LISA Instrument Performance

Details LISA Instrument Performance LISA Instrument Performance

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008head...10.0601l&link_type=abstract

American Astronomical Society, HEAD meeting #10, #6.01

Computer Science

Performance

Scientific paper

LISA is designed to observe gravitational waves in the frequency band from 10-1 to 10-4 Hz, where a rich spectrum of sources is expected. The measurements must be made from space to avoid the large motions of the earth that prevent the current generation of detectors (e.g. LIGO) from operating at these frequencies. The technology and expected performance behind this measurement capability will be reviewed with an emphasis on the interferometric measurement system, including recent laboratory results showing a novel tunable frequency-stabilized laser.

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