J/ApJ/813/39    LIGO gravitational-wave (GW) searches from SNRs    (Aasi+, 2015)

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 S., 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., Calderon Bustillo J., 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.JR, 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., Graf 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 J.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., K H., Kalogera V., Kandhasamy S., Kang G., Kanner J.B., Kasprzack M., Katsavounidis E., Katzman W., Kaufer H., Kaufer S., Kaur T., Kawabe K., Kawazoe F., Kefelian F., Keiser G.M., Keitel D., Kelley D.B., Kells W., Keppel D.G., Key J.S., Khalaidovski A., Khalili F.Y., Khazanov E.A., Kim C., Kim K., Kim N.G., Kim N., Kim Y.-M., King E.J., King P.J., Kinzel D.L., Kissel J.S., Klimenko S., Kline J., Koehlenbeck S., Kokeyama K., Kondrashov V., Korobko M., Korth W.Z., Kowalska I., Kozak D.B., Kringel V., Krishnan B., Krolak A., Krueger C., Kuehn G., Kumar A., Kumar P., Kuo L., Kutynia A., Landry M., Lantz B., Larson S., Lasky P.D., Lazzarini A., Lazzaro C., Le J., Leaci P., Leavey S., Lebigot E., Lebigot E.O., Lee C.H., Lee H.K., Lee H.M., Leonardi M., Leong J.R., Leroy N., Letendre N., Levin Y., Levine B., Lewis J., Li T.G.F., Libbrecht K., Libson A., Lin A.C., Littenberg T.B., Lockerbie N.A., Lockett V., Logue J., Lombardi A.L., Lorenzini M., Loriette V., Lormand M., Losurdo G., Lough J., Lubinski M.J., Luck H., Lundgren A.P., Lynch R., Ma Y., Macarthur J., MacDonald T., Machenschalk B., MacInnis M., Macleod D.M., Magana-Sandoval F., Magee R., Mageswaran M., Maglione C., Mailand K., Majorana E., Maksimovic I., Malvezzi V., Man N., Mandel I., Mandic V., Mangano V., Mansell G.L., Mantovani M., Marchesoni F., Marion F., Marka S., Marka Z., Markosyan A., Maros E., Martelli F., Martellini L., Martin I.W., Martin R.M., Martynov D., Marx J.N., Mason K., Masserot A., Massinger T.J., Matichard F., Matone L., Mavalvala N., Mazumder N., Mazzolo G., McCarthy R., McClelland D.E., McCormick S., McGuire S.C., McIntyre G., McIver J., McLin K., McWilliams S., Meacher D., Meadors G.D., Meidam J., Meinders M., Melatos A., Mendell G., Mercer R.A., Meshkov S., Messenger C., Meyers P.M., Mezzani F., Miao H., Michel C., Middleton H., Mikhailov E.E., Milano L., Miller A., Miller J., Millhouse M., Minenkov Y., Ming J., Mirshekari S., Mishra C., Mitra S., Mitrofanov V.P., Mitselmakher G., Mittleman R., Moe B., Moggi A., Mohan M., Mohanty S.D., Mohapatra S.R.P., Moore B., Moraru D., Moreno G., Morriss S.R., Mossavi K., Mours B., Mow-lowry C.M., Mueller C.L., Mueller G., Mukherjee S., Mullavey A., Munch J., Murphy D., Murray P.G., Mytidis A., Nagy M.F., Nardecchia I., Nash T., Naticchioni L., Nayak R.K., Necula V., Nedkova K., Nelemans G., Neri I., Neri M., Newton G., Nguyen T., Nielsen A.B., Nissanke S., Nitz A.H., Nocera F., Nolting D., Normandin M.E.N., Nuttall L.K., Ochsner E., O'dell J., Oelker E., Ogin G.H., Oh J.J., Oh S.H., Ohme F., Oppermann P., Oram R., O'Reilly B., Ortega W., O'Shaughnessy R., Osthelder C., Ott C.D., Ottaway D.J., Ottens R.S., Overmier H., Owen B.J., Padilla C., Pai A., Pai S., Palashov O., Palomba C., Pal-Singh A., Pan H., Pankow C., Pannarale F., Pant B.C., Paoletti F., Papa M.A., Paris H., Pasqualetti A., Passaquieti R., Passuello D., Patrick Z., Pedraza M., Pekowsky L., Pele A., Penn S., Perreca A., Phelps M., Pichot M., Piergiovanni F., Pierro V., Pillant G., Pinard L., Pinto I.M., Pitkin M., Poeld J., Poggiani R., Post A., Poteomkin A., Powell J., Prasad J., Predoi V., Premachandra S., Prestegard T., Price L.R., Prijatelj M., Principe M., Privitera S., Prix R., Prodi G.A., Prokhorov L., Puncken O., Punturo M., Puppo P., Purrer M., Qin J., Quetschke V., Quintero E., Quiroga G., Quitzow-James 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J., 813, 39 (2015)> =2015ApJ...813...39A 2015ApJ...813...39A (SIMBAD/NED BibCode)
ADC_Keywords: Interferometry ; Supernova remnants Keywords: gravitational waves; ISM: supernova remnants; stars: neutron Abstract: 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 F-statistic. We found no evidence of GW signals. We set 95% confidence upper limits as strong (low) as 4x10-25 on intrinsic strain, 2x10-7 on fiducial ellipticity, and 4x10-5 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. Description: The sixth LIGO science run (S6) ran from 2009 July 7 21:00:00 UTC (GPS 931035615) to 2010 October 21 00:00:00 UTC (GPS 971654415). It included two interferometers with 4-km arm lengths, H1 at LIGO Hanford Observatory (LHO) near Hanford, Washington and L1 at LIGO Livingston Observatory (LLO) near Livingston, Louisiana. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 45 10 Target objects and astronomical parameters used in each search table5.dat 31 4962 Upper limit data -------------------------------------------------------------------------------- See also: VII/272 : A catalogue of Galactic supernova remnants (Green, 2014) VII/267 : Gravitational Wave Galaxy Catalogue (White+ 2011) J/ApJ/760/12 : LIGO/Virgo gravitational-wave (GW) bursts with GRBs (Abadie+, 2012) J/ApJ/715/1438 : Gravitational-wave bursts with GRBs (Abbott+, 2010) J/ApJ/713/671 : Gravitational waves from pulsars (Abbott+, 2010) J/A+AS/58/197 : 11cm survey, 357.4≤l≤76, -1.5≤b≤1.5 (Reich+, 1984) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- SNR SNR Name (LLL.l+B.b; G) 11- 19 A9 --- OName Other name 21- 22 I2 h RAh Hour of right ascension (J2000) 23- 24 I2 min RAm Minute of right ascension (J2000) 25- 28 F4.1 s RAs Second of right ascension (J2000) 29 A1 --- DE- Sign of declination (J2000) 30- 31 I2 deg DEd Degree of declination (J2000) 32- 33 I2 arcmin DEm Arcminute of declination (J2000) 34- 35 I2 arcsec DEs Arcsecond of declination (J2000) 37- 40 F4.2 kpc Dist [0.2/8.5] Distance (D) (1) 42- 45 F4.2 kyr Age [0.1/5] Age (a) (1) -------------------------------------------------------------------------------- Note (1): Values of distance D and age a are at the optimistic (nearby and young) end of ranges given in the literature, except for the second search for Vela Jr. See the text for details and references. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- --- [G] 2- 10 A9 --- SNR Galactic coordinate name of SNR searched 11- 15 A5 --- Obs "_deep" or "_wide" for Vela Jr. (1) 17- 22 F6.1 Hz Freq [46.5/2033.5] Central frequency of upper limit band 24- 31 A8 --- Strain The 95% confidence limit on intrinsic GW strain -------------------------------------------------------------------------------- Note (1): The literature on G266.2-1.2 (Vela Jr.) features a wide range of age and distance estimates, enough that we performed two searches ("wide" and "deep"). The Vela Jr. wide search had jobs covering bands from 35mHz to nearly 2Hz at low frequencies, while the other searches had search job bands on the order of a few mHz to tens of mHz. See text for further explanations. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 11-Feb-2016
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