  In order to investigate the growth of super-massive black holes (SMBHs), we
construct the black hole mass function (BHMF) and Eddington ratio distribution
function (ERDF) of X-ray-selected broad-line AGNs at z~1.4 in the Subaru
XMM-Newton Deep Survey field. In this redshift range, a significant part of the
accretion growth of SMBHs is thought to be taking place. Black hole masses of
X-ray-selected broad-line AGNs are estimated using the width of the broad MgII
line and the 3000A monochromatic luminosity. We supplement the MgII FWHM values
with the Ha FWHM obtained from our NIR spectroscopic survey. Using the black
hole masses of broad-line AGNs at redshifts between 1.18 and 1.68, the binned
broad-line AGN BHMF and ERDF are calculated using the Vmax method. To properly
account for selection effects that impact the binned estimates, we derive the
corrected broad-line AGN BHMF and ERDF by applying the Maximum Likelihood
method, assuming that the ERDF is constant regardless of the black hole mass.
We do not correct for the non-negligible uncertainties in virial BH mass
estimates. If we compare the corrected broad-line AGN BHMF with that in the
local Universe, the corrected BHMF at z~1.4 has a higher number density above
10^8 Msolar but a lower number density below that mass range. The evolution may
be indicative of a down-sizing trend of accretion activity among the SMBH
population. The evolution of broad-line AGN ERDF from z=1.4 to 0 indicates that
the fraction of broad-line AGNs with accretion rate close to the
Eddington-limit is higher at higher redshifts.
