Black Hole masses for 14 gravitational lensed quasars
arXiv:2306.03472 · doi:10.1051/0004-6361/202347078
Abstract
We estimate black hole masses (M) for 14 gravitationally lensed quasars using the Balmer lines along with estimates based on MgII and CIV emission lines for four and two of them, respectively. We compare with results obtained for other lensed quasars. We use spectroscopic data from the Large Binocular Telescope (LBT), Magellan and the Very Large Telescope (VLT) to measure the FWHM of the broad emission lines. Combined with the bolometric luminosity measured from the spectra energy distribution, we estimate M including uncertainties from microlensing and variability. We obtain MBH using the single-epoch method from the H and/or H broad emission lines for 14 lensed quasars, including the first estimates for QJ0158-4325, HE0512-3329 and WFI2026-4536. The masses are typical of non-lensed quasars of similar luminosity, and the implied Eddington ratios are typical. We have increased the sample of lenses with estimates of MBH by 60%.
arXiv comment16 pages. Submitted to A&A
References in corpus (89)
- Unified Schemes for Radio-Loud Active Galactic Nuclei
- A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
- Energy input from quasars regulates the growth and activity of black holes and their host galaxies
- The slope of the black-hole mass versus velocity dispersion correlation
- 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
- The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity
- A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
- 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
- X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope
- A Method of Correcting Near-Infrared Spectra for Telluric Absorption
- 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
- Molecfit: A general tool for telluric absorption correction. I. Method and application to ESO instruments
- Automated data reduction workflows for astronomy
- 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
- Biases in Virial Black Hole Masses: An SDSS Perspective
- Molecfit: A general tool for telluric absorption correction II. Quantitative evaluation on ESO-VLT X-Shooter spectra
- H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: to 3.8% precision from strong lensing in a flat CDM model
- 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
- Determining Central Black Hole Masses in Distant Active Galaxies
- Probing the Coevolution of Supermassive Black Holes and Galaxies Using Gravitationally Lensed Quasar Hosts
- The Radius-Luminosity Relationship for Active Galactic Nuclei: The Effect of Host-Galaxy Starlight on Luminosity Measurements
- The Quasar Accretion Disk Size -- Black Hole Mass Relation
- The Quasar Accretion Disk Size - Black Hole Mass Relation
- An Alternative Approach To Measuring Reverberation Lags in Active Galactic Nuclei
- Low Resolution Spectral Templates For AGNs and Galaxies From 0.03 -- 30 microns
- Quantitative Interpretation of Quasar Microlensing Light Curves
- Comparing Single-Epoch Virial Black Hole Mass Estimators for Luminous Quasars
- What controls the C IV line profile in active galactic nuclei?
- The black hole mass - stellar velocity dispersion relation of narrow-line Seyfert 1 galaxies
- 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
- Early Growth and Efficient Accretion of Massive Black Holes at High Redshift
- The Lick AGN Monitoring Project 2011: Spectroscopic Campaign and Emission-Line Light Curves
- Correcting CIV-Based Virial Black Hole Masses
- Exploring the Low-Mass End of The M-Sigma Relation with Active Galaxies
- Cosmic Evolution of Mass Accretion Rate and Metalicity in Active Galactic Nuclei
- Comparing and calibrating black hole mass estimators for distant active galactic nuclei
- Black Hole Mass Estimates Based on CIV are Consistent with Those Based on the Balmer Lines
- Microlensing-Based Estimate of the Mass Fraction in Compact Objects in Lens
- Active galactic nuclei at z~1.5: II. Black Hole Mass estimation by means of broad emission lines
- The Microlensing Properties of a Sample of 87 Lensed Quasars
- Microlensing of the broad line region in 17 lensed quasars
- CIV Emission Line Properties and Systematic Trends in Quasar Black Hole Mass Estimates
- Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. VI. Velocity-resolved Reverberation Mapping of H Line
- The Sloan Digital Sky Survey Reverberation Mapping Project: Initial CIV Lag Results from Four Years of Data
- SDSS J092455.87+021924.9: an Interesting Gravitationally Lensed Quasar from the Sloan Digital Sky Survey
- Reverberation Mapping and the Physics of Active Galactic Nuclei
- Reverberation Mapping of Luminous Quasars at High-z
- HE 0435-1223: a wide separation quadruple QSO and gravitational lens
- WFI J2026-4536 and WFI J2033-4723: Two New Quadruple Gravitational Lenses
- Redshift Evolution in Black Hole-Bulge Relations: Testing CIV-based Black Hole Masses
- The Sloan Digital Sky Survey Quasar Lens Search. II. Statistical Lens Sample from the Third Data Release
- Is Mg II 2800 a Reliable Virial Broadening Estimator for Quasars?
- Calibrating CIV-based black hole mass estimators
- COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses III. Redshift of the lensing galaxy in eight gravitationally lensed quasars
- Gravitationally lensed quasars in Gaia -- IV. 150 new lenses, quasar pairs, and projected quasars
- MMT & Magellan Infrared Spectrograph
- 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
- SDSS J1335+0118: A New Two-Image Gravitational Lens
- A Study of Gravitational Lens Chromaticity with the Hubble Space Telescope
- Calibration and Limitations of the Mg II line-based Black Hole Masses
- Microlensing of the broad-line region in the quadruply imaged quasar HE0435-1223
- Data Reduction Pipeline for the MMT and Magellan Infrared Spectrograph
- H0LiCOW VII. Cosmic evolution of the correlation between black hole mass and host galaxy luminosity
- Can we improve CIV-based single epoch black hole mass estimations?
- Quasar Microlensing Variability Studies Favor Shallow Accretion Disk Temperature Profiles
- H0LiCOW VI. Testing the fidelity of lensed quasar host galaxy reconstruction
- Microlensing and Intrinsic Variability of the Broad Emission Lines of Lensed Quasars
- The Sloan Digital Sky Survey Reverberation Mapping Project: Improving Lag Detection with an Extended Multi-Year Baseline
- Strong Chromatic Microlensing in HE0047-1756 and SDSS1155+6346
- HST imaging of four gravitationally lensed quasars
- CTQ 414: A New Gravitational Lens
- Confirmation of Planet-Mass Objects in Extragalactic Systems
- Testing the Evolution of the Correlations between Supermassive Black Holes and their Host Galaxies using Eight Strongly Lensed Quasars
- I. Flux and color variations of the quadruply imaged quasar HE 0435-1223
- Estimate of the Accretion Disk Size in the Gravitationally Lensed Quasar HE 0435-1223 using Microlensing Magnification Statistics
- MiNDSTEp differential photometry of the gravitationally lensed quasars WFI2033-4723 and HE0047-1756: Microlensing and a new time delay
- The relation between supermassive black holes and their host galaxies
- Individual Estimates of the Virial Factor in 10 Quasars: Implications on the Kinematics of the Broad Line Region
- Testing Einstein's Equivalence Principle and its Cosmological Evolution from Quasar Gravitational Redshifts
- A Second-Order Moment of Microlensing Variability as a Novel Tool in Extragalactic Research