Constraining the Supermassive Black Hole Binary Population Using Pulsar Timing

Details Constraining the Supermassive Black Hole Binary Population Using Pulsar Timing Constraining the Supermassive Black Hole Binary Population Using Pulsar Timing

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21112006j&link_type=abstract

American Astronomical Society, AAS Meeting #211, #120.06; Bulletin of the American Astronomical Society, Vol. 39, p.950

Astronomy and Astrophysics

Astronomy

Scientific paper

Pulsar timing observations are used to place constraints on the merger rate of supermassive black hole binaries as a function of mass and red shift. Constraints are placed using currently available data from the Parkes Pulsar Timing Array project. Future constraints are estimated for various different scenarios including observations made with the Square Kilometer Array.

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