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Open Access#22010
Searches For Gravitational Waves From Known Pulsars With Science Run 5 LIGO Data
Abbott, B. P; Abbott, R; Acernese, F; Adhikari, R; Ajith, P; Allen, B; Allen, G; Alshourbagy, M; Amin, R. S; Anderson, S. B; Anderson, W. G; Antonucci, F; Aoudia, S; Arain, M. A; Araya, M; Armandula, H; Armor, P; Arun, K. G; Aso, Y; Aston, S; Astonea, P; Aufmuth, P; Aulbert, C; Babak, S; Baker, P; Ballardin, G; Ballmer, S; Barker, C; Barker, D; Barone, F; Barr, B; Barriga, P; Barsotti, L; Barsuglia, M; Barton, M. A; Bartos, I; Bassiri, R; Bastarrika, M; Bauer, T. S; Behnke, B; Beker, M; Benacquista, M; Betzwieser, J; Beyersdorf, P. T; Bigotta, S; Bilenko, I. A; Billingsley, G; Birindelli, S; Biswas, R; Bizouard, M. A; Black, E; Blackburn, J. K; Blackburn, L; Blair, D; Bland, B; Boccara, C; Bodiya, T. P; Bogue, L; Bondub, F; Bonelli, L; Bork, R; Boschi, V; Bose, S; Bosi, L; Braccinia, S; Bradaschia, C; Brady, P. R; Braginsky, V. B; Brau, J. E; Bridges, D. O; Brillet, A; Brinkmann, M; Brisson, V; Van Den Broeck, C; Brooks, A. F; Brown, D. A; Brummit, A; Brunet, G; Budzynski, R; Bulik, T; Bullington, A; Bulten, H. J; Buonanno, A; Burmeister, O; Buskulic, D; Byer, R. L; Cadonati, L; Cagnoli, G; Calloni, E; Camp, J. B; Campagna, E; Cannizzo, J; Cannon, K. C; Canuel, B; Cao, J; Carbognani, F; Cardenas, L; Caride, S; Castaldi, G; Caudill, S; Cavaglia, M; Cavalier, F; Cavalieri, R; Cella, G; Cepeda, C; Cesarini, E; Chalermsongsak, T; Chalkley, E; Charlton, P; Chassande-Mottin, E; Chatterji, S; Chelkowski, S; Chen, Y; Chincarini, A; Christensen, N; Chung, C. T. Y; Clark, D; Clark, J; Clayton, J. H; Cleva, F; Coccia, E; Cokelaer, T; Colacino, C. N; Colas, J; Colla, A; Colombini, M; Conte, R; Cook, D; Corbitt, T. R. C; Corda, C; Cornish, N; Corsi, A; Coulon, J. P; Coward, D; Coyne, D. C; Creighton, J. D. E; Creighton, T. D; Cruise, A. M; Culter, R. M; Cumming, A; Cunningham, L; Cuoco, E; Danilishin, S. L; D'Antonio, S; Danzmann, K; Dari, A; Dattilo, V; Daudert, B; Davier, M; Davies, G; Daw, E. J; Day, R; De Rosa, R; DeBra, D; Degallaix, J; del Prete, M; Dergachev, V; Desai, S; DeSalvo, R; Dhurandhar, S; Di Fiore, L; Di Lieto, A; Emilio, M. D. P; Di Virgilio, A; Diaz, M; Dietz, A; Donovan, F; Dooley, K. L; Doomes, E. E; Drago, M; Drever, R. W. P; Dueck, J; Duke, I; Dumas, J. C; Dwyer, J. G; Echols, C; Edgar, M; Effler, A; Ehrens, P; Espinoza, E; Etzel, T; Evans, M; Evans, T; Fafone, V; Fairhurst, S; Faltas, Y; Fan, Y; Fazi, D; Fehrmann, H; Ferrante, I; Fidecaro, F; Finn, L. S; Fiori, I; Flaminio, R; Flasch, K; Foley, S; Forrest, C; Fotopoulos, N; Fournier, J. D; Franc, J; Franzen, A; Frasca, S; Frasconi, F; Frede, M; Frei, M; Frei, Z; Freise, A; Frey, R; Fricke, T; Fritschel, P; Frolov, V. V; Fyffe, M; Galdi, V; Gammaitoni, L; Garofoli, J. A; Garufiab, F; Gemme, G; Genin, E; Gennai, A; Gholami, I; Giaime, J. A; Giampanis, S; Giardina, K. D; Giazotto, A; Goda, K; Goetz, E; Goggin, L. M; Gonzalez, G; Gorodetsky, M. L; Gossler, S; Gouaty, R; Granata, M; Granata, V; Grant, A; Gras, S; Gray, C; Gray, M; Greenhalgh, R. J. S; Gretarsson, A. M; Greverie, C; Grimaldi, F; Grosso, R; Grote, H; Grunewald, S; Guenther, M; Guidi, G; Gustafson, E. K; Gustafson, R; Hage, B; Hallam, J. M; Hammer, Derek; Hammond, G. D; Hanna, C; Hanson, J; Harms, J; Harry, G. M; Harry, I. W; Harstad, E. D; Haughian, K; Hayama, K; Heefner, J; Heitmann, H; Hello, P; Heng, I. S; Heptonstall, A; Hewitson, M; Hild, S; Hirose, E; Hoak, D; Hodge, K. A; Holt, K; Hosken, D. J; Hough, J; Hoyland, D; Huet, D; Hughey, B; Huttner, S. H; Ingram, D. R; Isogai, T; Ito, M; Ivanov, A; Jaranowski, P; Johnson, B; Johnson, W. W; Jones, D. I; Jones, G; Jones, R; de la Jordana, L. S; Ju, L; Kalmus, P; Kalogera, V; Kandhasamy, S; Kanner, J; Kasprzyk, D; Katsavounidis, E; Kawabe, K; Kawamura, S; Kawazoe, F; Kells, W; Keppel, D. G; Khalaidovski, A; Khalili, F. Y; Khan, R; Khazanov, E; King, P; Kissel, J. S; Klimenko, S; Kokeyama, K; Kondrashov, V; Kopparapu, R; Koranda, S; Kowalska, I; Kozak, D; Krishnan, B; Krolak, A; Kumar, R; Kwee, P; La Penna, P; Lam, P. K; Landry, M; Lantz, B; Lazzarini, A; Lei, H; Lei, M; Leindecker, N; Leonor, I; Leroy, N; Letendre, N; Li, C; Lin, H; Lindquist, P. E; Littenberg, T. B; Lockerbie, N. A; Lodhia, D; Longo, M; Lorenzini, M; Loriette, V; Lormand, M; Losurdo, G; Lu, P; Lubinski, M; Lucianetti, A; Luck, H; Machenschalk, B; MacInnis, M; Mackowski, J. M; Mageswaran, M; Mailand, K; Majorana, E; Mana, N; Mandel, I; Mandic, V; Mantovani, M; Marchesoni, F; Marion, F; Marka, S; Marka, Z; Markosyan, A; Markowitz, J; Maros, E; Marque, J; Martelli, F; Martin, I. W; Martin, R. M; Marx, J. N; Mason, K; Masserot, A; Matichard, F; Matone, L; Matzner, R. A; Mavalvala, N; McCarthy, R; McClelland, D. E; McGuire, S. C; McHugh, M; McIntyre, G; McKechan, D. J. A; McKenzie, K; Mehmet, M; Melatos, A; Melissinos, A. C; Mendell, G; Menendez, D. F; Menzinger, F; Mercer, R. A; Meshkov, S; Messenger, C; Meyer, M. S; Michel, C; Milano, L; Miller, J; Minelli, J; Minenkova, Y; Mino, Y; Mitrofanov, V. P; Mitselmakher, G; Mittleman, R; Miyakawa, O; Moe, B; Mohan, M; Mohanty, S. D; Mohapatra, S. R. P; Moreau, J; Moreno, G; Morgado, N; Morgia, A; Morioka, T; Mors, K; Mosca, S; Moscatelli, V; Mossavi, K; Mours, B; MowLowry, C; Mueller, G; Muhammad, D; zur Muhlen, H; Mukherjee, S; Mukhopadhyay, H; Mullavey, A; Muller-Ebhardt, H; Munch, J; Murray, P. G; Myers, E; Myers, J; Nash, T; Nelson, J; Neri, I; Newton, G; Nishizawa, A; Nocera, F; Numata, K; Ochsner, E; O'Dell, J; Ogin, G. H; O'Reilly, B; O'Shaughnessy, R; Ottaway, D. J; Ottens, R. S; Overmier, H; Owen, B. J; Pagliaroli, G; Palomba, C; Pan, Y; Pankow, C; Paoletti, F; Papa, M. A; Parameshwaraiah, V; Pardi, S; Pasqualetti, A; Passaquieti, R; Passuello, D; Patel, P; Pedraza, M; Penn, S; Perreca, A; Persichetti, G; Pichot, M; Piergiovanni, F; Pierro, V; Pietka, M; Pinard, L; Pinto, I. M; Pitkin, M; Pletsch, H. J; Plissi, M. V; Poggiani, R; Postiglione, F; Prato, M; Principe, M; Prix, R; Prodi, G. A; Prokhorov, L; Puncken, O; Punturo, M; Puppo, P; Quetschke, V; Raab, F. J; Rabaste, O; Rabeling, D. S; Radkins, H; Raffai, P; Raics, Z; Rainer, N; Rakhmanov, M; Rapagnani, P; Raymond, V; Re, V; Reed, C. M; Reed, T; Regimbau, T; Rehbein, H; Reid, S; Reitze, D. H; Ricci, F; Riesen, R; Riles, K; Rivera, B; Roberts, P; Robertson, N. A; Robinet, F; Robinson, C; Robinson, Edward L; Rocchi, A; Roddy, S; Rolland, L; Rollins, J; Romano, J. D; Romanoac, R; Romie, J. H; Rosinska, D; Rover, C; Rowan, S; Rudiger, A; Ruggi, P; Russell, P; Ryan, K; Sakata, S; Salemi, F; Sandberg, V; Sannibale, V; Santamaria, L; Saraf, S; Sarin, P; Sassolas, B; Sathyaprakash, B. S; Sato, S; Satterthwaite, M; Saulson, P. R; Savage, R; Savov, P; Scanlan, M; Schilling, R; Schnabel, R; Schofield, R; Schulz, B; Schutz, B. F; Schwinberg, P; Scott, J; Scott, S. M; Searle, A. C; Sears, B; Seifert, F; Sellers, D; Sengupta, A. S; Sentenac, D; Sergeev, A; Shapiro, B; Shawhan, P; Shoemaker, D. H; Sibley, A; Siemens, X; Sigg, D; Sinha, S; Sintes, A. M; Slagmolen, B. J. J; Slutsky, J; van der Sluys, M. V; Smith, J. R; Smith, Mathew R; Smith, N. D; Somiya, K; Sorazu, B; Stein, A; Stein, L. C; Steplewski, S; Stochino, A; Stone, R; Strain, K. A; Strigin, S; Stroeer, A; Sturani, R; Stuver, A. L; Summerscales, T. Z; Sun, K. X; Sung, M; Sutton, P. J; Swinkels, B; Szokoly, G. P; Talukder, D; Tang, L; Tanner, D. B; Tarabrin, S. P; Taylor, J. R; Taylor, R; Terenzi, R; Thacker, J; Thorne, K. A; Thorne, K. S; Uring, A. T. R; Tokmakov, K. V; Toncelli, A; Tonelli, M; Torres, C; Torrie, C; Tournefier, E; Travasso, F; Traylor, G; Trias, M; Trummer, J; Ugolini, D; Ulmen, J; Urbanek, K; Vahlbruch, H; Vajente, G; Vallisneri, M; van den Brand, J. F. J; van der Putten, S; Vass, S; Vaulin, R; Vavoulidis, M; Vecchio, A; Vedovato, G; van Veggel, A. A; Veitch, J; Veitch, P; Veltkamp, C; Verkindt, D; Vetrano, F; Vicere, A; Villar, A; Vineta, J. Y; Vocca, H; Vorvick, C; Vyachanin, S. P; Waldman, S. J; Wallace, L; Ward, R. L; Was, M; Weidner, A; Weinert, M; Weinstein, A. J; Weiss, R; Wen, L; Wen, S; Wette, K; Whelan, J. T; Whitcomb, S. E; Whiting, B. F; Wilkinson, C; Willems, P. A; Williams, H. R; Williams, L; Willke, B; Wilmut, I; Winkelmann, L; Winkler, W; Wipf, C. C; Wiseman, A. G; Woan, G; Wooley, R; Worden, J; Wu, W; Yakushin, I; Yamamoto, H; Yan, Z; Yoshida, S; Yvert, M; Zanolin, M; Zhang, J; Zhang, L; Zhao, C; Zotov, N; Zucker, M. E; Zweizig, J; Begin, S; Corongiu, A; D'Amico, N; Freire, P. C. C; Hessels, J. W. T; Hobbs, G. B; Kramer, M; Lyne, A. G; Manchester, R. N; Marshall, F. E; Middleditch, J; Possenti, A; Ransom, S. M; Stairs, I. H; Stappers, B; Ligo Sci Collaboration; Virgo, Collaboration
We present a search for gravitational waves from 116 known millisecond and young pulsars using data from the fifth science run of the LIGO detectors. For this search, ephemerides overlapping the run period were obtained for all pulsars using radio and X-ray observations. We demonstrate an updated search method that allows for small uncertainties in the pulsar phase parameters to be included in the search. We report no signal detection from any of the targets and therefore interpret our results as upper limits on the gravitational wave signal strength. The most interesting limits are those for young pulsars. We present updated limits on gravitational radiation from the Crab pulsar, where the measured limit is now a factor of 7 below the spin-down limit. This limits the power radiated via gravitational waves to be less than similar to 2% of the available spin-down power. For the X-ray pulsar J0537-6910 we reach the spin-down limit under the assumption that any gravitational wave signal from it stays phase locked to the X-ray pulses over timing glitches, and for pulsars J1913+1011 and J1952+3252 we are only a factor of a few above the spin-down limit. Of the recycled millisecond pulsars, several of themeasured upper limits are only about an order of magnitude above their spin-down limits. For these our best (lowest) upper limit on gravitational wave amplitude is 2.3 x 10(-26) for J1603-7202 and our best (lowest) limit on the inferred pulsar ellipticity is 7.0 x 10(-8) for J2124-3358. ; Australian Research Council ; Council of Scientific and Industrial Research of India ; Istituto Nazionale di Fisica Nucleare of Italy ; Spanish Ministerio de Educacion y Ciencia ; Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears ; Netherlands Organisation for Scientific Research ; Royal Society ; Scottish Funding Council ; Polish Ministry of Science and Higher Education ; Foundation for Polish Science ; Scottish Universities Physics Alliance ; National Aeronautics and Space Administration ; Carnegie Trust ; Leverhulme Trust ; David and Lucile Packard Foundation ; Research Corporation ; Alfred P. Sloan Foundation ; Natural Sciences and Engineering Research Council of Canada ; Commonwealth Government ; Astronomy
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Open Access#32015
SEARCHES FOR CONTINUOUS GRAVITATIONAL WAVES FROM NINE YOUNG SUPERNOVA REMNANTS
Aasi, J; Abbott, B. P; Abbott, R; Abbott, T; Abernathy, M. R; Acernese, F; Ackley, K; Adams, C; Adams, T; Addesso, P; Adhikari, R. X; Adya, V; Affeldt, C; Agathos, M; Agatsuma, K; Aggarwal, N; Aguiar, O. D; Ain, A; Ajith, P; Alemic, A; Allen, B; Allocca, A; Amariutei, D; Anderson, S. B; Anderson, W. G; Arai, K; Araya, M. C; Arceneaux, C; Areeda, J. S; Ast, S; Aston, S. M; Astone, P; Aufmuth, P; Aulbert, C; Aylott, B. E; Babak, S; Baker, P. T; Baldaccini, F; Ballardin, G; Ballmer, S. W; Barayoga, J. C; Barbet, M; Barclay, S; Barish, B. C; Barker, D; Barone, F; Barr, B; Barsotti, L; Barsuglia, M; Bartlett, J; Barton, M. A; Bartos, I; Bassiri, R; Basti, A; Batch, J. C; Bauer, Th. S; Baune, C; Bavigadda, V; Behnke, B; Bejger, M; Belczynski, C; Bell, A. S; Bell, C; Benacquista, M; Bergman, J; Bergmann, G; Berry, C. P. L; Bersanetti, D; Bertolini, A; Betzwieser, J; Bhagwat, S; Bhandare, R; Bilenko, I. A; Billingsley, G; Birch, J; Biscans, S; Bitossi, M; Biwer, C; Bizouard, M. A; Blackburn, J. K; Blackburn, L; Blair, C. D; Blair, D; Bloemen, S; Bock, O; Bodiya, T. P; Boer, M; Bogaert, G; Bojtos, P; Bond, C; Bondu, F; Bonelli, L; Bonnand, R; Bork, R; Born, M; Boschi, V; Bose, Sukanta; Bradaschia, C; Brady, P. R; Braginsky, V. B; Branchesi, M; Brau, J. E; Briant, T; Bridges, D. O; Brillet, A; Brinkmann, M; Brisson, V; Brooks, A. F; Brown, D. A; Brown, D. D; Brown, N. M; Buchman, S; Buikema, A; Bulik, T; Bulten, H. J; Buonanno, A; Buskulic, D; Buy, C; Cadonati, L; Cagnoli, G; Bustillo, J. Calderon; Calloni, E; Camp, J. B; Cannon, K. C; Cao, J; Capano, C. D; Carbognani, F; Caride, S; Caudill, S; Cavaglia, M; Cavalier, F; Cavalieri, R; Cella, G; Cepeda, C; Cesarini, E; Chakraborty, R; Chalermsongsak, T; Chamberlin, S. J; Chao, S; Charlton, P; Chassande-Mottin, E; Chen, Y; Chincarini, A; Chiummo, A; Cho, H. S; Cho, M; Chow, J. H; Christensen, N; Chu, Q; Chua, S; Chung, S; Ciani, G; Clara, F; Clark, J. A; Cleva, F; Coccia, E; Cohadon, P. -F; Colla, A; Collette, C; Colombini, M; Cominsky, L; Constancio, M; Conte, A; Cook, D; Corbitt, T. R; Cornish, N; Corsi, A; Costa, C. A; Coughlin, M. W; Coulon, J-P; Countryman, S; Couvares, P; Coward, D. M; Cowart, M. J; Coyne, D. C; Coyne, R; Craig, K; Creighton, J. D. E; Creighton, T. D; Cripe, J; Crowder, S. G; Cumming, A; Cunningham, L; Cuoco, E; Cutler, C; Dahl, K; Dal Canton, T; Damjanic, M; Danilishin, S. L; D'Antonio, S; Danzmann, K; Dartez, L; Dattilo, V; Dave, I; Daveloza, H; Davier, M; Davies, G. S; Daw, E. J; Day, R; Debra, D; Debreczeni, G; Degallaix, J; De laurentis, M; Deleglise, S; Del Pozzo, W; Denker, T; Dent, T; Dereli, H; Dergachev, V; De Rosa, R; DeRosa, R. T; DeSalvo, R; Dhurandhar, S; Diaz, M; Di Fiore, L; Di Lieto, A; Di Palma, I; Di Virgilio, A; Dojcinoski, G; Dolique, V; Dominguez, E; Donovan, F; Dooley, K. L; Doravari, S; Douglas, R; Downes, T. P; Drago, M; Driggers, J. C; Du, Z; Ducrot, M; Dwyer, S; Eberle, T; Edo, T; Edwards, M; Effler, A; Eggenstein, H-B; Ehrens, P; Eichholz, J; Eikenberry, S. S; Essick, R; Etzel, T; Evans, M; Evans, T; Factourovich, M; Fafone, V; Fairhurst, S; Fan, X; Fang, Q; Farinon, S; Farr, B; Farr, W. M; Favata, M; Fays, M; Fehrmann, H; Fejer, M. M; Feldbaum, D; Ferrante, I; Ferreira, E. C; Ferrini, F; Fidecaro, F; Fiori, I; Fisher, R. P; Flaminio, R; Fournier, J-D; Franco, S; Frasca, S; Frasconi, F; Frei, Z; Freise, A; Frey, R; Fricke, T. T; Fritschel, P; Frolov, V. V; Fuentes-Tapia, S; Fulda, P; Fyffe, M; Gair, J. R; Gammaitoni, L; Gaonkar, S; Garufi, F; Gatto, A; Gehrels, N; Gemme, G; Gendre, B; Genin, E; Gennai, A; Gergely, L. A; Ghosh, S; Giaime, J. A; Giardina, K. D; Giazotto, A; Gleason, J; Goetz, E; Goetz, R; Gondan, L; Gonzalez, G; Gordon, N; Gorodetsky, M. L; Gossan, S; Gossler, S; Gouaty, R; Graef, C; Graff, P. B; Granata, M; Grant, A; Gras, S; Gray, C; Greenhalgh, R. J. S; Gretarsson, A. M; Groot, P; Grote, H; Grunewald, S; Guidi, G. M; Guido, C. J; Guo, X; Gushwa, K; Gustafson, E. K; Gustafson, R; Hacker, J; Hall, E. D; Hammond, G; Hanke, M; Hanks, J; Hanna, C; Hannam, M. D; Hanson, J; Hardwick, T; Harms, J; Harry, G. M; Harry, I. W; Hart, M; Hartman, M. T; Haster, C-J; Haughian, K; Heidmann, A; Heintze, M; Heinzel, G; Heitmann, H; Hello, P; Hemming, G; Hendry, M; Heng, I. S; Heptonstall, A. W; Heurs, M; Hewitson, M; Hild, S; Hoak, D; Hodge, K. A; Hofman, D; Hollitt, S. E; Holt, K; Hopkins, P; Hosken, D. J; Hough, J; Houston, E; Howell, E. J; Hu, Y. M; Huerta, E; Hughey, B; Husa, S; Huttner, S. H; Huynh, M; Huynh-Dinh, T; Idrisy, A; Indik, N; Ingram, D. R; Inta, R; Islas, G; Isler, C; Isogai, T; Iyer, B. R; Izumi, K; Jacobson, M; Jang, H; Jaranowski, P; Jawahar, S; Ji, Y; Jimenez-Forteza, F; Johnson, W. W; Jones, D. I; Jones, R; Jonker, R. J. G; Ju, L; Haris, K; Kalogera, V; Kandhasamy, S; Kang, G; Kanner, J. 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United States National Science Foundation (NSF) ; Science and Technology Facilities Council (STFC) of the United Kingdom ; Max-Planck-Society (MPS) ; State of Niedersachsen/Germany ; Australian Research Council ; International Science Linkages program of the Commonwealth of Australia ; Council of Scientific and Industrial Research of India ; Department of Science and Technology, India ; Science & Engineering Research Board (SERB), India ; Ministry of Human Resource Development, India ; Spanish Ministerio de Economia y Competitividad ; Conselleria d'Economia i Competitivitat and Conselleria d'Educaci, Cultura i Universitats of the Govern de les Illes Balears ; Foundation for Fundamental Research on Matter - Netherlands Organization for Scientific Research ; Polish Ministry of Science and Higher Education ; FOCUS Programme of Foundation for Polish Science ; European Union ; Royal Society ; Scottish Funding Council ; Scottish Universities Physics Alliance ; National Aeronautics and Space Administration ; Hungarian Scientific Research Fund (OTKA) ; Lyon Institute of Origins (LIO) ; National Research Foundation of Korea ; Industry Canada ; Province of Ontario through the Ministry of Economic Development and Innovation ; National Science and Engineering Research Council Canada ; Brazilian Ministry of Science, Technology, and Innovation ; Carnegie Trust ; Leverhulme Trust ; David and Lucile Packard Foundation ; Research Corporation ; Alfred P. Sloan Foundation ; NSF ; STFC ; MPS ; INFN ; CNRS ; Science and Technology Facilities Council ; Science and Technology Facilities Council: ST/L000938/1 ; Science and Technology Facilities Council: ST/I006285/1 ; Science and Technology Facilities Council: ST/I006269/1 ; Science and Technology Facilities Council: ST/L000946/1 ; Science and Technology Facilities Council: ST/L000962/1 ; Science and Technology Facilities Council: ST/L003465/1 ; Science and Technology Facilities Council: ST/K000845/1 ; Science and Technology Facilities Council: ST/J00166X/1 ; Science and Technology Facilities Council: ST/L000911/1 Gravitational Waves ; Science and Technology Facilities Council: Gravitational Waves ; Science and Technology Facilities Council: PPA/G/S/2002/00652 ; Science and Technology Facilities Council: ST/I006269/1 Gravitational Waves ; Science and Technology Facilities Council: ST/L000911/1 ; Science and Technology Facilities Council: 1362895 ; Science and Technology Facilities Council: ST/I006277/1 ; Science and Technology Facilities Council: ST/H002359/1 ; Science and Technology Facilities Council: ST/K005014/1 ; Science and Technology Facilities Council: ST/K00137X/1 ; Science and Technology Facilities Council: ST/M006735/1 ; Science and Technology Facilities Council: ST/M000931/1 ; Science and Technology Facilities Council: ST/L000938/1 Gravitational Waves ; We describe directed searches for continuous gravitational waves (GWs) in data from the sixth Laser Interferometer Gravitational-wave Observatory (LIGO) science data run. The targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with non-pulsing suspected neutron stars. One target ' s parameters are uncertain enough to warrant two searches, for a total of 10. Each search covered a broad band of frequencies and first and second frequency derivatives for a fixed sky direction. The searches coherently integrated data from the two LIGO interferometers over time spans from 5.3-25.3 days using the matched-filtering. -statistic. We found no evidence of GW signals. We set 95% confidence upper limits as strong (low) as 4 x 10(-25) on intrinsic strain, 2 x 10(-7) on fiducial ellipticity, and 4 x 10(-5) on r-mode amplitude. These beat the indirect limits from energy conservation and are within the range of theoretical predictions for neutron-star ellipticities and r-mode amplitudes.
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