Abstract
The LIGO Scientific Collaboration recently reported a new upper limit on an isotropic stochastic background of gravitational waves obtained based on the data from the third LIGO science run (S3). Here I present a new method for obtaining directional upper limits on stochastic gravitational waves that essentially implements a gravitational wave radiometer. The LIGO Scientific Collaboration intends to use this method for future LIGO science runs.
| Original language | English (US) |
|---|---|
| Pages (from-to) | S179-S185 |
| Journal | Classical and Quantum Gravity |
| Volume | 23 |
| Issue number | 8 |
| DOIs | |
| State | Published - Apr 21 2006 |
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)