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DC Field | Value | Language |
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dc.contributor.author | Aasi, J. | - |
dc.contributor.author | Abbott, B.P. | - |
dc.contributor.author | Abbott, R. | - |
dc.contributor.author | Iyer, B.R. | - |
dc.contributor.author | LIGO Scientific Collaboration and Virgo Collaboration | - |
dc.contributor.author | +842 Co authors | - |
dc.date.accessioned | 2015-02-01T06:40:54Z | - |
dc.date.available | 2015-02-01T06:40:54Z | - |
dc.date.issued | 2015-01-15 | - |
dc.identifier.citation | Physical Review D, 2015, Vol.91, p 022004 | en |
dc.identifier.issn | 1550-7998 | - |
dc.identifier.issn | 1550-2368(Online) | - |
dc.identifier.uri | http://hdl.handle.net/2289/6156 | - |
dc.description | Open Access | en |
dc.description.abstract | In this paper we present the results of a coherent narrow-band search for continuous gravitational-wave signals from the Crab and Vela pulsars conducted on Virgo VSR4 data. In order to take into account a possible small mismatch between the gravitational-wave frequency and two times the star rotation frequency, inferred from measurement of the electromagnetic pulse rate, a range of 0.02 Hz around two times the star rotational frequency has been searched for both the pulsars. No evidence for a signal has been found and 95% confidence level upper limits have been computed assuming both that polarization parameters are completely unknown and that they are known with some uncertainty, as derived from x-ray observations of the pulsar wind torii. For Vela the upper limits are comparable to the spin-down limit, computed assuming that all the observed spin-down is due to the emission of gravitational waves. For Crab the upper limits are about a factor of 2 below the spin-down limit, and represent a significant improvement with respect to past analysis. This is the first time the spin-down limit is significantly overcome in a narrow-band search. | en |
dc.language.iso | en | en |
dc.publisher | American Physical Society | en |
dc.relation.uri | http://arxiv.org/abs/1410.8310 | en |
dc.relation.uri | http://dx.doi.org/10.1103/PhysRevD.91.022004 | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/2014arXiv1410.8310T | en |
dc.rights | 2015 American Physical Society | en |
dc.title | Narrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 data | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (TP) |
Files in This Item:
File | Description | Size | Format | |
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2015_PhysRevD_91_022004.pdf | Open Access | 736.88 kB | Adobe PDF | View/Open |
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