Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-06-05
Phys.Rev.D62:041502,2000
Astronomy and Astrophysics
Astrophysics
to appear in Rapid Commun, Phys Rev D
Scientific paper
10.1103/PhysRevD.62.041502
Coalescence of low mass compact binaries of neutron stars and black holes are primary burst sources for LIGO and VIRGO.Of importance in the early stages of observations will be the classification of candidate detections by source-type. The diversity in source parameters and serendipity in any new window of observations suggest to consider model-independent detection algorithms. Here a frequency dynamics algorithm is described which extracts a trajectory in the $\dot{f}(f)$-plane from the noisy signal. The algorithm is studied in simulated binary coalescence. Robust results are obtained with experimental noise data. Experiments show the method to be superior to matched filtering in the presence of model imperfections.
Sarkar Abhinanda
van Putten Maurice H. P. M.
No associations
LandOfFree
An $\dot{f}(f)$-frequency dynamics algorithm for gravitational waves does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with An $\dot{f}(f)$-frequency dynamics algorithm for gravitational waves, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An $\dot{f}(f)$-frequency dynamics algorithm for gravitational waves will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-578603