Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/48827
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DC Field | Value | Language |
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dc.contributor.author | Abbott, B. | - |
dc.contributor.author | Abbott, R. | - |
dc.contributor.author | Adhikari, R. | - |
dc.contributor.author | Ageev, A. | - |
dc.contributor.author | Allen, B. | - |
dc.contributor.author | Amin, R. | - |
dc.contributor.author | Anderson, S. | - |
dc.contributor.author | Anderson, W. | - |
dc.contributor.author | Araya, M. | - |
dc.contributor.author | Armandula, H. | - |
dc.contributor.author | Asiri, F. | - |
dc.contributor.author | Aufmuth, P. | - |
dc.contributor.author | Aulbert, C. | - |
dc.contributor.author | Babak, S. | - |
dc.contributor.author | Balasubramanian, R. | - |
dc.contributor.author | Ballmer, S. | - |
dc.contributor.author | Barish, B. | - |
dc.contributor.author | Barker, C. | - |
dc.contributor.author | Barker, D. | - |
dc.contributor.author | Barnes, M. | - |
dc.contributor.author | et al. | - |
dc.date.issued | 2004 | - |
dc.identifier.citation | Physical Review D: Particles, Fields, Gravitation and Cosmology, 2004; 69(8):082004-1-082004-16 | - |
dc.identifier.issn | 1550-7998 | - |
dc.identifier.issn | 1550-2368 | - |
dc.identifier.uri | http://hdl.handle.net/2440/48827 | - |
dc.description.abstract | Data collected by the GEO 600 and LIGO interferometric gravitational wave detectors during their first observational science run were searched for continuous gravitational waves from the pulsar J1939+2134 at twice its rotation frequency. Two independent analysis methods were used and are demonstrated in this paper: a frequency domain method and a time domain method. Both achieve consistent null results, placing new upper limits on the strength of the pulsar’s gravitational wave emission. A model emission mechanism is used to interpret the limits as a constraint on the pulsar’s equatorial ellipticity. | - |
dc.description.statementofresponsibility | B. Allen...C.J. Killow...C. Kim...D. Ottaway...et al. | - |
dc.language.iso | en | - |
dc.publisher | American Physical Soc | - |
dc.rights | ©2004 American Physical Society | - |
dc.source.uri | http://dx.doi.org/10.1103/physrevd.69.082004 | - |
dc.title | Setting upper limits on the strength of periodic gravitational waves from PSR J1939+2134 using the first science data from the GEO 600 and LIGO detectors | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1103/PhysRevD.69.082004 | - |
pubs.publication-status | Published | - |
dc.identifier.orcid | Ottaway, D. [0000-0001-6794-1591] | - |
Appears in Collections: | Aurora harvest Physics publications |
Files in This Item:
File | Description | Size | Format | |
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hdl_48827.pdf | Published version | 790.43 kB | Adobe PDF | View/Open |
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