D. R. and Inta, R. and Isogai, T. and Ivanov, A. and Izumi, K. and Jacobson, M. and Jang, H. and Jaranowski, P. and Johnson, W. W. and Jones, D. I. and Jones, G. and Jones, R. and Ju, L. and Kalmus, P. and Kalogera, V. and Kamaretsos, I. and Kandhasamy, S. and Kang, G. and Kanner, J. B. and Katsavounidis, E. and Katzman, W. and Kaufer, H. and Kawabe, K. and Kawamura, S. and Kawazoe, F. and Kells, W. and Keppel, D. G. and Keresztes, Z. and Khalaidovski, A. and Khalili, F. Y. and Khazanov, E. A. and Kim, B. and Kim, Chunglee and Kim, D. and Kim, H. and Kim, K. and Kim, N. and Kim, Y. -M. and King, P. J. and Kinsey, M. and Kinzel, D. L. and Kissel, J. S. and Klimenko, S. and Kokeyama, K. and Kondrashov, V. and Kopparapu, R. and Koranda, S. and Korth, W. Z. and Kowalska, I. and Kozak, D. and Kringel, V. and Krishnamurthy, S. and Krishnan, B. and Krolak, A. and Kuehn, G. and Kumar, R. and Kwee, P. and Lam, P. K. and Landry, M. and Lang, M. and Lantz, B. and Lastzka, N. and Lawrie, C. and Lazzarini, A. and Leaci, P. and Lee, C. H. and Lee, H. M. and Leindecker, N. and Leong, J. R. and Leonor, I. and Leroy, N. and Letendre, N. and Li, J. and Li, T. G. F. and Liguori, N. and Lindquist, P. E. and Lockerbie, N. A. and Lodhia, D. and Lorenzini, M. and Loriette, V. and Lormand, M. and Losurdo, G. and Luan, J. and Lubinski, M. and Lueck, H. and Lundgren, A. P. and Macdonald, E. and Machenschalk, B. and MacInnis, M. and Macleod, D. M. and Mageswaran, M. and Mailand, K. and Majorana, E. and Maksimovic, I. and Man, N. and Mandel, I. and Mandic, V. and Mantovani, M. and Marandi, A. and Marchesoni, F. and Marion, F. and Marka, S. and Marka, Z. and Markosyan, A. and Maros, E. and Marque, J. and Martelli, F. and Martin, I. W. and Martin, R. M. and Marx, J. N. and Mason, K. and Masserot, A. and Matichard, F. and Matone, L. and Matzner, R. A. and Mavalvala, N. and Mazzolo, G. and McCarthy, R. and McClelland, D. E. and McGuire, S. C. and McIntyre, G. and McIver, J. and McKechan, D. J. A. and Meadors, G. D. and Mehmet, M. and Meier, T. and Melatos, A. and Melissinos, A. C. and Mendell, G. and Menendez, D. and Mercer, R. A. and Meshkov, S. and Messenger, C. and Meyer, M. S. and Miao, H. and Michel, C. and Milano, L. and Miller, J. and Minenkov, Y. and Mitrofanov, V. P. and Mitselmakher, G. and Mittleman, R. and Miyakawa, O. and Moe, B. and Moesta, P. and Mohan, M. and Mohanty, S. D. and Mohapatra, S. R. P. and Moraru, D. and Moreno, G. and Morgado, N. and Morgia, A. and Mori, T. and Mosca, S. and Mossavi, K. and Mours, B. and Mow-Lowry, C. M. and Mueller, C. L. and Mueller, G. and Mukherjee, S. and Mullavey, A. and Mueller-Ebhardt, H. and Munch, J. and Murphy, D. and Murray, P. G. and Mytidis, A. and Nash, T. and Naticchioni, L. and Nawrodt, R. and Necula, V. and Nelson, J. and Newton, G. and Nishizawa, A. and Nocera, F. and Nolting, D. and Nuttall, L. and Ochsner, E. and O'Dell, J. and Oelker, E. and Ogin, G. H. and Oh, J. J. and Oh, S. H. and Oldenburg, R. G. and O'Reilly, B. and O'Shaughnessy, R. and Osthelder, C. and Ott, C. D. and Ottaway, D. J. and Ottens, R. S. and Overmier, H. and Owen, B. J. and Page, A. and Pagliaroli, G. and Palladino, L. and Palomba, C. and Pan, Y. and Pankow, C. and Paoletti, F. and Papa, M. A. and Parisi, M. and Pasqualetti, A. and Passaquieti, R. and Passuello, D. and Patel, P. and Pedraza, M. and Peiris, P. and Pekowsky, L. and Penn, S. and Peralta, C. and Perreca, A. and Persichetti, G. and Phelps, M. and Pickenpack, M. and Piergiovanni, F. and Pietka, M. and Pinard, L. and Pinto, I. M. and Pitkin, M. and Pletsch, H. J. and Plissi, M. V. and Poggiani, R. and Poeld, J. and Postiglione, F. and Prato, M. and Predoi, V. and Price, L. R. and Prijatelj, M. and Principe, M. and Privitera, S. and Prix, R. and Prodi, G. A. and Prokhorov, L. and Puncken, O. and Punturo, M. and Puppo, P. and Quetschke, V. and Raab, F. J. and Rabeling, D. S. and Racz, I. and Radkins, H. and Raffai, P. and Rakhmanov, M. and Ramet, C. R. and Rankins, B. and Rapagnani, P. and Raymond, V. and Re, V. and Redwine, K. and Reed, C. M. and Reed, T. and Regimbau, T. and Reid, S. and Reitze, D. H. and Ricci, F. and Riesen, R. and Riles, K. and Robertson, N. A. and Robinet, F. and Robinson, C. and Robinson, E. L. and Rocchi, A. and Roddy, S. and Rodriguez, C. and Rodruck, M. and Rolland, L. and Rollins, J. and Romano, J. D. and Romano, R. and Romie, J. H. and Rosinska, D. and Roever, C. and Rowan, S. and Ruediger, A. and Ruggi, P. and Ryan, K. and Ryll, H. and Sainathan, P. and Sakosky, M. and Salemi, F. and Samblowski, A. and Sammut, L. and Sancho de la Jordana, L. and Sandberg, V. and Sankar, S. and Sannibale, V. and Santamaria, L. and Santiago-Prieto, I. and Santostasi, G. and Sassolas, B. and Sathyaprakash, B. S. and Sato, S. and Saulson, P. R. and Savage, R. L. and Schilling, R. and Schlamminger, S. and Schnabel, R. and Schofield, R. M. S. and Schulz, B. and Schutz, B. F. and Schwinberg, P. and Scott, J. and Scott, S. M. and Searle, A. C. and Seifert, F. and Sellers, D. and Sengupta, A. S. and Sentenac, D. and Sergeev, A. and Shaddock, D. A. and Shaltev, M. and Shapiro, B. and Shawhan, P. and Shoemaker, D. H. and Sibley, A. and Siemens, X. and Sigg, D. and Singer, A. and Singer, L. and Sintes, A. M. and Skelton, G. and Slagmolen, B. J. J. and Slutsky, J. and Smith, J. R. and Smith, M. R. and Smith, N. D. and Smith, R. J. E. and Somiya, K. and Sorazu, B. and Soto, J. and Speirits, F. C. and Sperandio, L. and Stefszky, M. and Stein, A. J. and Steinert, E. and Steinlechner, J. and Steinlechner, S. and Steplewski, S. and Stochino, A. and Stone, R. and Strain, K. A. and Strigin, S. and Stroeer, A. S. and Sturani, R. and Stuver, A. L. and Summerscales, T. Z. and Sung, M. and Susmithan, S. and Sutton, P. J. and Swinkels, B. and Tacca, M. and Taffarello, L. and Talukder, D. and Tanner, D. B. and Tarabrin, S. P. and Taylor, J. R. and Taylor, R. and Thomas, P. and Thorne, K. A. and Thorne, K. S. and Thrane, E. and Thuering, A. and Titsler, C. and Tokmakov, K. V. and Toncelli, A. and Tonelli, M. and Torre, O. and Torres, C. and Torrie, C. I. and Tournefier, E. and Travasso, F. and Traylor, G. and Trias, M. and Tseng, K. and Ugolini, D. and Urbanek, K. and Vahlbruch, H. and Vajente, G. and Vallisneri, M. and van den Brand, J. F. J. and Van Den Broeck, C. and van der Putten, S. and van Veggel, A. A. and Vass, S. and Vasuth, M. and Vaulin, R. and Vavoulidis, M. and Vecchio, A. and Vedovato, G. and Veitch, J. and Veitch, P. J. and Veltkamp, C. and Verkindt, D. and Vetrano, F. and Vicere, A. and Villar, A. E. and Vinet, J. -Y. and Vitale, S. and Vitale, S. and Vocca, H. and Vorvick, C. and Vyatchanin, S. P. and Wade, A. and Waldman, S. J. and Wallace, L. and Wan, Y. and Wang, X. and Wang, Z. and Wanner, A. and Ward, R. L. and Was, M. and Wei, P. and Weinert, M. and Weinstein, A. J. and Weiss, R. and Wen, L. and Wen, S. and Wessels, P. and West, M. and Westphal, T. and Wette, K. and Whelan, J. T. and Whitcomb, S. E. and White, D. and Whiting, B. F. and Wilkinson, C. and Willems, P. A. and Williams, H. R. and Williams, L. and Willke, B. and Winkelmann, L. and Winkler, W. and Wipf, C. C. and Wiseman, A. G. and Wittel, H. and Woan, G. and Wooley, R. and Worden, J. and Yablon, J. and Yakushin, I. and Yamamoto, H. and Yamamoto, K. and Yang, H. and Yeaton-Massey, D. and Yoshida, S. and Yu, P. and Yvert, M. and Zadrozny, A. and Zanolin, M. and Zendri, J. -P. and Zhang, F. and Zhang, L. and Zhang, W. and Zhang, Z. and Zhao, C. and Zotov, N. and Zucker, M. E. and Zweizig, J.}},
  issn         = {{1550-2368}},
  language     = {{eng}},
  number       = {{2}},
  publisher    = {{American Physical Society}},
  series       = {{Physical Review D (Particles, Fields, Gravitation and Cosmology)}},
  title        = {{All-sky search for periodic gravitational waves in the full S5 LIGO data}},
  url          = {{https://lup.lub.lu.se/search/files/2386333/2970361.pdf}},
  doi          = {{10.1103/PhysRevD.85.022001}},
  volume       = {{85}},
  year         = {{2012}},
}