Upper limit map of a background of gravitational waves

Pitkin, M. (2007) Upper limit map of a background of gravitational waves. Physical Review D, 76 (8). ISSN 1550-7998

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Abstract

We searched for an anisotropic background of gravitational waves using data from the LIGO S4 science run and a method that is optimized for point sources. This is appropriate if, for example, the gravitational wave background is dominated by a small number of distinct astrophysical sources. No signal was seen. Upper limit maps were produced assuming two different power laws for the source strain power spectrum. For an f−3 power law and using the 50 Hz to 1.8 kHz band the upper limits on the source strain power spectrum vary between 1.2×10−48 Hz−1 (100 Hz/f)3 and 1.2×10−47 Hz−1  (100 Hz/f)3, depending on the position in the sky. Similarly, in the case of constant strain power spectrum, the upper limits vary between 8.5×10−49 Hz−1 and 6.1×10−48 Hz−1. As a side product a limit on an isotropic background of gravitational waves was also obtained. All limits are at the 90% confidence level. Finally, as an application, we focused on the direction of Sco-X1, the brightest low-mass x-ray binary. We compare the upper limit on strain amplitude obtained by this method to expectations based on the x-ray flux from Sco-X1.

Item Type:
Journal Article
Journal or Publication Title:
Physical Review D
Subjects:
ID Code:
135883
Deposited By:
Deposited On:
30 Jul 2019 14:15
Refereed?:
Yes
Published?:
Published
Last Modified:
19 Aug 2020 05:37