Beating the spin-down limit on gravitational wave emission from the crab pulsar (2008, ApJ, 683, L45) [Erratum]

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The Astrophysical Journal 706 (1) , L203-L204. 10.1088/0004-637X/706/1/L203

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Abstract

A processing error in the signal template used in this search led to upper limits about 30% lower than we now know is warranted by the early S5 data. We have re-analyzed that data and find new upper limits on the strain parameter h 0 of 4.9 × 10–25/3.9 × 10–25 for uniform/restricted prior assumptions concerning the Crab inclination and polarization angles. These results have now been superseded by upper limits of 2.6 × 10–25/2.0 × 10–25 based on the full S5 data and presented in Abbott et al. (2009). The multitemplate search was not affected by the error. This is an Erratum for the article in Astrophysical Journal, 683 L45 2008

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	IOP
ISSN:	0004-637X
Last Modified:	13 Jan 2023 03:21
URI:	https://orca.cardiff.ac.uk/id/eprint/35750

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