Abstract
We present a data analysis technique for detecting a stochastic background of gravitational radiation. Current observational constraints and upper limits on the stochastic background signal strength, and methods for dealing with cross-correlated noise are also discussed.
Original language | English |
---|---|
Pages (from-to) | 212-221 |
Number of pages | 10 |
Journal | Proceedings of SPIE - The International Society for Optical Engineering |
Volume | 4856 |
DOIs | |
State | Published - 2002 |
Event | Gravitational - Wave Detection - Waikoloa, HI, United States Duration: Aug 23 2002 → Aug 25 2002 |
Keywords
- Data analysis
- Gravitational radiation
- Stochastic background