C1IV:. Gravitational Wave Data Analysis

Astronomy and Astrophysics – Astrophysics

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Scientific paper

Resonant bar detectors are routinely searching for astronomical sources of gravitational waves and to setting upper limits on event rates. Interferometric detectors are beginning to operate at sensitivity levels good enough to set meaningful upper limits and begin astrophysical searches. With the long baseline interferometers scheduled to take data at unprecedented sensitivity levels the next few years will be a very exciting period for gravitational waves. In session C1iv there were talks focusing on gravitational wave searches (Krolak and Sintes), setting upper limits on astrophysical signals (Brady and Whelan), theoretical developments in modelling binary black holes (Iyer), testing general relativity with gravitational wave data (Will) and tools for gravitational wave data analysis (Schutz). There was also a one-hour round-table discussion on setting upper limits chaired by Andersson.

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