Search Results - "Grier, C. J."
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The Structure of the Broad-line Region in Active Galactic Nuclei. II. Dynamical Modeling of Data From the AGN10 Reverberation Mapping Campaign
Published in The Astrophysical journal (10-11-2017)“…We present inferences on the geometry and kinematics of the broad-Hβ line-emitting region in four active galactic nuclei monitored as part of the fall 2010…”
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THE SLOAN DIGITAL SKY SURVEY REVERBERATION MAPPING PROJECT: VELOCITY SHIFTS OF QUASAR EMISSION LINES
Published in The Astrophysical journal (01-11-2016)“…ABSTRACT Quasar emission lines are often shifted from the systemic velocity due to various dynamical and radiative processes in the line-emitting region. The…”
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The Sloan Digital Sky Survey Reverberation Mapping Project: Initial C iv Lag Results from Four Years of Data
Published in The Astrophysical journal (10-12-2019)“…We present reverberation-mapping (RM) lags and black hole mass measurements using the C ivλ1549 broad emission line from a sample of 348 quasars monitored as a…”
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The Sloan Digital Sky Survey Reverberation Mapping Project: Accretion Disk Sizes from Continuum Lags
Published in The Astrophysical journal (01-08-2019)“…We present accretion disk structure measurements from continuum lags in the Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) project. Lags are measured…”
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The Sloan Digital Sky Survey Reverberation Mapping Project: How Broad Emission Line Widths Change When Luminosity Changes
Published in The Astrophysical journal (01-11-2020)“…Quasar broad emission lines are largely powered by photoionization from the accretion continuum. Increased central luminosity will enhance line emissivity in…”
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Detection of Time Lags between Quasar Continuum Emission Bands Based On Pan-STARRS Light Curves
Published in The Astrophysical journal (20-02-2017)“…We study the time lags between the continuum emission of quasars at different wavelengths, based on more than four years of multi-band (g, r, i, z) light…”
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The Sloan Digital Sky Survey Reverberation Mapping Project: Systematic Investigations of Short-timescale C IV Broad Absorption Line Variability
Published in The Astrophysical journal (10-02-2019)“…We systematically investigate short-timescale (<10 day rest-frame) C iv broad absorption-line (BAL) variability to constrain quasar-wind properties and provide…”
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C IV BROAD ABSORPTION LINE ACCELERATION IN SLOAN DIGITAL SKY SURVEY QUASARS
Published in The Astrophysical journal (20-06-2016)“…ABSTRACT We present results from the largest systematic investigation of broad absorption line (BAL) acceleration to date. We use spectra of 140 quasars from…”
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Discovery of Nuclear X-ray Sources in Sings Galaxies
Published in The Astrophysical journal (10-04-2011)“…We present the results of a search for nuclear X-ray activity in nearby galaxies using Chandra archival data in a sample of 62 galaxies from the Spitzer…”
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The Sloan Digital Sky Survey Reverberation Mapping Project: Mg ii Lag Results from Four Years of Monitoring
Published in The Astrophysical journal (01-09-2020)“…We present reverberation mapping results for the Mg ii λ2800 broad emission line in a sample of 193 quasars at 0.35 < z < 1.7 with photometric and…”
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The Mass of the Black Hole in the Quasar PG 2130+099
Published in The Astrophysical journal (01-12-2008)“…We present the results of a recent reverberation-mapping campaign undertaken to improve measurements of the radius of the broad-line region and the central…”
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Taking a Long Look: A Two-decade Reverberation Mapping Study of High-luminosity Quasars
Published in The Astrophysical journal (01-07-2021)“…Abstract Reverberation mapping (RM) of active galactic nuclei (AGNs) has been used over the past three decades to determine AGN broad-line region (BLR) sizes…”
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The Sloan Digital Sky Survey Reverberation Mapping Project: The Hβ Radius-Luminosity Relation
Published in The Astrophysical journal (01-08-2020)“…Results from a few decades of reverberation mapping (RM) studies have revealed a correlation between the radius of the broad-line emitting region (BLR) and the…”
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THE TYPECASTING OF ACTIVE GALACTIC NUCLEI: Mrk 590 NO LONGER FITS THE ROLE
Published in The Astrophysical journal (01-12-2014)“…We present multi wavelength observations that trace more than 40 yr in the life of the active galactic nucleus (AGN) in Mrk 590, traditionally known as a…”
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STELLAR VELOCITY DISPERSION MEASUREMENTS IN HIGH-LUMINOSITY QUASAR HOSTS AND IMPLICATIONS FOR THE AGN BLACK HOLE MASS SCALE
Published in The Astrophysical journal (20-08-2013)“…We present new stellar velocity dispersion measurements for four luminous quasars with the Near-Infrared Integral Field Spectrometer instrument and the ALTAIR…”
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The Sloan Digital Sky Survey Reverberation Mapping Project: Hα and Hβ Reverberation Measurements from First-year Spectroscopy and Photometry
Published in The Astrophysical journal (10-12-2017)“…Abstract We present reverberation mapping results from the first year of combined spectroscopic and photometric observations of the Sloan Digital Sky Survey…”
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THE SLOAN DIGITAL SKY SURVEY REVERBERATION MAPPING PROJECT: FIRST BROAD-LINE Hβ AND Mg ii LAGS AT z 0.3 FROM SIX-MONTH SPECTROSCOPY
Published in The Astrophysical journal (10-02-2016)“…ABSTRACT Reverberation mapping (RM) measurements of broad-line region (BLR) lags in quasars are important for directly measuring black hole masses in these…”
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The Sloan Digital Sky Survey Reverberation Mapping Project: Low-ionization Broad-line Widths and Implications for Virial Black Hole Mass Estimation
Published in The Astrophysical journal (01-09-2019)“…The width of the broad emission lines in quasars is commonly characterized by either the FWHM or the square root of the second moment of the line profile (…”
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THE SIZE OF THE NARROW-LINE-EMITTING REGION IN THE SEYFERT 1 GALAXY NGC 5548 FROM EMISSION-LINE VARIABILITY
Published in The Astrophysical journal (20-12-2013)“…The narrow [OIII] [lambda][lambda]4959, 5007 emission-line fluxes in the spectrum of the well-studied Seyfert 1 galaxy NGC 5548 are shown to vary with time…”
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The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151
Published in The Astrophysical journal (01-10-2020)“…Abstract We derive a distance of 15.8 ± 0.4 Mpc to the archetypal Seyfert 1 galaxy NGC 4151 based on the near-infrared Cepheid period–luminosity relation and…”
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