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Narrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 data

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Aasi, J.; Abbott, B.; Abbott, R.; Abbott, T.; Abernathy, M; Acernese, F.; Ackley, K.; Adams, C.; Adams, T.; Addesso, P.; Brady, P. R.; Piergiovanni, F.; Blair, C. D.; Hofman, D.; Katzman, W.; Summerscales, T. Z.; McWilliams, S.; Bonnand, R.; Steinlechner, S.; Pinto, I. M.; Moreno, G.; Oh, S. H.; Dominguez, E.; Iyer, B. R.; King, E. J.; MacInnis, M.; Poteomkin, A.; Bork, R.; Chalermsongsak, T.; Willke, B.; Clara, F.; Born, M.; Vallisneri, M.; Lorenzini, M.; Boschi, V.; Paris, H.; Wessels, P.; Raja, S.; Bhandare, R.; Sutton, P. J.; Colombini, M.; Bose, Sukanta; Ballmer, S. W.; Gergely, L. Á.; Krishnan, B.; Matichard, F.; Raymond, V.; Kokeyama, K.; De Rosa, R.; van Bakel, N; Lebigot, E.; Countryman, S.; Walsh, S.; Heitmann, H.; Hartman, M. T.; Bejger, M.; Veitch, P. J.; Ochsner, E.; Fafone, V.; Kasprzack, M.; Powell, J.; Patrick, Z.; Aggarwal, N.; Rowan, S.; Biwer, C.; Slagmolen, B.J.J.; Bradaschia, C.; Driggers, J. C.; Man, N.; Evans, T.; Pele, A.; Romie, J. H.; Díaz, M. C.; Canton, T. Dal; Leroy, N.; Couvares, P.; Ma, Y.; Fricke, T. T.; Razzano, M.; Mavalvala, N.; Coward, D. M.; Gleason, J.; DeRosa, R. T.; Bodiya, T. P.; Capano, C. D.; Koehlenbeck, S.; Izumi, K.; Zhang, Y.; Bulten, H.J.; Constancio, M.; Cowart, M. J.; Coyne, D. C.; Padilla, C.; Isler, J. C.; O’Shaughnessy, R.; Kaufer, S.; Singer, L.; Murray, P. G.; Bilenko, I. A.; Hopkins, P.; Radkins, H.; Wang, H.; Kim, C.; Lee, C. H.; Tiwari, V.; Mullavey, A.; Coyne, R.; Collette, C.; Rajalakshmi, G.; Oram, R.; Giazotto, A.; Królak, A.; Barone, F.; Cepeda, C; Agatsuma, K.; Craig, K.; Di Fiore, L.; Yamamoto, H.; Du, Z.; Creighton, J. D. E.; Mazzolo, G.; Ain, A.; Puppo, P.; Wimmer, M.; Ryan, K.; Smith, R. J. E.; Tomlinson, C.; Eggenstein, H.-B.; Creighton, T. D.; Littenberg, T. B.; Macleod, D. M.; Mohapatra, S. R. P.; Saleem, M.; Lundgren, A. P.; Gatto, A.; Viceré, A.; Marchesoni, F.; Fairhurst, S.; Westphal, T.; Kéfélian, F.; Prasad, J.; Wade, M.; Chiummo, A.; Grunewald, S.; Lebigot, E. O.; Re, V.; Bergman, J.; Effler, A.; Scott, J.; Blackburn, J. K.; Cripe, J.; Ashton, G.; Cesarini, E.; Groot, P.; Quiroga, G.; Schuette, D.; Genin, E.; Fidecaro, F.; Martelli, F.; Fan, X.; Heidmann, A.; Salemi, F.; Batch, J. C.; Anderson, W. G.; Hough, J.; Gehrels, N.; Yancey, C. C.; Del Pozzo, W.; Lück, H.; Krueger, C.; Daveloza, H.; Anderson, S. B.; Fang, Q.; Farinon, S.; Predoi, V.; Barbet, M.; Bell, C.; Lee, H. M.; Straniero, N.; Pai, A.; Kim, N.; Rüdiger, A.; Corsi, A.; Caride, S.; Márka, S.; van Beuzekom, M; Overmier, H.; Farr, B.; Brillet, A.; Sachdev, S.; Hosken, D. J.; Caudill, S.; McCarthy, R.; DeSalvo, R.; Downes, T. P.; Farr, W. M.; Gennai, A.; Zhao, C.; Brown, N. M.; Favata, M.; Fays, M.; Rocchi, A.; Yang, Q.; Sengupta, A. S.; Swinkels, B.; Van Den Brand, J.; Grant, A.; Brisson, V.; Massinger, T. J.; Meinders, M.; Clark, J. A.; McIver, J.; Heurs, M.; Wang, M.; Miller, J.; Guidi, G. M.; Winkler, W.; Carbognani, F.; Reed, C M; Welborn, T.; Jacobson, M.; Barsuglia, M.; Sammut, L.; Rollins, J. G.; Granata, M.; Coccia, E.; Verkindt, D.; Fehrmann, H.; Hughey, B.; Dhurandhar, S.; Romanov, G.; Singer, A.; Hoak, D.; Hanson, J.; Basti, A.; Guido, C. J.; Kawabe, K.; Sergeev, A.; Behnke, B.; Guo, X.; Hewitson, M.; Zhou, M.; Gair, J. R.; McIntyre, G.; Magaña-Sandoval, F.; Araya, M. C.; Gray, C.; Gushwa, K.; Buikema, A.; Regimbau, T.; Ramirez, K.; Cavalier, F.; Thorne, K. A.; Premachandra, S.; Lombardi, A. L.; Scott, S. M.; Evans, M.; Dent, T.; Ming, J.; Vincent-Finley, R.; Aston, S. M.; Dahl, K.; Sequino, V.; Kim, Y.-M.; Brau, J. E.; Morriss, S. R.; Gemme, G.; González, G.; Gustafson, E. K.; Hodge, K. A.; Danzmann, K.; Gustafson, R.; Hacker, J.; Schilling, R.; Zhu, X. J.; Sintes, A. M.; Tonelli, M.; Cook, D.; Babak, S.; Damjanic, M.; Mytidis, A.; Ducrot, M.; Mueller, G.; Key, J. S.; Bock, O.; Nguyen, T.; Jang, H.; Yvert, M.; Denker, T.; Sandberg, V.; Kuehn, G.; Millhouse, M.; Serna, G.; Schofield, R. M. S.; Indik, N.; Eberle, T.; Wallace, L.; Hall, E. D.; Klimenko, S.; Gendre, B.; Biscans, S.; Calloni, E.; Baldaccini, F.; Nolting, D.; Jaranowski, P.; Leong, J. R.; Smith-Lefebvre, N. D.; Pillant, G.; Baker, P. T.; Khalaidovski, A.; Hemming, G.; Chamberlin, S. J.; Melatos, A.; Haster, C.-J.; Inta, R.; Jawahar, S.; Dattilo, V.; Sanders, J. R.; Sadeghian, L.; Dergachev, V.; Rei, L.; Mazumder, N.; Singh, R.; Gretarsson, A. M.; Gammaitoni, L.; Nitz, A. H.; Wang, X.; Ji, Y.; Ferrini, F.; Smith, J. R.; Cunningham, L.; O’Reilly, B.; Aulbert, C.; Hu, Y. M.; Jiménez-Forteza, F.; Khazanov, E. A.; Fournier, J.-D.; Cadonati, L.; Johnson, W. W.; Sidery, T. L.; Stuver, A. L.; Van Den Broeck, C.; Eikenberry, S. S.; Kowalska, I.; Fiori, I.; Chen, Y.; Gossan, S.; Ottaway, D. J.; Libbrecht, K.; Wipf, C. C.; Kumar, A.; Zucker, M. E.; Arceneaux, C.; Sevigny, A.; Magee, R.; Nielsen, A. B.; Son, E. J.; Sigg, D.; Korth, W. Z.; Gouaty, R.; Jones, D. I.; Lubinski, M. J.; Hild, S.; Thomas, P.; Debreczeni, G.; Leaci, P.; Pekowsky, L.; Kumar, P.; Maros, E.; Szczepanczyk, M.; Kuo, L.; Libson, A.; Keitel, D.; Di Lieto, A.; Nagy, M. F.; 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Kanner, J. B.; Cumming, A.; Maksimovic, I.; Tellez, G.; Ward, R. L.; Dartez, L.; Meadors, G. D.; Kandhasamy, S.; Brown, D. D.; Daw, E. J.; Mohan, M.; Zuraw, S.; Mercer, R. A.; Kelley, D. B.; Tacca, M.; Nardecchia, I.; Chow, J. H.; Torrie, C. I.; Thirugnanasambandam, M. P.; Meacher, D.; Malvezzi, V.; Mueller, C. L.; Vetrano, F.; Heintze, M.; Milano, L.; Romano, R.; Meshkov, S.; Bavigadda, V.; van der Sluys, M. V.; Messenger, C.; Martin, R. M.; Prestegard, T.; Márka, Z.; Fulda, P.; Meyers, P. M.; Katsavounidis, E.; Edo, T.; Crowder, S. G.; Souradeep, T.; Pinard, L.; Barker, D.; Bersanetti, D.; Zanolin, M.; Fyffe, M.; Frasconi, F.; Ju, L.; Sadecki, T.; Masserot, A.; Fuentes-Tapia, S.; Mezzani, F.; Feldbaum, D.; Miao, H.; Urban, A. L.; Whelan, J. T.; Franco, S.; Munch, J.; Leavey, S.; D’Antonio, S.; Frey, R.; Ogin, G. H.; Agathos, M.; Lewis, J.; Travasso, F.; Palashov, O.; Doravari, S.; van Heijningen, J.; Vahlbruch, H.; Bauer, Th. S.; Michel, C.; Osthelder, C.; Kawazoe, F.; Newton, G.; Schreiber, E.; Nash, T.; Pedraza, M.; Vitale, S.; Naticchioni, L.; Mitselmakher, G.; Berry, C. P. L.; Mirshekari, S.; Nayak, R. K.; Barish, B. C.; Gräf, C.; Fejer, M. M.; Bitossi, M.; Bergmann, G.; Bartlett, J.; Schnabel, R.; Coulon, J.-P.; Hello, P.; Lazzarini, A.; Serafinelli, R.; Mohanty, S. D.; Heinzel, G.; Necula, V.; Hanke, M.; Baune, C.; Vedovato, G.; Woan, G.; Harry, I. W.; Mantovani, M.; Flaminio, R.; Hee, S.; Phelps, M.; Di Palma, I.; Martynov, D.; van Veggel, A. A.; Cho, M.; Goetz, R.; Vo, T.; Owen, B. J.; Nedkova, K.; Poeld, J.; Letendre, N.; Papa, M. A.; Simakov, D.; Palomba, C.; Quetschke, V.; Warner, J.; Pal-Singh, A.; Santiago-Prieto, I.; Nocera, F.; Pan, H.; Marion, F.; Huynh-Dinh, T.; Hammond, G.; Bizouard, M. A.; Bertolini, A.; Moe, B.; Siemens, X.; Keiser, G. M.; Mandel, I.; Smith, M. R.; Oh, J. J.; Calderón Bustillo, J.; Pankow, C.; Jonker, R. J. G.; Pannarale, F.; Wade, L.; Zendri, J.-P.; Miller, A.; Harms, J.; Kaur, T.; Rácz, I.; Areeda, J. S.; Mittleman, R.; Vocca, H.; Dooley, K. L.; Aylott, B. E.; Bloemen, S.; Pant, B. C.; Rapagnani, P.; Martellini, L.; Punturo, M.; Strain, K. A.; Price, L. R.; Roma, V.; White, D. J.; Benacquista, M.; Shahriar, M. S.; Prijatelj, M.; Minenkov, Y.; Kondrashov, V.; Jones, R.; Vass, S.; Sentenac, D.; O’Dell, J.; Colla, A.; Levin, Y.; Bassiri, R.; Pichot, M.; DeBra, D.; Principe, M.; Lasky, P. D.; Privitera, S.; Weiss, R.; Zweizig, J.; Chao, S.; Cagnoli, G.; Leonardi, M.; Hollitt, S. E.; Charlton, P.; Cornish, N.; Goetz, E.; Kinzel, D. L.; Whiting, B. F.; Prodi, G. A.; Chung, S.; Mitra, S.; Robinet, F.; Reid, S.; Bhagwat, S.; Worden, J.; Reitze, D. H.; Staley, A.; Reula, O.; Nissanke, S.; Lynch, R.; Larson, S.; Vorvick, C.; Penn, S.; Edwards, M.; Martin, I. W.; Nelemans, G.; Christensen, N.; Fritschel, P.; Ricci, F.; Cavaglià, M.; Riles, K.; Costa, C. A.; Briant, T.; Day, R.; Markosyan, A.; Kim, K.; Di Virgilio, A.; Etzel, T.; Houston, E.; Lormand, M.; Xie, S.; Chu, Q.; Normandin, M. E. N.; Scheuer, J.; Betzwieser, J.; Silva, A. D.; Coughlin, M. W.; Sassolas, B.; Talukder, D.; Sathyaprakash, B. S.; Passaquieti, R.; McLin, K.; Was, M.; Raab, F. J.; Graff, P. B.; Mitrofanov, V. P.; Belczynski, C.; Douglas, R.; Aufmuth, P.; Ciani, G.; Allen, B.; Saulson, P. R.; Cuoco, E.; Adhikari, R. X.; Chakraborty, R.; Lockett, V.; Ghosh, S.; Greenhalgh, R. J. S.; King, P. J.; McClelland, D. E.; Zhang, Fan; Bridges, D. O.; Shoemaker, D. H.; Shaltev, M.; Stone, R.; Brinkmann, M.; Shao, Z.; Traylor, G.; Shapiro, B.; Pürrer, M.; Mukherjee, S.; Wilkinson, C.; Idrisy, A.; Nuttall, L. K.; Prokhorov, L.; Gondan, L.; Ballardin, G.; Amariutei, D.; Garufi, F.; Shawhan, P.; Arai, K.; Danilishin, S. L.; Matone, L.; Holt, K.; Adya, V.; Loriette, V.; Mours, B.; Bojtos, P.; Cutler, C.; Steinmeyer, D.; Birch, J.; Thomas, M.; Stebbins, J.; Blackburn, L.; Steinke, M.; Rolland, L.; Ottens, R. S.; Yablon, J.; Korobko, M.; Bell, A. S.; Robertson, N. A.; Howell, E. J.; Gorodetsky, M. L.; Heptonstall, A. W.; Steinlechner, J.; Hanna, C.; Brooks, A. F.; Moore, B.; Kim, N. G.; Alemic, A.; Barton, M. A.; Ortega, W.; Ferreira, E. C.; Taylor, R.; Tanner, D. B.; Vajente, G.; Tápai, M.; Vousden, W. D.; Tarabrin, S. P.; Schmidt, P.; Post, A.; Zhang, L.; Quitzow-James, R.; Savage, R.; Kissel, J. S.; Husa, S.; Keppel, D. G.; Taracchini, A.; Haris, K.; Ajith, P.; Ohme, F.; Logue, J.; Mossavi, K.; Cho, H. S.; Hannam, M. D.; Unnikrishnan, C S; Tse, M.; Venkateswara, K.; Tshilumba, D.; Weaver, B.; Cominsky, L.; Siellez, K.; Bond, C.; Chua, S.; Cleva, F.; Losurdo, G.; Kline, J.; Li, T. G. F.; Ugolini, D.; Lazzaro, C.; Fisher, R. P.; Pierro, V.; Chassande-Mottin, E.; Donovan, F.; Kalogera, V.; Vecchio, A.; Vasúth, M.; Walker, M.; Vaulin, R.; Williams, L.; Ehrens, P.; Steplewski, S.; Drago, M.; Dwyer, S.; Cella, G.; Affeldt, C.; Marx, J. N.; Conte, A.; Mandic, V.; Hardwick, T.; Raffai, P.; Allocca, A.; Le, J.; Blair, D.; Vyatchanin, S. P.; Wen, L.; Wade, A. R.; Aguiar, O. D.; Gras, S.; Theeg, T.; Gordon, N.; Goßler, S.; Dereli, H.; Moggi, A.; Eichholz, J.; Middleton, H.; Kang, G.; Ruggi, P.; Giaime, J. A.; Mangano, V.; Weinstein, A. J.; Wei, L.-W.; Weinert, M.; Factourovich, M.; Ingram, D. R.; Usman, S. A.; Huerta, E.; Huttner, S. H.; Gaonkar, S.; Oelker, E.; Ast, S.; Neri, I.; Sellers, D.; Buskulic, D.; Mikhailov, E. E.; Willis, J. L.; Williams, R.; Williamson, A. R.; Grote, H.; Kozak, D. B.; Veitch, J.; Barayoga, J. C.; Buonanno, A.; Perreca, A.; Islas, G.; Paoletti, F.; Billingsley, G.; Davies, G. S.; Neri, M.; Boer, M.; Yakushin, I.; Yam, W.; MacDonald, T.; Corbitt, T. R.; Lough, J.; Davier, M.; Rabeling, D. S.; Kringel, V.; Puncken, O.; Sturani, R.; Freise, A.; Chincarini, A.; Zhang, M.; Bogaert, G.; Meidam, J.; Essick, R.; McCormick, S.; Frei, Z.; Rosińska, D.; Machenschalk, B.; Robie, R.; Thrane, E.; Dolique, V.; Bondu, F.; Bonelli, L.; Murphy, D.; Greco, G.; Mow-Lowry, C. M.; Haughian, K.; Schutz, B. F.; Bartos, I.; Sawadsky, A.; Giardina, K. D.

Description

In this paper we present the results of a coherent narrow-band search for continuous gravitational-wave signals from the Crab and Vela pulsars conducted on Virgo VSR4 data. In order to take into account a possible small mismatch between the gravitational-wave frequency and two times the star rotation frequency, inferred from measurement of the electromagnetic pulse rate, a range of 0.02 Hz around two times the star rotational frequency has been searched for both the pulsars. No evidence for a...[Show more]

dc.contributor.authorAasi, J.
dc.contributor.authorAbbott, B.
dc.contributor.authorAbbott, R.
dc.contributor.authorAbbott, T.
dc.contributor.authorAbernathy, M
dc.contributor.authorAcernese, F.
dc.contributor.authorAckley, K.
dc.contributor.authorAdams, C.
dc.contributor.authorAdams, T.
dc.contributor.authorAddesso, P.
dc.contributor.authorBrady, P. R.
dc.contributor.authorPiergiovanni, F.
dc.contributor.authorBlair, C. D.
dc.contributor.authorHofman, D.
dc.contributor.authorKatzman, W.
dc.contributor.authorSummerscales, T. Z.
dc.contributor.authorMcWilliams, S.
dc.contributor.authorBonnand, R.
dc.contributor.authorSteinlechner, S.
dc.contributor.authorPinto, I. M.
dc.contributor.authorMoreno, G.
dc.contributor.authorOh, S. H.
dc.contributor.authorDominguez, E.
dc.contributor.authorIyer, B. R.
dc.contributor.authorKing, E. J.
dc.contributor.authorMacInnis, M.
dc.contributor.authorPoteomkin, A.
dc.contributor.authorBork, R.
dc.contributor.authorChalermsongsak, T.
dc.contributor.authorWillke, B.
dc.contributor.authorClara, F.
dc.contributor.authorBorn, M.
dc.contributor.authorVallisneri, M.
dc.contributor.authorLorenzini, M.
dc.contributor.authorBoschi, V.
dc.contributor.authorParis, H.
dc.contributor.authorWessels, P.
dc.contributor.authorRaja, S.
dc.contributor.authorBhandare, R.
dc.contributor.authorSutton, P. J.
dc.contributor.authorColombini, M.
dc.contributor.authorBose, Sukanta
dc.contributor.authorBallmer, S. W.
dc.contributor.authorGergely, L. Á.
dc.contributor.authorKrishnan, B.
dc.contributor.authorMatichard, F.
dc.contributor.authorRaymond, V.
dc.contributor.authorKokeyama, K.
dc.contributor.authorDe Rosa, R.
dc.contributor.authorvan Bakel, N
dc.contributor.authorLebigot, E.
dc.contributor.authorCountryman, S.
dc.contributor.authorWalsh, S.
dc.contributor.authorHeitmann, H.
dc.contributor.authorHartman, M. T.
dc.contributor.authorBejger, M.
dc.contributor.authorVeitch, P. J.
dc.contributor.authorOchsner, E.
dc.contributor.authorFafone, V.
dc.contributor.authorKasprzack, M.
dc.contributor.authorPowell, J.
dc.contributor.authorPatrick, Z.
dc.contributor.authorAggarwal, N.
dc.contributor.authorRowan, S.
dc.contributor.authorBiwer, C.
dc.contributor.authorSlagmolen, B.J.J.
dc.contributor.authorBradaschia, C.
dc.contributor.authorDriggers, J. C.
dc.contributor.authorMan, N.
dc.contributor.authorEvans, T.
dc.contributor.authorPele, A.
dc.contributor.authorRomie, J. H.
dc.contributor.authorDíaz, M. C.
dc.contributor.authorCanton, T. Dal
dc.contributor.authorLeroy, N.
dc.contributor.authorCouvares, P.
dc.contributor.authorMa, Y.
dc.contributor.authorFricke, T. T.
dc.contributor.authorRazzano, M.
dc.contributor.authorMavalvala, N.
dc.contributor.authorCoward, D. M.
dc.contributor.authorGleason, J.
dc.contributor.authorDeRosa, R. T.
dc.contributor.authorBodiya, T. P.
dc.contributor.authorCapano, C. D.
dc.contributor.authorKoehlenbeck, S.
dc.contributor.authorIzumi, K.
dc.contributor.authorZhang, Y.
dc.contributor.authorBulten, H.J.
dc.contributor.authorConstancio, M.
dc.contributor.authorCowart, M. J.
dc.contributor.authorCoyne, D. C.
dc.contributor.authorPadilla, C.
dc.contributor.authorIsler, J. C.
dc.contributor.authorO’Shaughnessy, R.
dc.contributor.authorKaufer, S.
dc.contributor.authorSinger, L.
dc.contributor.authorMurray, P. G.
dc.contributor.authorBilenko, I. A.
dc.contributor.authorHopkins, P.
dc.contributor.authorRadkins, H.
dc.contributor.authorWang, H.
dc.contributor.authorKim, C.
dc.contributor.authorLee, C. H.
dc.contributor.authorTiwari, V.
dc.contributor.authorMullavey, A.
dc.contributor.authorCoyne, R.
dc.contributor.authorCollette, C.
dc.contributor.authorRajalakshmi, G.
dc.contributor.authorOram, R.
dc.contributor.authorGiazotto, A.
dc.contributor.authorKrólak, A.
dc.contributor.authorBarone, F.
dc.contributor.authorCepeda, C
dc.contributor.authorAgatsuma, K.
dc.contributor.authorCraig, K.
dc.contributor.authorDi Fiore, L.
dc.contributor.authorYamamoto, H.
dc.contributor.authorDu, Z.
dc.contributor.authorCreighton, J. D. E.
dc.contributor.authorMazzolo, G.
dc.contributor.authorAin, A.
dc.contributor.authorPuppo, P.
dc.contributor.authorWimmer, M.
dc.contributor.authorRyan, K.
dc.contributor.authorSmith, R. J. E.
dc.contributor.authorTomlinson, C.
dc.contributor.authorEggenstein, H.-B.
dc.contributor.authorCreighton, T. D.
dc.contributor.authorLittenberg, T. B.
dc.contributor.authorMacleod, D. M.
dc.contributor.authorMohapatra, S. R. P.
dc.contributor.authorSaleem, M.
dc.contributor.authorLundgren, A. P.
dc.contributor.authorGatto, A.
dc.contributor.authorViceré, A.
dc.contributor.authorMarchesoni, F.
dc.contributor.authorFairhurst, S.
dc.contributor.authorWestphal, T.
dc.contributor.authorKéfélian, F.
dc.contributor.authorPrasad, J.
dc.contributor.authorWade, M.
dc.contributor.authorChiummo, A.
dc.contributor.authorGrunewald, S.
dc.contributor.authorLebigot, E. O.
dc.contributor.authorRe, V.
dc.contributor.authorBergman, J.
dc.contributor.authorEffler, A.
dc.contributor.authorScott, J.
dc.contributor.authorBlackburn, J. K.
dc.contributor.authorCripe, J.
dc.contributor.authorAshton, G.
dc.contributor.authorCesarini, E.
dc.contributor.authorGroot, P.
dc.contributor.authorQuiroga, G.
dc.contributor.authorSchuette, D.
dc.contributor.authorGenin, E.
dc.contributor.authorFidecaro, F.
dc.contributor.authorMartelli, F.
dc.contributor.authorFan, X.
dc.contributor.authorHeidmann, A.
dc.contributor.authorSalemi, F.
dc.contributor.authorBatch, J. C.
dc.contributor.authorAnderson, W. G.
dc.contributor.authorHough, J.
dc.contributor.authorGehrels, N.
dc.contributor.authorYancey, C. C.
dc.contributor.authorDel Pozzo, W.
dc.contributor.authorLück, H.
dc.contributor.authorKrueger, C.
dc.contributor.authorDaveloza, H.
dc.contributor.authorAnderson, S. B.
dc.contributor.authorFang, Q.
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dc.contributor.authorBarbet, M.
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dc.contributor.authorChincarini, A.
dc.contributor.authorZhang, M.
dc.contributor.authorBogaert, G.
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dc.date.accessioned2015-06-16T02:54:04Z
dc.date.available2015-06-16T02:54:04Z
dc.identifier.issn1550-7998
dc.identifier.urihttp://hdl.handle.net/1885/13951
dc.description.abstractIn this paper we present the results of a coherent narrow-band search for continuous gravitational-wave signals from the Crab and Vela pulsars conducted on Virgo VSR4 data. In order to take into account a possible small mismatch between the gravitational-wave frequency and two times the star rotation frequency, inferred from measurement of the electromagnetic pulse rate, a range of 0.02 Hz around two times the star rotational frequency has been searched for both the pulsars. No evidence for a signal has been found and 95% confidence level upper limits have been computed assuming both that polarization parameters are completely unknown and that they are known with some uncertainty, as derived from x-ray observations of the pulsar wind torii. For Vela the upper limits are comparable to the spin-down limit, computed assuming that all the observed spin-down is due to the emission of gravitational waves. For Crab the upper limits are about a factor of 2 below the spin-down limit, and represent a significant improvement with respect to past analysis. This is the first time the spin-down limit is significantly overcome in a narrow-band search.
dc.description.sponsorshipThe authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Economía y Competitividad, the Conselleria d’Economia Hisenda i Innovació of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, OTKA of Hungary, the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Sciences and Engineering Research Council of Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.
dc.publisherAmerican Physical Society
dc.rights© 2015 American Physical Society. http://www.sherpa.ac.uk/romeo/issn/1550-7998/ Author can archive publisher's version/PDF (Sherpa/Romeo 4/9/2017)
dc.sourcePhysical Review D: Particles, Fields, Gravitation and Cosmology
dc.subjectgravitational-wave frequency
dc.subjectCrab
dc.subjectVela
dc.subjectpulsar
dc.subjectnarrow-band
dc.subjectelectromagnetic pulse rate
dc.titleNarrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 data
dc.typeJournal article
local.identifier.citationvolume91
dc.date.issued2015
local.identifier.absfor010504 - Mathematical Aspects of General Relativity
local.identifier.absfor020502 - Lasers and Quantum Electronics
local.identifier.absfor029902 - Complex Physical Systems
local.identifier.ariespublicationa383154xPUB905
local.publisher.urlhttp://www.aps.org/
local.type.statusPublished Version
local.contributor.affiliationChow Jong H., Department of Quantum Science, CPMS Research School of Physics and Engineering, The Australian National University
local.contributor.affiliationMansell, G. L., Department of Quantum Science, CPMS Research School of Physics and Engineering, The Australian National University
local.contributor.affiliationWade, A. R., Department of Quantum Science, CPMS Research School of Physics and Engineering, The Australian National University
local.contributor.affiliationWard, R. L., Department of Quantum Science, CPMS Research School of Physics and Engineering, The Australian National University
local.identifier.essn1550-2368
local.bibliographicCitation.issue2
local.identifier.doi10.1103/PhysRevD.91.022004
dc.date.updated2016-06-14T08:34:41Z
local.identifier.scopusID2-s2.0-84921530995
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