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

Year: 2012

Authors: Abadie J., Abbott B. P., Abbott R., Abbott T.D., Abernathy M., Accadia T., Acernese F., Adams C., Adhikari R., Affeldt C., Ajith P., Allen B., Allen G., Amador Ceron E., Amariutei D., Amin R. S., Anderson S. B., Anderson W. G., Arai K., Arain M. A., Araya M., Aston S., Astone P., Atkinson D., Aufmuth P., Aulbert C., Aylott B.E., Babak S., Baker P., Ballardin G., Ballmer S., Barker D., Barone F., Barr B., Barriga P. Barsotti L., Barsuglia M., Barton M.A., Bartos I., Bassiri R., Bastarrika M., Basti A., Batch J., Bauchrowitz, Bauer Th. S., Bebronne M., Behnke B., Beker M.G., Bell A. S., Belletoile A., Belopolski I., Benacquista M., Berliner J.M., Bertolini A., Betzwieser J., Beveridge N., Beyersdorf P.T., Bilenko I.A., Billingsley G ., Birch JK., Biswas R., Bitossi M., Bizouard M.A., Black E., Blackburn J.K., Blackburn L., Blair D., Bland B., Blom M., Bock O., Bodiya T. P., Bogan C., Bondarescu R., Bondu F., Bonelli L., Bonnand R., Bork R., Born M., Boschi V., Bose S., Bosi L., Bouhou B., Braccini S., Bradaschia C., Brady P.R., Braginsky V.B., Branchesi M., Brau J.E., Breyer J., Briant T., Bridges D.O., Brillet A., Brinkmann M., Brisson V., Britzger M., Brooks A.F., Brown D.A., Brummit A., Bulik T., Bulten H.J., Buonanno A., Burguet-Castell J., Burmeister O., Buskulic D., Buy C., Byer R.L., Cadonati L., Cagnoli G., Calloni E., Camp J.B., Campsie P., Cannizzo J., Cannon K., Canuel B., Cao J., Capano C.D., 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., Chiummo A., Cho h., Christensen N., Chua S.S.Y., Chung C.T.Y., Chung S., Ciani G., Clara F., Clark D.E., Clark J., Clayton J.H., Cleva F., Coccia E., Cohadon P.-F., Colacino C.N., Colas J., Colla A., Colombini M., Conte A., Conte R., Cook D., Corbitt T.R.C., Cordier M., Cornish N., Corsi A., Costa C.A., Coughlin M., Coulon J.P., Couvares P., Coward D.M., Coyne D.C., Creighton J.D.E., Creighton T.D., Cruise A. M., Cumming A., Cunningham L., Cuoco E., Cutler R.M., Dahl K., Danilishin S.L., Dannenberg R., D’Antonio S., Danzmann K., Dattilo V., Daudert B., Daveloza., Davier M., Davies G., Daw E.J., Day R., Dayanga T., De Rosa R., DeBra D., Debreczeni G., Degallaix J., Del Pozzo W., del Prete M., Dent T., Dergachev V., DeRosa r., DeSalvo R., Dhurandhar S., Di Fiore L., DiGuglielmo J., Di Lieto A., Di Palma I., Di Paolo Emilio M., Di Virgilio A., Diaz M., Dietz A., Donovan F., Dooley K.L., Dorsher S., Drago M., Drever R.W.P., Driggers J., Du Z., Dumas J.C., Dwyer S., Eberle T., Edgar M., Edwards M., Effler A., Ehrens P., Endroczi G., Engel R., Etzel T., Evans K., Evans M., Evans T., Factourovich M., Fafone V., Fairhurst S., Fan Y., Farr B.F., Farr W., Fazi D., Fehrmann H., Feldbaum D., Ferrante I., Fidecaro F., Finn L.S., Fiori I., Fisher R.P., Flaminio R. Flanigan M., Foley S., Forsi E., Forte L.A., Fotopoulos N., Fournier J.D., Franc J., Frasca S., Frasconi F., Frede M., Frei M., Frei Z., Freise A., Fey R., Fricke T.T., Friedrich D., Fritschel P., Frolov V.V., Fulda P., Fyffe M., Galimberti M., Gammaitoni L., Ganija M.R., Garcia J., Garofoli J.A., Garufi F., Gaspar M.E., Gemme G., Geng R., Genin E., Gennai A., Gergely L.A., Ghosh S., Giaime J.A., Giampanis S., Giardina K.D., Giazotto A., Gill C., Goetz E., Goggin L.M., Gonzalez G., Gorodetsky M.L., Gossler S., Gouaty R., Graef C., Granata M., Grant A., Gras S., Gray C., Gray N., Greenhalgh R. J. S., Gretarsson A. M., Greverie C., Grosso R., Grote H., Grunewald S., Guidi G.M., Guido C., Gupta R., Gustafson E.K., Gustafson R., Ha T., Hage B., Hallam J.M., Hammer D., Hammond G.D., Hanks J., Hanna C., Hanson J., Harms J., Harry G. M., Harry I.W., Harstad E.D., Hartman M.T., Haughian K., Hayama K., Hayau J.F., Hayler T., Heefner J., Heidmann A., Heintze M.C., Heitmann H., Hello P., Hendry M. A., Heng I.S., Heptonstall A., Herrera V., Hewitson M., Hild S., Hoak D., Hodge K.A., Holt K., Hong T., Hooper S., Hosken D.J., Hough J., Howell E., Hughey B., Husa S., Huttner S.H., Huynh-Dinh T., Ingram D.R., Inta R., Isogai T., Ivanov A., Izumi K., Jacobson M., Jang H., Jaranowski P., Johnson W.W., Jones D.I., Jones G., Jones R., Ju L., Kalmus P., Kalogera V., Kamaretsos I., Kandhasamy S., Kang G., Kanner J.B., Katsavounidis E., Katzman W., Kaufer H., Kawabe K., Kawamura S., Kawazoe F., Kells W., Keppel D.G., Keresztes Z., Khalaidovski A., Khalili F.Y., Khazanov E., Kim B., Kim C., Kim D., Kim H., King K., Kim N., Kim Y.M., King P.J., Kinsey M., Kissel J.S., Klimenko S., Kokeyama K., Kondrashov V., Kopparapu R.; Koranda S., Korth W.Z., Kowalska I., Kozak D., Kringel V., Krishnamurthy S., Krishnan B., Krolak A., Kuehn G., Kumar R., Kwee P., Lam P. K., Landry M., Lang M., Lantz B., Lastzka N., Lawrie C., Lazzarini A., Leaci P., Lee C.H., Lee H.M., Leindecker N., Leong J.R., Leonor I., Leroy N., Letendre N., Li J., Li T.G.F., Liguori N., Lindquist P.E., Lockerbie N.A., Lodhia D., Lorenzini M., Loriette V., Lormand M., Losurdo G., Luan J., Lubinski M., Lueck H., Lundgren A., Macdonald E., Machenschalk B., MacInnis M., Macleod D.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., Markosyan A., 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., Mazzolo G., McCarthy R., McClelland D.E., McGuire S.C., McIntyre G., McIver J., McKechan D.J.A., Medors G.D., Mehmet M., Meier T., Melatos A., Melissinos A., Mendell G., Menendez D.F., Mercer R.A., Meshkov S., Messenger C., Meyer M.S., Miao H., Michel C., Milano L., Miller J., Minenkov Y., Mitrofanov V.P., Mitselmakher G., Mittleman R., Miyakawa O., Moe B., Moesta P., Mohan M., Mohanty S.D., Mohapatra S.R.P., Moraru D., Moreno G., Morgado N., Morgia A., Mori T., Mosca S., Mossavi K., Mours B., Mow-Lowry C.M., Mueller G., Mueller S., Mukherjee S., Mullavey A., Mueller-Ebhardt H., Munch J., Murphy P.G., Murray P.G., Mytidis A., Nash T., Naticchioni L., Nawrodt R., Necula V., Nelson J., Newton G., Nishizawa A., Nocera F., Nolting D., Nuttall L., Ochsner E., O’Dell J., Oelker E., Ogin G.H., Oh J.J., Oh S.H., Oldenburg R., O’Reilly B., O’Shaughnessy R., Osthelder C., Ott C.D., Ottaway D.J., Ottens R.S., Overmier H., Owen B.J., Page A., Pagliaroli G., Palladino L., Palomba C., Pan Y., Pankow C., Paoletti F., Papa M.A., Parisi M., Pasqualetti A., Passaquieti R., Passuello D., Patel P., Pedraza M., Peiris P., Pekowsky L., Penn S., Peralta C., Perreca A., Persichetti G., Phelps M., Pickenpack M., Piergiovanni F., Pietka M., Pinard L., Pinto I. M., Pitkin M., Pletsch H. J., Plissi M. V., Poggiani R, Poeld J., Postiglione F., Prato M., Predoi V., Price L.r., Prijatelj M., Principe M., Privitera S., Prix R., Prodi G. A., Prokhorov L., Puncken O., Punturo M., Puppo P., Quetschke V., Raab F. J., Rabeling D. S., Racz I., Radkins H., Raffai P., Rakhmanov M., Ramet C.r., Rankins B., Rapagnani P., Raymond V., Re V., Redwine K., Reed C. M., Reed T., Regimbau T., Reid S., Reitze D. H., Ricci F., Riesen R., Riles K., Roberts P., Robertson N.A., Robinet F., Robinson C., Robinson E. L., Rocchi A., Roddy S., Rodriguez C., Rodruck M., Rolland L., Rollins J., Romano J. D., Romano R., Romie J. H., Rosinska D., Rover C., Rowan S., Rudiger A., Ruggi P., Ryan K., Ryll R., Sainathan P., Sakosky M., Salemi F., Samblowski A., Sammut L., Sancho de la Jordana L., Sandberg V., Sankar S., Sannibale V., Santamaria L., Santiago-Prieto L., Santostasi G., Sassolas B., Sathyaprakash B. S., Sato S., Saulson P. R., Savage R., Schilling R., Schlamminger S., Schnabel R., Schofield R., Schulz B., Schutz B. F., Schwinberg P., Scott J., Scott S. M., Searle A. C., Seifert F., Sellers D., Sengupta A. S., Sentenac D., Sergeev A., Shaddock D.A., Shaltev M., Shapiro B., Shawhan P., Shoemaker D. H., Sibley A., Siemens X., Sigg D., Singer A., Singer L., Sintes A. M., Skelton G., Slagmolen B. J. J., Slutsky J., Smith J. R., Smith M. R., Smith N. D., Smith R.J.E., Somiya K., Sorazu B., Soto J., Speirits F.C., Sperandio L., Stefszky M., Stein A. J., Steinet E., Steinlechner J., Steinlechner S., Steplewski S., Stochino A., Stone R., Strain K. A., Strigin S., Stroeer A., Sturani R., Stuver A. L., Summerscales T.Z., Sung M., Susmithan S., Sutton P. J., Swinkels B., Tacca M., Taffarello L., Talukder D., Tanner D. B., Tarabrin S. P., Taylor J. R., Taylor R., Thomas P., Thorne K. A., Thorne K. S., Thrane E., Thuering A., Titsler C., Tokmakov K. V., Toncelli A., Tonelli M., Torre O., Torres C., Torrie C. I., Tournefier E., Travasso F., Traylor G.., Trias M., Tseng K., Ugolini D., Urbanek K., Vahlbruch H., Vajente G., Vallisneri M., van den Brand J. F. J., Van Den Broeck C., van der Putten S., van der Veggel A. A., Vass S., Vasuth M., Vaulin R., Vavoulidis M., Vecchio A., Vedovato G., Veitch J., Veitch P. J., Veltkamp C., Verkindt D., Vetrano F., Vicere A., Villar A., Vinet J. -Y., Vitale S., Vitale S., Vocca H., Vorvick C., Vyachanin S.P., Wade A., Waldman S.J., Wallace L., Wan Y., Wang X., Wang Z., Wanner A., Ward R.L., Was M., Wei P., Weinert M., Weinstein A. J., Weiss R., Wen L., Wen S., Wessels P., West M., Westphal T., Wette K., Whelan J.T., Whitcomb S.E., White D., Whiting B. F., Wilkinson C., Willems P. A., Williams H. R., Williams L., Willke B., Winkelmann L., Winkler W., Wipf C. C., Wiseman A. G., Wittel H., 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., Zadrozny A., Zanolin M., Zendri J.-P., Zhang F., Zhang L., Zhang W., Zhang Z., Zhao C., Zotov N., Zucker M. E., Zweizig J.

Autors Affiliation: LIGO Calif Inst Technol, Pasadena, CA 91125 USA; Calif State Univ Fullerton, Fullerton, CA 92831 USA; Univ Glasgow, SUPA, Glasgow G12 8QQ, Lanark, Scotland; Univ Savoie, Lab Annecy Le Vieux Phys Particules LAPP, CNRS IN2P3, F-74941 Annecy Le Vieux, France; Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy; Univ Naples Federico II, Naples, Italy; Complesso Univ Monte S Angelo, I-80126 Naples, Italy; Univ Salerno, I-84084 Salerno, Italy; LIGO Livingston Observ, Livingston, LA 70754 USA; Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany; Leibniz Univ Hannover, D-30167 Hannover, Germany; Univ Wisconsin, Milwaukee, WI 53201 USA; Stanford Univ, Stanford, CA 94305 USA; Univ Florida, Gainesville, FL 32611 USA; Louisiana State Univ, Baton Rouge, LA 70803 USA; Univ Birmingham, Birmingham B15 2TT, W Midlands, England; Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy; Univ Roma La Sapienza, I-00185 Rome, Italy; LIGO Hanford Observ, Richland, WA 99352 USA; Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany; Montana State Univ, Bozeman, MT 59717 USA; European Gravitat Observ, I-56021 Cascina, PI, Italy; Syracuse Univ, Syracuse, NY 13244 USA; Univ Western Australia, Crawley, WA 6009, Australia; LIGO Massachusetts Inst Technol, Cambridge, MA 02139 USA; Univ Paris Diderot, Lab AstroParticule & Cosmol APC, CNRS IN2P3, CEA DSM IRFU,Observ Paris, F-75013 Paris, France; Columbia Univ, New York, NY 10027 USA; Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy; Univ Pisa, I-56100 Pisa, Italy; Univ Siena, I-53100 Siena, Italy; Nikhef, Amsterdam, Netherlands; Vrije Univ Amsterdam, NL-1081 HV Amsterdam, Netherlands; Univ Texas Brownsville & Texas Southmost Coll, Brownsville, TX 78520 USA; San Jose State Univ, San Jose, CA 95192 USA; Moscow MV Lomonosov State Univ, Moscow 119992, Russia; Univ Paris 11, LAL, IN2P3, CNRS, F-91898 Orsay, France; CNRS, ESPCI, F-75005 Paris, France; NASA Goddard Space Flight Ctr, Greenbelt, MD 20771 USA; Penn State Univ, University Pk, PA 16802 USA; Univ Nice Sophia Antipolis, CNRS, Observ Cote Azur, F-06304 Nice, France; Univ Rennes 1, Inst Phys Rennes, CNRS, F-35042 Rennes, France; Univ Lyon 1, CNRS, IN2P3, LMA, F-69622 Lyon, France; Washington State Univ, Pullman, WA 99164 USA; Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy; Univ Perugia, I-06123 Perugia, Italy; Ist Nazl Fis Nucl, Sez Firenze, I-50019 Sesto Fiorentino, Italy; Univ Urbino Carlo Bo, I-61029 Urbino, Italy; Univ Oregon, Eugene, OR 97403 USA; Univ Paris 06, Lab Kastler Brossel, ENS, CNRS, F-75005 Paris, France; Rutherford Appleton Lab, HSIC, Didcot OX11 0QX, Oxon, England; IM PAN, PL-00956 Warsaw, Poland; Warsaw Univ, Astron Observ, PL-00478 Warsaw, Poland; CAMK PAN, PL-716 Warsaw, Poland; Bialystok Univ, PL-15424 Bialystok, Poland; IPJ, PL-05400 Otwock, Poland; Inst Astron, PL-65265 Zielona Gora, Poland; Univ Maryland, College Pk, MD 20742 USA; Univ Massachusetts, Amherst, MA 01003 USA; Univ Mississippi, University, MS 38677 USA; Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada; Tsinghua Univ, Beijing 100084, Peoples R China; Univ Michigan, Ann Arbor, MI 48109 USA; Charles Sturt Univ, Wagga Wagga, NSW 2678, Australia; Caltech CaRT, Pasadena, CA 91125 USA; Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy; Pusan Natl Univ, Pusan 609735, South Korea; Carleton Coll, Northfield, MN 55057 USA; Australian Natl Univ, Canberra, ACT 0200, Australia; Univ Melbourne, Parkville, Vic 3010, Australia; Cardiff Univ, Cardiff CF24 3AA, S Glam, Wales; Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome, Italy; Univ Roma Tor Vergata, I-00133 Rome, Italy; Univ Aquila, I-67100 Laquila, Italy; Univ Salerno, I-84084 Salerno, Italy; Univ Sheffield, Sheffield S10 2TN, S Yorkshire, England; RMKI, H-1121 Budapest, Hungary; Ist Nazl Fis Nucl, Grp Collegato Trento, Trento, Italy; Univ Trento, I-38050 Povo, Trento, Italy; Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy; Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India; Univ Minnesota, Minneapolis, MN 55455 USA; CALTECH, Pasadena, CA 91125 USA; Northwestern Univ, Evanston, IL 60208 USA; Univ Texas Austin, Austin, TX 78712 USA; Eotvos Lorand Univ, H-1117 Budapest, Hungary; Univ Adelaide, Adelaide, SA 5005, Australia; Univ Szeged, H-6720 Szeged, Hungary; Embry Riddle Aeronaut Univ, Prescott, AZ 86301 USA; Natl Inst Math Sci, Taejon 305390, South Korea; Perimeter Inst Theoret Phys, Toronto, ON N2L 2Y5, Canada; Natl Astron Observ Japan, Tokyo 1818588, Japan; Univ Illes Balears, E-07122 Palma De Mallorca, Spain; Korea Inst Sci & Technol Informat, Taejon 305806, South Korea; Univ Southampton, Southampton SO17 1BJ, Hants, England; Inst Appl Phys, Nizhnii Novgorod 603950, Russia; Lund Observ, SE-22100 Lund, Sweden; Hanyang Univ, Seoul 133791, South Korea; Seoul Natl Univ, Seoul 151742, South Korea; Univ Strathclyde, Glasgow G1 1XQ, Lanark, Scotland; Southern Univ, Baton Rouge, LA 70813 USA; A&M Coll, Baton Rouge, LA 70813 USA; Univ Rochester, Rochester, NY 14627 USA; Rochester Inst Technol, Rochester, NY 14623 USA; Hobart & William Smith Coll, Geneva, NY 14456 USA; Univ Sannio Benevento, I-82100 Benevento, Italy; Louisiana Tech Univ, Ruston, LA 71272 USA; McNeese State Univ, Lake Charles, LA 70609 USA; Univ Washington, Seattle, WA 98195 USA; Andrews Univ, Berrien Springs, MI 49104 USA; Trinity Univ, San Antonio, TX 78212 USA; SE Louisiana Univ, Hammond, LA 70402 USA

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 h0 is 1  1024, while at the high end of our frequency range we achieve a worst-case upper limit of 3:8  1024 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.

Journal/Review: PHYSICAL REVIEW D

Volume: 85 (2)      Pages from: 022001  to: 022001

More Information: The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The 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 Educacion y Ciencia, the Conselleria d\’Economia Hisenda i Innovacio 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, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This document has been assigned LIGO Laboratory Document No. LIGO-P1100029-v36.
KeyWords: gravitational waves; science run; limit
DOI: 10.1103/PhysRevD.85.022001

Citations: 59
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