Observing Massive Black Hole Binary Coalescences with LISA

Details Observing Massive Black Hole Binary Coalescences with LISA Observing Massive Black Hole Binary Coalescences with LISA

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aps..aprr10003b&link_type=abstract

American Physical Society, APS April Meeting, April 16-19, 2005, abstract #R10.003

Astronomy and Astrophysics

Astrophysics

Scientific paper

Massive black hole binary coalescences are among the most important astrophysical sources of gravitational waves to be observed by LISA. The ability to observe and characterize such sources with masses ˜10^5 M and larger at high redshifts is strongly dependent on the sensitivity of LISA in the low frequency (0.1 mHz and below) regime. We examine LISA's ability to observe these systems at redshifts up to z ˜10 for various proposed values of the low frequency sensitivity, under current assumptions about the merger rates. The discussion will focus on the astrophysical information that can be gained by these observations.

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