Noise and signal reconstruction and characterization in the AURIGA detector

Details Noise and signal reconstruction and characterization in the AURIGA detector Noise and signal reconstruction and characterization in the AURIGA detector

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..523..423b&link_type=abstract

GRAVITATIONAL WAVES: Third Edoardo Amaldi Conference. AIP Conference Proceedings, Volume 523, pp. 423-424 (2000).

Physics

Gravitational Wave Detectors And Experiments, Data Analysis: Algorithms And Implementation, Data Management

Scientific paper

Both the noise power spectrum and signal transfer function must be well
known to reliably extract candidates of gravitational wave (GW) signals
using linear Wiener filters. We review AURIGA data analysis techniques
relative to post-filtering statistical tests and validation. .

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