Dieses Ergebnis aus BASE kann Gästen nicht angezeigt werden. Login für vollen Zugriff.

SEARCH FOR GRAVITATIONAL WAVE BURSTS FROM SIX MAGNETARS

Title:	SEARCH FOR GRAVITATIONAL WAVE BURSTS FROM SIX MAGNETARS
Authors:	Abadie J; Abbott BP; Abbott R; Abernathy M; Accadia T; Acernese F; Adams C; Adhikari R; Affeldt C; Allen B; Allen GS; Ceron EA; Amariutei D; Amin RS; Anderson SB; Anderson WG; Antonucci F; Arai K; Arain MA; Araya MC; Aston SM; Astone P; Atkinson D; Aufmuth P; Aulbert C; Aylott BE; Babak S; Baker P; Ballardin G; Ballmer S; Barker D; Barnum S; Barone F; Barr B; Barriga P; Barsotti L; Barsuglia M; Barton MA; Bartos I; Bassiri R; Bastarrika M; Basti A; Bauchrowitz J; Bauer TS; Behnke B; Beker MG; Bell AS; Belletoile A; Belopolski I; Benacquista M; Bertolini A; Betzwieser J; Beveridge N; Beyersdorf PT; Bilenko IA; Billingsley G; Birch J; Birindelli S; Biswas R; Bitossi M; Bizouard MA; Black E; Blackburn JK; Blackburn L; Blair D; Bland B; Blom M; Bock O; Bodiya TP; Bogan C; Bondarescu R; Bondu F; Bonelli L; Bonnand R; Bork R; Born M; Boschi V; Bose S; Bosi L; Bouhou B; Boyle M; Braccini S; Bradaschia C; Brady PR; Braginsky VB; Brau JE; Breyer J; Bridges DO; Brillet A; Brinkmann M; Brisson V; Britzger M; Brooks AF; Brown DA; Brummit A; Budzynski R; Bulik T; Bulten HJ; Buonanno A; Burguet-Castell J; Burmeister O; Buskulic D; Buy C; Byer RL; Cadonati L; Cagnoli G; Cain J; Calloni E; Camp JB; Campagna E; Campsie P; Cannizzo J; Cannon K; Canuel B; Cao J; Capano C; Carbognani F; Caride S; Caudill S; Cavaglia M; Cavalier F; Cavalieri R; Cella G; Cepeda C; Cesarini E; Chaibi O; Chalermsongsak T; Chalkley E; Charlton P; Chassande-Mottin E; Chelkowski S; Chen Y; Chincarini A; Christensen N; Chua SSY; Chung CTY; Chung S; Clara F; Clark D; Clark J; Clayton JH; Cleva F; Coccia E; Colacino CN; Colas J; Colla A; Colombini M; Conte R; Cook D; Corbitt TR; Cornish N; Corsi A; Costa CA; Coughlin M; Coulon JP; Coward DM; Coyne DC; Creighton JDE; Creighton TD; Cruise AM; Culter RM; Cumming A; Cunningham L; Cuoco E; Dahl K; Danilishin SL; Dannenberg R; D'Antonio S; Danzmann K; Das K; Dattilo V; Daudert B; Daveloza H; Davier M; Davies G; Daw EJ; Day R; Dayanga T; De Rosa R; DeBra D; Debreczeni G; Degallaix J; del Prete M; Dent T; Dergachev V; DeRosa R; DeSalvo R; Dhurandhar S; Di Fiore L; Di Lieto A; Di Palma I; Emilio MDP; Di Virgilio A; Diaz M; Dietz A; Donovan F; Dooley KL; Dorsher S; Douglas ESD; Drago M; Drever RWP; Driggers JC; Dumas JC; Dwyer S; Eberle T; Edgar M; Edwards M; Effler A; Ehrens P; Engel R; Etzel T; Evans M; Evans T; Factourovich M; Fafone V; Fairhurst S; Fan Y; Farr BF; Fazi D; Fehrmann H; Feldbaum D; Ferrante I; Fidecaro F; Finn LS; Fiori I; Flaminio R; Flanigan M; Foley S; Forsi E; Forte LA; Fotopoulos N; Fournier JD; Franc J; Frasca S; Frasconi F; Frede M; Frei M; Frei Z; Freise A; Frey R; Fricke TT; Friedrich D; Fritschel P; Frolov VV; Fulda P; Fyffe M; Galimberti M; Gammaitoni L; Garcia J; Garofoli JA; Garufi F; Gaspar ME; Gemme G; Genin E; Gennai A; Ghosh S; Giaime JA; Giampanis S; Giardina KD; Giazotto A; Gill C; Goetz E; Goggin LM; Gonzalez G; Gorodetsky ML; Gossler S; Gouaty R; Graef C; Granata M; Grant A; Gras S; Gray C; Greenhalgh RJS; Gretarsson AM; Greverie C; Grosso R; Grote H; Grunewald S; Guidi GM; Guido C; Gupta R; Gustafson EK; Gustafson R; Hage B; Hallam JM; Hammer D; Hammond G; Hanks J; Hanna C; Hanson J; Harms J; Harry GM; Harry IW; Harstad ED; Hartman MT; Haughian K; Hayama K; Hayau JF; Hayler T; Heefner J; Heitmann H; Hello P; Hendry MA; Heng IS; Heptonstall AW; Herrera V; Hewitson M; Hild S; Hoak D; Hodge KA; Holt K; Hong T; Hooper S; Hosken DJ; Hough J; Howell EJ; Huet D; Hughey B; Husa S; Huttner SH; Ingram DR; Inta R; Isogai T; Ivanov A; Jaranowski P; Johnson WW; Jones DI; Jones G; Jones R; Ju L; Kalmus P; Kalogera V; Kandhasamy S; Kanner JB; Katsavounidis E; Katzman W; Kawabe K; Kawamura S; Kawazoe F; Kells W; Kelner M; Keppel DG; Khalaidovski A; Khalili FY; Khazanov EA; Kim H; Kim N; King PJ; Kinzel DL; Kissel JS; Klimenko S; Kondrashov V; Kopparapu R; Koranda S; Korth WZ; Kowalska I; Kozak D; Kringel V; Krishnamurthy S; Krishnan B; Krolak A; Kuehn G; Kumar R; Kwee P; Landry M; Lantz B; Lastzka N; Lazzarini A; Leaci P; Leong J; Leonor I; Leroy N; Letendre N; Li J; Li TGF; Liguori N; Lindquist PE; Lockerbie NA; Lodhia D; Lorenzini M; Loriette V; Lormand M; Losurdo G; Lu P; Luan J; Lubinski M; Luck H; Lundgren AP; Macdonald E; Machenschalk B; MacInnis M; Mageswaran M; Mailand K; Majorana E; Maksimovic I; Man N; Mandel I; Mandic V; Mantovani M; Marandi A; Marchesoni F; Marion F; Marka S; Marka Z; Maros E; Marque J; Martelli F; Martin IW; Martin RM; Marx JN; Mason K; Masserot A; Matichard F; Matone L; Matzner RA; Mavalvala N; McCarthy R; McClelland DE; McGuire SC; McIntyre G; McKechan DJA; Meadors G; Mehmet M; Meier T; Melatos A; Melissinos AC; Mendell G; Mercer RA; Merill L; Meshkov S; Messenger C; Meyer MS; Miao H; Michel C; Milano L; Miller J; Minenkov Y; Mino Y; Mitrofanov VP; Mitselmakher G; Mittleman R; Miyakawa O; Moe B; Moesta P; Mohan M; Mohanty SD; Mohapatra SRP; Moraru D; Moreno G; Morgado N; Morgia A; Mosca S; Moscatelli V; Mossavi K; Mours B; Mow-Lowry CM; Mueller G; Mukherjee S; Mullavey A; Muller-Ebhardt H; Munch J; Murray PG; Nash T; Nawrodt R; Nelson J; Neri I; Newton G; Nishida E; Nishizawa A; Nocera F; Nolting D; Ochsner E; O'Dell J; Ogin GH; Oldenburg RG; O'Reilly B; O'Shaughnessy R; Osthelder C; Ott CD; Ottaway DJ; Ottens RS; Overmier H; Owen BJ; Page A; Pagliaroli G; Palladino L; Palomba C; Pan Y; Pankow C; Paoletti F; Papa MA; Parameswaran A; Pardi S; Parisi M; Pasqualetti A; Passaquieti R; Passuello D; Patel P; Pathak D; Pedraza M; Pekowsky L; Penn S; Peralta C; Perreca A; Persichetti G; Phelps M; Pichot M; Pickenpack M; Piergiovanni F; Pietka M; Pinard L; Pinto IM; Pitkin M; Pletsch HJ; Plissi MV; Podkaminer J; Poggiani R; Poeld J; Postiglione F; Prato M; Predoi V; Price LR; Prijatelj M; Principe M; Privitera S; Prix R; Prodi GA; Prokhorov L; Puncken O; Punturo M; Puppo P; Quetschke V; Raab FJ; Rabeling DS; Racz I; Radkins H; Raffai P; Rakhmanov M; Ramet CR; Rankins B; Rapagnani P; Raymond V; Re V; Redwine K; Reed CM; Reed T; Regimbau T; Reid S; Reitze DH; Ricci F; Riesen R; Riles K; Roberts P; Robertson NA; Robinet F; Robinson C; Robinson EL; Rocchi A; Roddy S; Rolland L; Rollins J; Romano JD; Romano R; Romie JH; Rosinska D; Rover C; Rowan S; Udiger AR; Ruggi P; Ryan K; Sakata S; Sakosky M; Salemi F; Salit M; Sammut L; de la Jordana LS; Sandberg V; Sannibale V; Santamaria L; Santiago-Prieto I; Santostasi G; Saraf S; Sassolas B; Sathyaprakash BS; Sato S; Satterthwaite M; Saulson PR; Savage R; Schilling R; Schlamminger S; Schnabel R; Schofield RMS; Schulz B; Schutz BF; Schwinberg P; Scott J; Scott SM; Searle AC; Seifert F; Sellers D; Sengupta AS; Sentenac D; Sergeev A; Shaddock DA; Shaltev M; Shapiro B; Shawhan P; Weerathunga TS; Shoemaker DH; Sibley A; Siemens X; Sigg D; Singer A; Singer L; Sintes AM; Skelton G; Slagmolen BJJ; Slutsky J; Smith JR; Smith MR; Smith ND; Smith R; Somiya K; Sorazu B; Soto J; Speirits FC; Sperandio L; Stefszky M; Stein AJ; Steinlechner J; Steinlechner S; Steplewski S; Stochino A; Stone R; Strain KA; Strigin S; Stroeer AS; Sturani R; Stuver AL; Summerscales TZ; Sung M; Susmithan S; Sutton PJ; Swinkels B; Szokoly GP; Tacca M; Talukder D; Tanner DB; Tarabrin SP; Taylor JR; Taylor R; Thomas P; Thorne KA; Thorne KS; Thrane E; Thuring A; Titsler C; Tokmakov KV; Toncelli A; Tonelli M; Torre O; Torres C; Torrie CI; Tournefier E; Travasso F; Traylor G; Trias M; Tseng K; Turner L; Ugolini D; Urbanek K; Vahlbruch H; Vaishnav B; Vajente G; Vallisneri M; van den Brand JFJ; Van Den Broeck C; van der Putten S; van der Sluys MV; van Veggel AA; Vass S; Vasuth M; Vaulin R; Vavoulidis M; Vecchio A; Vedovato G; Veitch J; Veitch PJ; Veltkamp C; Verkindt D; Vetrano F; Vicere A; Villar AE; Vinet JY; Vocca H; Vorvick C; Vyachanin SP; Waldman SJ; Wallace L; Wanner A; Ward RL; Was M; Wei P; Weinert M; Weinstein AJ; Weiss R; Wen L; Wen S; Wessels P; West M; Westphal T; Wette K; Whelan JT; Whitcomb SE; White D; Whiting BF; Wilkinson C; Willems PA; Williams HR; Williams L; Willke B; Winkelmann L; Winkler W; Wipf CC; Wiseman AG; Woan G; Wooley R; Worden J; Yablon J; Yakushin I; Yamamoto H; Yamamoto K; Yang H; Yeaton-Massey D; Yoshida S; Yu P; Yvert M; Zanolin M; Zhang L; Zhang Z; Zhao C; Zotov N; Zucker ME; Zweizig J; Aptekar RL; Boynton WV; Briggs MS; Cline TL; Connaughton V; Frederiks DD; Gehrels N; Goldsten JO; Golovin D; van der Horst AJ; Hurley KC; Kaneko Y; von Kienlin A; Kouveliotou C; Krimm HA; Lin L; Mitrofanov I; Ohno M; Pal'shin VD; Rau A; Sanin A; Tashiro MS; Terada Y; Yamaoka K
Contributors:	Abadie, J; Abbott, Bp; Abbott, R; Abernathy, M; Accadia, T; Acernese, F; Adams, C; Adhikari, R; Affeldt, C; Allen, B; Allen, G; Ceron, Ea; Amariutei, D; Amin, R; Anderson, Sb; Anderson, Wg; Antonucci, F; Arai, K; Arain, Ma; Araya, Mc; Aston, Sm; Astone, P; Atkinson, D; Aufmuth, P; Aulbert, C; Aylott, Be; Babak, S; Baker, P; Ballardin, G; Ballmer, S; Barker, D; Barnum, S; Barone, F; Barr, B; Barriga, P; Barsotti, L; Barsuglia, M; Barton, Ma; Bartos, I; Bassiri, R; Bastarrika, M; Basti, A; Bauchrowitz, J; Bauer, T; Behnke, B; Beker, Mg; Bell, A; Belletoile, A; Belopolski, I; Benacquista, M; Bertolini, A; Betzwieser, J; Beveridge, N; Beyersdorf, Pt; Bilenko, Ia; Billingsley, G; Birch, J; Birindelli, S; Biswas, R; Bitossi, M; Bizouard, Ma; Black, E; Blackburn, Jk; Blackburn, L; Blair, D; Bland, B; Blom, M; Bock, O; Bodiya, Tp; Bogan, C; Bondarescu, R; Bondu, F; Bonelli, L; Bonnand, R; Bork, R; Born, M; Boschi, V; Bose, S; Bosi, L; Bouhou, B; Boyle, M; Braccini, S; Bradaschia, C; Brady, Pr; Braginsky, Vb; Brau, Je; Breyer, J; Bridges, Do; Brillet, A; Brinkmann, M; Brisson, V; Britzger, M; Brooks, Af; Brown, Da; Brummit, A; Budzynski, R; Bulik, T; Bulten, Hj; Buonanno, A; Burguet-Castell, J
Publication Year:	2011
Collection:	IRIS Università degli Studi di Bologna (CRIS - Current Research Information System)
Subject Terms:	gravitational waves
Description:	oft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitation of non-radial modes which would emit gravitational waves (GWs). We present the results of a search for GW bursts from six galactic magnetars that is sensitive to neutron star f-modes, thought to be the most efficient GW emitting oscillatory modes in compact stars. One of them, SGR 0501+4516, is likely ∼1 kpc from Earth, an order of magnitude closer than magnetars targeted in previous GW searches. A second, AXP 1E 1547.0−5408, gave a burst with an estimated isotropic energy >1044 erg which is comparable to the giant flares. We find no evidence of GWs associated with a sample of 1279 electromagnetic triggers from six magnetars occurring between 2006 November and 2009 June, in GW data from the LIGO, Virgo, and GEO600 detectors. Our lowest model-dependent GW emission energy upper limits for band- and time-limited white noise bursts in the detector sensitive band, and for f-mode ringdowns (at 1090 Hz), are 3.0 × 1044d21 erg and 1.4 × 1047d21 erg, respectively, where and d0501 is the distance to SGR 0501+4516. These limits on GW emission from f-modes are an order of magnitude lower than any previous, and approach the range of electromagnetic energies seen in SGR giant flares for the first time.
Document Type:	article in journal/newspaper
File Description:	ELETTRONICO
Language:	English
Relation:	info:eu-repo/semantics/altIdentifier/wos/WOS:000293135700010; volume:734; issue:2; firstpage:1; lastpage:9; numberofpages:9; journal:THE ASTROPHYSICAL JOURNAL LETTERS; https://hdl.handle.net/11585/998389
DOI:	10.1088/2041-8205/734/2/L35
Availability:	https://hdl.handle.net/11585/998389; https://doi.org/10.1088/2041-8205/734/2/L35
Accession Number:	edsbas.E1EF3B0F
Database:	BASE