Abstract
Accreting neutron stars in binary systems, and Sco X-1 in particular, are considered one of the prime astrophysical targets for Earth-based gravitational wave laser interferometers. Here we discuss a data analysis strategy that we have developed for this class of systems which is now being applied to the science data collected by GEO600 and LIGO.
| Original language | English |
|---|---|
| Pages (from-to) | S729-S734 |
| Journal | Classical and Quantum Gravity |
| Volume | 21 |
| Issue number | 5 |
| Early online date | 9 Feb 2004 |
| DOIs | |
| Publication status | Published - 7 Mar 2004 |
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