The Sloan Digital Sky Survey Reverberation Mapping Project: Low-Ionization Broad-Line Widths and Implications for Virial Black Hole Mass Estimation
arXiv:1903.10015 · doi:10.3847/1538-4357/ab322b
Abstract
The width of the broad emission lines in quasars is commonly characterized either by the full-width-at-half-maximum (FWHM) or the square root of the second moment of the line profile (), and used as an indicator of the virial velocity of the broad-line region (BLR) in the estimation of black hole (BH) mass. We measure FWHM and for H, H and Mg II broad lines in both the mean and root-mean-square (rms) spectra of a large sample of quasars from the Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) project. We introduce a new quantitative recipe to measure that is reproducible, less susceptible to noise and blending in the wings, and scales with the intrinsic width of the line. We compare the four definitions of line width (FWHM and in mean and rms spectra, respectively) for each of the three broad lines and among different lines. There are strong correlations among different width definitions for each line, providing justification for using the line width measured in single-epoch spectroscopy as a virial velocity indicator. There are also strong correlations among different lines, suggesting alternative lines to H can be used to estimate virial BH masses. We further investigate the correlations between virial BH masses using different line width definitions and the stellar velocity dispersion of the host galaxies, and the dependence of line shape (characterized by the ratio FWHM/) on physical properties of the quasar. Our results provide further evidence that FWHM is more sensitive to the orientation of a flattened BLR geometry than , but the overall comparison between the virial BH mass and host stellar velocity dispersion does not provide conclusive evidence that one particular width definition is significantly better than the others.
arXiv comment14 pages, 9 figures. Accepted by ApJ
References in corpus (37)
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- The slope of the black-hole mass versus velocity dispersion correlation
- The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
- The 2.5 m Telescope of the Sloan Digital Sky Survey
- SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems
- Reverberation Measurements for 17 Quasars and the Size-Mass-Luminosity Relations in Active Galactic Nuclei
- Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei. II. A Homogeneous Analysis of a Large Reverberation-Mapping Database
- A Catalog of Quasar Properties from SDSS DR7
- Some Aspects of Measurement Error in Linear Regression of Astronomical Data
- Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships
- The Multi-Object, Fiber-Fed Spectrographs for SDSS and the Baryon Oscillation Spectroscopic Survey
- The Low-Luminosity End of the Radius-Luminosity Relationship for Active Galactic Nuclei
- Estimating Black Hole Masses in Active Galaxies Using the Halpha Emission Line
- Supermassive Black Holes in Active Galactic Nuclei. II. Calibration of the M-sigma Relationship for AGNs
- An Empirical Ultraviolet Template for Iron Emission in Quasars as Derived from I Zw 1
- Biases in Virial Black Hole Masses: An SDSS Perspective
- Systematic Effects in Measurement of Black Hole Masses by Emission-Line Reverberation of Active Galactic Nuclei: Eddington Ratio and Inclination
- An expanded M_bh-sigma diagram, and a new calibration of active galactic nuclei masses
- The diversity of quasars unified by accretion and orientation
- Eigenvector 1: An Optimal Correlation Space for Active Galactic Nuclei
- Comparing Single-Epoch Virial Black Hole Mass Estimators for Luminous Quasars
- The Lick AGN Monitoring Project: The MBH - sigma Relation For Reverberation-Mapped Active Galaxies
- Kepler Observations of Rapid Optical Variability in Active Galactic Nuclei
- The Sloan Digital Sky Survey Reverberation Mapping Project: H and H Reverberation Measurements From First-year Spectroscopy and Photometry
- Estimating Black Hole Masses in Active Galactic Nuclei Using the MgII 2800 Emission Line
- Stellar Velocity Dispersion Measurements in High-Luminosity Quasar Hosts and Implications for the AGN Black Hole Mass Scale
- The Sloan Digital Sky Survey Reverberation Mapping Project: Technical Overview
- The Lick AGN Monitoring Project 2011: Spectroscopic Campaign and Emission-Line Light Curves
- The Sloan Digital Sky Survey Reverberation Mapping Project: Sample Characterization
- Do quiescent and active galaxies have different M_BH-sigma relations?
- The Black Hole Mass Scale of Classical and Pseudo Bulges in Active Galaxies
- The Sloan Digital Sky Survey Reverberation Mapping Project: First Broad-line Hbeta and MgII Lags at z>~0.3 from six-Month Spectroscopy
- The Sloan Digital Sky Survey Reverberation Mapping Project: No Evidence for Evolution in the M-sigma Relation to z~1
- The effect of nuclear gas distribution on the mass determination of supermassive black holes
- Simultaneous Ultraviolet and Optical Emission-line Profiles of Quasars: Implications for Black Hole Mass Determination
- The orientation dependence of quasar single-epoch black hole mass scaling relationships
- Orientation and quasar black hole mass estimation
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- Systematically smaller single-epoch quasar black hole masses using a radius-luminosity relationship corrected for spectral bias
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- X-ray Unveiling Events in a z~1.6 Active Galactic Nucleus in the 7 Ms Chandra Deep Field-South
- Measuring the Time Variation of the Fine-structure Constant with Quasars Detected by LAMOST
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