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Upper limits on the strength of periodic gravitational waves from PSR J1939+2134

B Allen et al 2004 Class. Quantum Grav. 21 S671-S676   doi: 10.1088/0264-9381/21/5/042  Help

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B Allen39, G Woan35, (for the LIGO Scientific Collaboration), B Abbott13, R Abbott13, R Adhikari14, B Allen39, R Amin34, S B Anderson13, W G Anderson29, M Araya13, H Armandula13, F Asiri13, P Aufmuth31, C Aulbert1, S Babak7, R Balasubramanian7, S Ballmer14, B C Barish13, D Barker15, C Barker-Patton15, M Barnes13, B Barr35, M A Barton13, K Bayer14, R Beausoleil26, K Belczynski23, R Bennett35, S J Berukoff1, J Betzwieser14, B Bhawal13, G Billingsley13, E Black13, K Blackburn13, B Bland-Weaver15, B Bochner14, L Bogue13, R Bork13, S Bose40, P R Brady39, J E Brau37, D A Brown39, S Brozek31, A Bullington26, A Buonanno6, R Burgess14, D Busby13, W E Butler38, R L Byer26, L Cadonati14, G Cagnoli35, J B Camp21, C A Cantley35, L Cardenas13, K Carter16, M M Casey35, J Castiglione34, A Chandler13, J Chapsky13, P Charlton13, S Chatterji14, Y Chen6, V Chickarmane17, D Chin36, N Christensen8, D Churches7, C Colacino31,2, R Coldwell34, M Coles16, D Cook15, T Corbitt14, D Coyne13, J D E Creighton39, T D Creighton13, D R M Crooks35, P Csatorday14, B J Cusack3, C Cutler1, E D'Ambrosio13, K Danzmann31,2,20, R Davies7, E Daw17, D DeBra26, T Delker34, R DeSalvo13, S Dhurandar12, M Díaz29, H Ding13, R W P Drever4, R J Dupuis35, C Ebeling8, J Edlund13, P Ehrens13, E J Elliffe35, T Etzel13, M Evans13, T Evans16, C Fallnich31, D Farnham13, M M Fejer26, M Fine13, L S Finn28, É Flanagan9, A Freise2, R Frey37, P Fritschel14, V Frolov16, M Fyffe16, K S Ganezer5, J A Giaime17, A Gillespie13, K Goda14, G González17, S Goßler31, P Grandclément23, A Grant35, C Gray15, A M Gretarsson16, D Grimmett13, H Grote2, S Grunewald1, M Guenther15, E Gustafson26, R Gustafson36, W O Hamilton17, M Hammond16, J Hanson16, C Hardham26, G Harry14, A Hartunian13, J Heefner13, Y Hefetz14, G Heinzel2, I S Heng31, M Hennessy26, N Hepler28, A Heptonstall35, M Heurs31, M Hewitson35, N Hindman15, P Hoang13, J Hough35, M Hrynevych13, W Hua26, R Ingley33, M Ito37, Y Itoh1, A Ivanov13, O Jennrich35, W W Johnson17, W Johnston29, L Jones13, D Jungwirth13, V Kalogera23, E Katsavounidis14, K Kawabe20,2, S Kawamura22, W Kells13, J Kern16, A Khan16, S Killbourn35, C J Killow35, C Kim23, C King13, P King13, S Klimenko34, P Kloevekorn2, S Koranda39, K Kötter31, J Kovalik16, D Kozak13, B Krishnan1, M Landry15, J Langdale16, B Lantz26, R Lawrence14, A Lazzarini13, M Lei13, V Leonhardt31, I Leonor37, K Libbrecht13, P Lindquist13, S Liu13, J Logan13, M Lormand16, M Lubinski15, H Lück31,2, T T Lyons13, B Machenschalk1, M MacInnis14, M Mageswaran13, K Mailand13, W Majid13, M Malec31, F Mann13, A Marin14, S Márka13, E Maros13, J Mason13, K Mason14, O Matherny15, L Matone15, N Mavalvala14, R McCarthy15, D E McClelland3, M McHugh19, P McNamara35, G Mendell15, S Meshkov13, C Messenger33, G Mitselmakher34, R Mittleman14, O Miyakawa13, S Miyoki13, S Mohanty1, G Moreno15, K Mossavi2, B Mours13, G Mueller34, S Mukherjee1, J Myers15, S Nagano2, T Nash10, H Naundorf1, R Nayak12, G Newton35, F Nocera13, P Nutzman23, T Olson24, B O'Reilly16, D J Ottaway14, A Ottewill39, D Ouimette13, H Overmier16, B J Owen28, M A Papa1, C Parameswariah16, V Parameswariah15, M Pedraza13, S Penn11, M Pitkin35, M Plissi35, M Pratt14, V Quetschke31, F Raab15, H Radkins15, R Rahkola37, M Rakhmanov34, S R Rao13, D Redding13, M W Regehr13, T Regimbau14, K T Reilly13, K Reithmaier13, D H Reitze34, S Richman14, R Riesen16, K Riles36, A Rizzi16, D I Robertson35, N A Robertson35,26, L Robison13, S Roddy16, J Rollins14, J D Romano29, J Romie13, H Rong34, D Rose13, E Rotthoff28, S Rowan35, A Rüdiger20,2, P Russell13, K Ryan15, I Salzman13, G H Sanders13, V Sannibale13, B Sathyaprakash7, P R Saulson27, R Savage15, A Sazonov34, R Schilling20,2, K Schlaufman28, V Schmidt13, R Schofield37, M Schrempel31, B F Schutz1,7, P Schwinberg15, S M Scott3, A C Searle3, B Sears13, S Seel13, A S Sengupta12, C A Shapiro28, P Shawhan13, D H Shoemaker14, Q Z Shu34, A Sibley16, X Siemens39, L Sievers13, D Sigg15, A M Sintes1,32, K Skeldon35, J R Smith2, M Smith14, M R Smith13, P Sneddon35, R Spero13, G Stapfer16, K A Strain35, D Strom37, A Stuver28, T Summerscales28, M C Sumner13, P J Sutton28, J Sylvestre13, A Takamori13, D B Tanner34, H Tariq13, I Taylor7, R Taylor13, K S Thorne6, M Tibbits28, S Tilav13, M Tinto4, C Torres29, C Torrie13,35, S Traeger31, G Traylor16, W Tyler13, D Ugolini30, M Vallisneri6, M van Putten14, S Vass13, A Vecchio33, C Vorvick15, L Wallace13, H Walther20, H Ward35, B Ware13, K Watts16, D Webber13, A Weidner20,2, U Weiland31, A Weinstein13, R Weiss14, H Welling31, L Wen13, S Wen17, J T Whelan19, S E Whitcomb13, B F Whiting34, P A Willems13, P R Williams1, R Williams4, B Willke31,2, A Wilson13, B J Winjum28, W Winkler20,2, S Wise34, A G Wiseman39, G Woan35, R Wooley16, J Worden15, I Yakushin16, H Yamamoto13, S Yoshida25, I Zawischa31, L Zhang13, N Zotov18, M Zucker16 and J Zweizig13
1 Albert Einstein Institut für Gravitationsphysik, D-14476 Golm, Germany
2 Albert Einstein Institut für Gravitationsphysik, D-30157 Hannover, Germany
3 Australian National University, Canberra, 0200, Australia
4 California Institute of Technology, Pasadena, CA 91125, USA
5 California State University Dominguez Hills, Carson, CA 90747, USA
6 Caltech-CaRT, Pasadena, CA 91125, USA
7 Cardiff University, Cardiff, CF2 3YB, UK
8 Carleton College, Northfield, MN 55057, USA
9 Cornell University, Ithaca, NY 14853, USA
10 Fermi National Accelerator Laboratory, Batavia, IL 60510, USA
11 Hobart and William Smith Colleges, Geneva, NY 14456, USA
12 Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
13 LIGO—California Institute of Technology, Pasadena, CA 91125, USA
14 LIGO—Massachusetts Institute of Technology, Cambridge, MA 02139, USA
15 LIGO Hanford Observatory, Richland, WA 99352, USA
16 LIGO Livingston Observatory, Livingston, LA 70754, USA
17 Louisiana State University, Baton Rouge, LA 70803, USA
18 Louisiana Tech University, Ruston, LA 71272, USA
19 Loyola University, New Orleans, LA 70118, USA
20 Max Planck Institut für Quantenoptik, D-85748, Garching, Germany
21 NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA
22 National Astronomical Observatory of Japan, Tokyo 181-8588, Japan
23 Northwestern University, Evanston, IL 60208, USA
24 Salish Kootenai College, Pablo, MT 59855, USA
25 Southeastern Louisiana University, Hammond, LA 70402, USA
26 Stanford University, Stanford, CA 94305, USA
27 Syracuse University, Syracuse, NY 13244, USA
28 The Pennsylvania State University, University Park, PA 16802, USA
29 The University of Texas at Brownsville and Texas Southmost College, Brownsville, TX 78520, USA
30 Trinity University, San Antonio, TX 78212, USA
31 Universität Hannover, D-30167 Hannover, Germany
32 Universitat de les Illes Balears, E-07071 Palma de Mallorca, Spain
33 University of Birmingham, Birmingham, B15 2TT, UK
34 University of Florida, Gainsville, FL 32611, USA
35 University of Glasgow, Glasgow, G12 8QQ, UK
36 University of Michigan, Ann Arbor, MI 48109, USA
37 University of Oregon, Eugene, OR 97403, USA
38 University of Rochester, Rochester, NY 14627, USA
39 University of Wisconsin-Milwaukee, Milwaukee, WI 53201, USA
40 Washington State University, Pullman, WA 99164, USA

Abstract. The first science run of the LIGO and GEO gravitational wave detectors presented the opportunity to test methods of searching for gravitational waves from known pulsars. Here we present new direct upper limits on the strength of waves from the pulsar PSR J1939+2134 using two independent analysis methods, one in the frequency domain using frequentist statistics and one in the time domain using Bayesian inference. Both methods show that the strain amplitude at Earth from this pulsar is less than a few times 10−22.

PACS numbers: 04.80.Nn, 95.55.Ym, 97.60.Gb, 07.05.Kf

Print publication: Issue 5 (7 March 2004)
Received 2 October 2003
Published 9 February 2004

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