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.
Abbott, B., et al. “Upper Limit Map of a Background of Gravitational Waves.” Physical Review D, vol. 76, no. 8, American Physical Society, Oct. 2007, p. 082003, doi:10.1103/PhysRevD.76.082003.
Physical Review D
©2007 American Physical Society. Original published version available at https://doi.org/10.1103/PhysRevD.76.082003