Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21543306s&link_type=abstract
American Astronomical Society, AAS Meeting #215, #433.06; Bulletin of the American Astronomical Society, Vol. 42, p.370
Other
Scientific paper
We have computed the mass of the central black hole in 145 quasars chosen from the SDSS (Sloan Digital Sky Survey) DR3. The objects were chosen to sample the peak in quasar evolution and have redshifts in the range 1.85 < z < 4.26. Masses were computed using standard gas dynamics techniques with the luminosity at 1350Å and the width (FWHM) of the Doppler broadened Carbon IV emission line. Also, we were able to compare masses calculated from the CIV line with those calculated from the MgII line for one third of our data set. We will discuss how the mass of the SMBHs change over the range of redshifts and how this may be correlated with other quasar properties. This project is funded by a grant from NASA.
Carlton A. K.
Galaxy Evolution Survey Arkansas
Kashkanova A.
Kennefick Daniel
Kennefick Julia
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