The Sloan Digital Sky Survey Reverberation Mapping Project: estimating masses of black holes in quasars with single-epoch spectroscopy

E Dalla Bontà, BM Peterson, MC Bentz… - The Astrophysical …, 2020 - iopscience.iop.org
It is well known that reverberation mapping of active galactic nuclei (AGNs) reveals a
relationship between AGN luminosity and the size of the broad-line region, and that use of …

The 2dF QSO Redshift Survey–XII. The spectroscopic catalogue and luminosity function

SM Croom, RJ Smith, BJ Boyle, T Shanks… - Monthly Notices of …, 2004 - academic.oup.com
We present the final catalogue of the 2dF QSO Redshift Survey (2QZ), based on Anglo-
Australian Telescope 2dF spectroscopic observations of 44 576 colour-selected (ub J r) …

The cosmological evolution of quasar black hole masses

RJ McLure, JS Dunlop - Monthly Notices of the Royal …, 2004 - academic.oup.com
Virial black hole mass estimates are presented for 12 698 quasars in the redshift interval
0.1≤ z≤ 2.1, based on modelling of spectra from the Sloan Digital Sky Survey (SDSS) first …

Black hole masses and eddington ratios at 0.3< z< 4

JA Kollmeier, CA Onken, CS Kochanek… - The Astrophysical …, 2006 - iopscience.iop.org
We study the distribution of Eddington luminosity ratios, L bol/L Edd, of active galactic nuclei
(AGNs) discovered in the AGN and Galaxy Evolution Survey (AGES). We combine Hβ, Mg II …

The 2dF QSO Redshift Survey–XIV. Structure and evolution from the two-point correlation function

SM Croom, BJ Boyle, T Shanks, RJ Smith… - Monthly Notices of …, 2005 - academic.oup.com
In this paper we present a clustering analysis of quasi-stellar objects (QSOs) using over
20000 objects from the final catalogue of the 2dF QSO Redshift Survey (2QZ), measuring the …

What controls the C iv line profile in active galactic nuclei?

A Baskin, A Laor - Monthly Notices of the Royal Astronomical …, 2005 - academic.oup.com
The high-ionization lines in active galactic nuclei (AGN), such as C iv, tend to be blueshifted
with respect to the lower-ionization lines, such as Hβ, and often show a strong blue excess …

Estimating black hole masses in active galactic nuclei using the Mg II λ2800 emission line

JG Wang, XB Dong, TG Wang, LC Ho… - The Astrophysical …, 2009 - iopscience.iop.org
We investigate the relationship between the linewidths of broad Mg ii λ2800 and Hβ in active
galactic nuclei (AGNs) to refine them as tools to estimate black hole (BH) masses. We …

The black hole mass-galaxy bulge relationship for QSOs in the sloan digital sky survey data release 3

S Salviander, GA Shields, K Gebhardt… - The Astrophysical …, 2007 - iopscience.iop.org
We investigate the relationship between black hole mass, M BH, and host galaxy velocity
dispersion, σ*, for QSOs in Data Release 3 of the Sloan Digital Sky Survey. We derive M BH …

Near-infrared spectroscopy of high-redshift active galactic nuclei. I. A metallicity-accretion rate relationship

O Shemmer, H Netzer, R Maiolino, E Oliva… - The Astrophysical …, 2004 - iopscience.iop.org
We present new near-infrared spectroscopic measurements of the Hβ region for a sample of
29 luminous high-redshift quasars. We have measured the width of Hβ in those sources and …

Cosmic evolution of quasar clustering: implications for the host haloes

C Porciani, M Magliocchetti… - Monthly Notices of the …, 2004 - academic.oup.com
We present detailed clustering measurements from the 2dF Quasi-Stellar Object Redshift
Survey (2QZ) in the redshift range 0.8< z< 2.1. Using a flux-limited sample of∼ 14 000 …