Observing Galactic Binary Populations with LISA

Details Observing Galactic Binary Populations with LISA Observing Galactic Binary Populations with LISA

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aps..apr.c4002b&link_type=abstract

American Physical Society, APS April Meeting, April 16-19, 2005, abstract #C4.002

Physics

Scientific paper

The Laser Interferometer Space Antenna (LISA) is a planned space- based gravitational wave detector that will be sensitive to gravitational waves in the mHz band. Although a wide variety of galactic and extra- galactic sources are expected in this band, the bulk of the signals will come from close compact-object binaries in the disk, halo, and globular cluster system of the Galaxy. The science reach of LISA and the information that can be gained from both the confusion-limited signal and individually resolved signals will be discussed.

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