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19942026
most citedCoevolution (Or Not) of Supermassive Black Holes and Host Galaxies

4.2k citations · 53.7k across the 547 of their papers we have counts for

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Showing 2016 · astro-ph.GAShow all

21 papers · 2 filters

astro-ph.GA2016★ 58 cited

Chandra Survey of Nearby Galaxies: The Catalog

Rui She, Luis C. Ho, Hua Feng

We searched in the public archive of the Chandra X-ray Observatory as of March 2016 and assembled a sample of 719 galaxies within 50 Mpc with ACIS observations available. By cross-…

astro-ph.GA2016★ 2 cited

The (dark) halo-to-stellar mass ratio in the Spitzer Survey of Stellar Structure in Galaxies (SG)

Simón Díaz-García, Heikki Salo, Eija Laurikainen +1

We use 3.6 m photometry for 1154 disk galaxies () in the Spitzer Survey of Stellar Structure in Galaxies (SG, Sheth et al. 2010) to obtain the stellar compon…

astro-ph.GA2016★ 4 cited

Young star clusters in circumnuclear starburst rings

Richard de Grijs, Chao Ma, Siyao Jia +2

We analyse the cluster luminosity functions (CLFs) of the youngest star clusters in three galaxies exhibiting prominent circumnuclear starburst rings. We focus specifically on NGC…

astro-ph.GA2016★ 25 cited

The complex, dusty narrow-line region of NGC 4388: Gas-jet interactions, outflows, and extinction revealed by near-IR spectroscopy

A. Rodriguez-Ardila, R. E. Mason, L. Martins +14

We present Gemini/GNIRS spectroscopy of the Seyfert 2 galaxy NGC 4388, with simultaneous coverage from 0.85 - 2.5 m. Several spatially-extended emission lines are detected for t…

astro-ph.GA2016★ 11 cited

The Influence of Environment on the Chemical Evolution in Low-mass Galaxies

Yiqing Liu, Luis C. Ho, Eric Peng

The mean alpha-to-iron abundance ratio ([/Fe]) of galaxies is sensitive to the chemical evolution processes at early time, and it is an indicator of star formation timescale ($τ…

astro-ph.GA2016★ 19 cited

Improving the Flux Calibration in Reverberation Mapping by Spectral Fitting: Application to the Seyfert Galaxy MCG--6-30-15

Chen Hu, Jian-Min Wang, Luis C. Ho +4

We propose a method for the flux calibration of reverberation mapping spectra based on accurate measurement of [O III] emission by spectral fitting. The method can achieve…

astro-ph.GA2016★ 73 cited

Reverberation Mapping of the Broad-line Region in NGC 5548: Evidence for Radiation Pressure?

Kai-Xing Lu, Pu Du, Chen Hu +8

NGC 5548 is the best-observed reverberation-mapped active galactic nucleus with long-term, intensive monitoring. Here we report results from a new observational campaign between Ja…

astro-ph.GA2016★ 13 cited

Detection of Prominent Stellar Disks in the Progenitors of Present-day Massive Elliptical Galaxies

Roozbeh H. Davari, Luis C. Ho, Bahram Mobasher +1

Massive galaxies at higher redshifts ( 2) show different characteristics from their local counterparts: They are compact and most likely have a disk. In this study, w…

astro-ph.GA2016★ 14 cited

The Sloan Digital Sky Survey Reverberation Mapping Project: Biases in z>1.46 Redshifts due to Quasar Diversity

K. D. Denney, Keith Horne, W. N. Brandt +5

We use the coadded spectra of 32 epochs of Sloan Digital Sky Survey (SDSS) Reverberation Mapping Project observations of 482 quasars with z>1.46 to highlight systematic biases in t…

astro-ph.GA2016★ 60 cited

Measurement of the Black Hole Mass in NGC 1332 from ALMA Observations at 0.044 Arcsecond Resolution

Aaron J. Barth, Benjamin D. Boizelle, Jeremy Darling +4

We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 3 observations of CO(2-1) emission from the circumnuclear disk in the E/S0 galaxy NGC 1332 at 0.044" resolution…

astro-ph.GA2016★ 15 cited

On the limits of measuring the bulge and disk properties of local and high-redshift massive galaxies

Roozbeh Davari, Luis C. Ho, Chien Y. Peng

A considerable fraction of the massive quiescent galaxies at \emph{z} 2, which are known to be much more compact than galaxies of comparable mass today, appear to have a…

astro-ph.GA2016★ 172 cited

Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. V. A New Size-Luminosity Scaling Relation for the Broad-Line Region

Pu Du, Kai-Xing Lu, Zhi-Xiang Zhang +12

This paper reports results of the third-year campaign of monitoring super-Eddington accreting massive black holes (SEAMBHs) in active galactic nuclei (AGNs) between 2014-2015. Ten…

astro-ph.GA2016★ 20 cited

Chandra X-ray and Hubble Space Telescope Imaging of Optically Selected Kiloparsec-Scale Binary Active Galactic Nuclei II: Host Galaxy Morphology and AGN Activity

Jinyi Shangguan, Xin Liu, Luis C. Ho +4

Binary active galactic nuclei (AGNs) provide clues to how gas-rich mergers trigger and fuel AGNs and how supermassive black hole (SMBH) pairs evolve in a gas-rich environment. Whil…

astro-ph.GA2016★ 37 cited

Toward Precision Black Hole Masses with ALMA: NGC 1332 as a Case Study in Molecular Disk Dynamics

A. J. Barth, J. Darling, A. J. Baker +4

We present first results from a program of Atacama Large Millimeter/submillimeter Array (ALMA) CO(2-1) observations of circumnuclear gas disks in early-type galaxies. The program w…

astro-ph.GA2016★ 114 cited

Spectroscopic Indication for a Centi-parsec Supermassive Black Hole Binary in the Galactic Center of NGC 5548

Yan-Rong Li, Jian-Min Wang, Luis C. Ho +8

As a natural consequence of cosmological hierarchical structure formation, sub-parsec supermassive black hole binaries (SMBHBs) should be common in galaxies but thus far have elude…

astro-ph.GA2016★ 21 cited

The Carnegie-Irvine Galaxy Survey. IV. A Method to Determine the Average Mass Ratio of Mergers That Built Massive Elliptical Galaxies

Song Huang, Luis C. Ho, Chien Y. Peng +2

Many recent observations and numerical simulations suggest that nearby massive, early-type galaxies were formed through a "two-phase" process. In the proposed second phase, the ext…

astro-ph.GA2016★ 19 cited

Low-Mass Active Galactic Nuclei with Rapid X-Ray Variability

Luis Ho, Minjin Kim

We present a detailed study of the optical spectroscopic properties of 12 active galactic nuclei (AGNs) with candidate low-mass black holes (BHs) selected by Kamizasa et al. throug…

astro-ph.GA2016★ 115 cited

Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. VI. Velocity-resolved Reverberation Mapping of H Line

Pu Du, Kai-Xing Lu, Chen Hu +9

In the sixth of the series of papers reporting on a large reverberation mapping (RM) campaign of active galactic nuclei (AGNs) with high accretion rates, we present velocity-resolv…

astro-ph.GA2016★ 180 cited

The Sloan Digital Sky Survey Reverberation Mapping Project: Velocity Shifts of Quasar Emission Lines

Yue Shen, W. N. Brandt, Gordon T. Richards +9

Quasar emission lines are often shifted from the systemic velocity due to various dynamical and radiative processes in the line-emitting region. The level of these velocity shifts…

astro-ph.GA2016★ 35 cited

The Sloan Digital Sky Survey Reverberation Mapping Project: An Investigation of Biases in CIV Emission-Line Properties

K. D. Denney, Keith Horne, W. N. Brandt +6

We investigate the dependence on data quality of quasar properties measured from the CIV emission line region at high redshifts. Our measurements come from 32 epochs of Sloan Digit…

astro-ph.GA2016★ 67 cited

The Fundamental Plane of the Broad-line Region in Active Galactic Nuclei

Pu Du, Jian-Min Wang, Chen Hu +3

Broad emission lines in active galactic nuclei (AGNs) mainly arise from gas photoionized by continuum radiation from an accretion disk around a central black hole. The shape of the…