Calibration and Limitations of the Mg II line-based Black Hole Masses
arXiv:1804.02798 · doi:10.3847/1538-4357/aabf3e
Abstract
We present the single-epoch black hole mass (M) calibrations based on the rest-frame UV and optical measurements of Mg II 2798Å and H 4861Å lines and AGN continuum, using a sample of 52 moderate-luminosity AGNs at z0.4 and z0.6 with high-quality Keck spectra. We combine this sample with a large number of luminous AGNs from the Sloan Digital Sky Survey to increase the dynamic range for a better comparison of UV and optical velocity and luminosity measurements. With respect to the reference M based on the line dispersion of H and continuum luminosity at 5100Å, we calibrate the UV and optical mass estimators, by determining the best-fit values of the coefficients in the mass equation. By investigating whether the UV estimators show systematic trend with Eddington ratio, FWHM of H, the Fe II strength, and the UV/optical slope, we find no significant bias except for the slope. By fitting the systematic difference of Mg II-based and H-based masses with the L/L ratio, we provide a correction term as a function of the spectral index as C = 0.24 (1+) + 0.17, which can be added to the Mg II-based mass estimators if the spectral slope can be well determined. The derived UV mass estimators typically show 0.2 dex intrinsic scatter with respect to H-based M, suggesting that the UV-based mass has an additional uncertainty of 0.2 dex, even if high quality rest-frame UV spectra are available.
arXiv comment16 pages, 11 figures, 4 tables, accepted to be published in ApJ. Revised based on minor correction
References in corpus (50)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Stellar population synthesis at the resolution of 2003
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- Reverberation Measurements for 17 Quasars and the Size-Mass-Luminosity Relations in Active Galactic Nuclei
- Composite Quasar Spectra From the Sloan Digital Sky Survey
- 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
- Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships
- 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
- The Relationship Between Luminosity and Broad-Line Region Size in Active Galactic Nuclei
- AGN Black Hole Masses and Bolometric Luminosities
- Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei: I. Comparing the Photoionization and Reverberation Techniques
- The Radius-Luminosity Relationship for Active Galactic Nuclei: The Effect of Host-Galaxy Starlight on Luminosity Measurements II. The Full Sample of Reverberation-Mapped AGNs
- The cosmological evolution of quasar black-hole masses
- An Empirical Ultraviolet Template for Iron Emission in Quasars as Derived from I Zw 1
- Systematic Effects in Measurement of Black Hole Masses by Emission-Line Reverberation of Active Galactic Nuclei: Eddington Ratio and Inclination
- Measuring the black hole masses of high redshift quasars
- The Radius-Luminosity Relationship for Active Galactic Nuclei: The Effect of Host-Galaxy Starlight on Luminosity Measurements
- Modeling reverberation mapping data II: dynamical modeling of the Lick AGN Monitoring Project 2008 dataset
- The black hole mass - stellar velocity dispersion relation of narrow-line Seyfert 1 galaxies
- The Lick AGN Monitoring Project: The MBH - sigma Relation For Reverberation-Mapped Active Galaxies
- Fe II Emission in 14 Low-Redshift Quasars: I - Observations
- The Black Hole Mass - Galaxy Bulge Relationship for QSOs in the SDSS DR3
- 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 Lick AGN Monitoring Project 2011: Spectroscopic Campaign and Emission-Line Light Curves
- The Prevalence of Gas Outflows in Type 2 AGNs
- Cosmic Evolution of Black Holes and Spheroids. I: The M_BH-sigma Relation at z=0.36
- Comparing and calibrating black hole mass estimators for distant active galactic nuclei
- Do quiescent and active galaxies have different M_BH-sigma relations?
- Systematic Uncertainties in Black Hole Masses Determined from Single Epoch Spectra
- Recalibration of the virial factor and M-sigma relation for local active galaxies
- The Lick AGN Monitoring Project: Recalibrating Single-Epoch Virial Black Hole Mass Estimates
- The Sloan Digital Sky Survey Reverberation Mapping Project: First Broad-line Hbeta and MgII Lags at z>~0.3 from six-Month Spectroscopy
- Cosmic Evolution of Black Holes and Spheroids. IV. The BH Mass - Spheroid Luminosity Relation
- Are Outflows Biasing Single-Epoch CIV Black Hole Mass Estimates?
- The Lick AGN Monitoring Project 2011: Reverberation Mapping of Markarian 50
- The Mass of the Central Black Hole in the Seyfert Galaxy NGC 4151
- The relation between black hole mass and velocity dispersion at z~0.37
- Is Mg II 2800 a Reliable Virial Broadening Estimator for Quasars?
- Eddington ratio governs the equivalent width of MgII emission line in active galactic nuclei
- Cosmic Evolution of Black Holes and Spheroids. V. The Relation Between Black Hole Mass and Host Galaxy Luminosity for a Sample of 79 Active Galaxies
- Swift/UVOT grism monitoring of NGC 5548 in 2013: an attempt at MgII reverberation mapping
- Emission Line Properties of Seyfert Galaxies in the 12 Micron Sample
- MgII Line Variability of High Luminosity Quasars
- A New Approach to the Internal Calibration of Reverberation Mapping Spectra
- Relation between the variations in the MgII emission-line and the 3000 Å continuum
- Reverberation Mapping of PG 0934+013 with the Southern African Large Telescope
- Rest-frame UV single-epoch black hole mass estimates of low-luminosity AGN at intermediate redshifts
Cited by in corpus (33)
- H0LiCOW - IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant
- STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354
- Spectral properties of quasars from Sloan Digital Sky Survey data release 14: The catalog
- Reverberation mapping of Active Galactic Nuclei: from X-ray corona to dusty torus
- Gemini GNIRS near-infrared spectroscopy of 50 quasars at z>~5.7
- The X-shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars
- The X-SHOOTER/ALMA sample of Quasars in the Epoch of Reionization. I. NIR spectral modeling, iron enrichment and broad emission line properties
- A census of ionized gas outflows in type 1 AGNs: gas outflows in AGNs. V
- No Redshift Evolution in the Broad Line Region Metallicity up to z=7.54: Deep NIR Spectroscopy of ULAS J1342+0928
- Time delay measurement of Mg II line in CTS C30.10 with SALT
- No signs of star formation being regulated in the most luminous quasars at z~2 with ALMA
- Metallicity in Quasar Broad Line Regions at Redshift 6
- Rapid Black Hole Growth at the Dawn of the Universe: A Super-Eddington Quasar at z=6.6
- The FeII/MgII flux ratio of low-luminosity quasars at z~3
- The SOUX AGN sample: Optical/UV/X-ray SEDs and the nature of the disc
- Calibrating Mg II-based black-hole mass estimators using Low-to-High-Luminosity Active Galactic Nuclei
- The Farthest Quasar Mini-BAL Outflow from its Central Source: VLT/UVES Observation of SDSSJ0242+0049
- The MBHBM Project -- II. Molecular Gas Kinematics in the Lenticular Galaxy NGC 3593 Reveal a Supermassive Black Hole
- An FMOS Survey of moderate-luminosity broad-line AGN in COSMOS, SXDS and E-CDF-S
- Dating individual quasars with the HeII proximity effect
- Studying the [OIII]5007A emission-line width in a sample of 80 local active galaxies: A surrogate for ?
- Comparison of The UV and Optical Fe II Emission in Type 1 AGNs
- The SOUX AGN Sample: SDSS-XMM-Newton Optical, Ultraviolet and X-ray selected active galactic nuclei spanning a wide range of parameter space -- Sample definition
- VLT/UVES Observation of the Outflow in Quasar SDSS J1439-0106
- The first look at Narrow-Line Seyfert 1 Galaxies with eROSITA
- Spectroscopy of broad absorption line quasars at -- I: evidence for quasar winds shaping broad/narrow emission line regions
- [OIII] 5007A Emission Line Width as a Surrogate for stellar dispersion in Type 1 AGNs?
- Measuring the AGN sublimation radius with a new approach: reverberation mapping of the broad line polarization
- The U.S. Naval Observatory VLBI Spectroscopic Catalog
- Gemini Near Infrared Spectrograph - Distant Quasar Survey: Prescriptions for Calibrating UV-Based Estimates of Supermassive Black Hole Masses in High-Redshift Quasars
- Black Hole masses for 14 gravitational lensed quasars
- Uncertainty Quantification of the Virial Black Hole Mass with Conformal Prediction
- Strong correlation between FeII/MgII ratio and Eddington ratio of type 1 Active galactic nuclei