Search Results - "Bentz, M. C."
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SWIFT/UVOT GRISM MONITORING OF NGC 5548 IN 2013: AN ATTEMPT AT Mg ii REVERBERATION MAPPING
Published in The Astrophysical journal (10-09-2015)“…ABSTRACT Reverberation-mapping-based scaling relations are often used to estimate the masses of black holes from single-epoch spectra of active galactic nuclei…”
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Space Telescope and Optical Reverberation Mapping Project. XI. Disk-wind Characteristics and Contributions to the Very Broad Emission Lines of NGC 5548
Published in The Astrophysical journal (01-08-2020)“…In 2014 the NGC 5548 Space Telescope and Optical Reverberation Mapping campaign discovered a two-month anomaly when variations in the absorption and emission…”
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Diverse Kinematic Signatures from Reverberation Mapping of the Broad-Line Region in AGNs
Published in The Astrophysical journal (20-10-2009)“…A detailed analysis of the data from a high sampling rate, multi-month reverberation mapping campaign, undertaken primarily at MDM Observatory with supporting…”
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THE INFRARED LIGHT CURVE OF SN 2011fe IN M101 AND THE DISTANCE TO M101
Published in The Astrophysical journal (20-07-2012)“…We present near-infrared light curves of supernova (SN) 2011fe in M101, including 34 epochs in H band starting 14 days before maximum brightness in the B band…”
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Reverberation Mapping Measurements of Black Hole Masses in Six Local Seyfert Galaxies
Published in The Astrophysical journal (20-09-2010)“…We present the final results from a high sampling rate, multi-month, spectrophotometric reverberation mapping campaign undertaken to obtain either new or…”
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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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TLDR: time lag/delay reconstructor
Published in Monthly notices of the Royal Astronomical Society (01-08-2021)“…ABSTRACT We present the time lag/delay reconstructor (TLDR), an algorithm for reconstructing velocity delay maps in the maximum a posteriori framework for…”
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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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A Revised Broad-line Region Radius and Black Hole Mass for the Narrow-line Seyfert 1 NGC 4051
Published in The Astrophysical journal (10-09-2009)“…We present the first results from a high sampling rate, multimonth reverberation mapping campaign undertaken primarily at MDM Observatory with supporting…”
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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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The AGNIFS survey: spatially resolved observations of hot molecular and ionized outflows in nearby active galaxies
Published in Monthly notices of the Royal Astronomical Society (01-05-2023)“…ABSTRACT We present the hot molecular and warm ionized gas kinematics for 33 nearby (0.001 ≲ z ≲ 0.056) X-ray selected active galaxies using the H$_2\,…”
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ON THE SCATTER IN THE RADIUS-LUMINOSITY RELATIONSHIP FOR ACTIVE GALACTIC NUCLEI
Published in The Astrophysical journal (01-03-2015)“…We investigate and quantify the observed scatter in the empirical relationship between the broad line region size R and the luminosity of the active galactic…”
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THE STRUCTURE OF THE BROAD-LINE REGION IN ACTIVE GALACTIC NUCLEI. I. RECONSTRUCTED VELOCITY-DELAY MAPS
Published in The Astrophysical journal (10-02-2013)“…We present velocity-resolved reverberation results for five active galactic nuclei. We recovered velocity-delay maps using the maximum entropy method for four…”
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The AGNIFS survey: distribution and excitation of the hot molecular and ionized gas in the inner kpc of nearby AGN hosts
Published in Monthly notices of the Royal Astronomical Society (01-07-2021)“…ABSTRACT We use the Gemini NIFS instrument to map the H$_2\, 2.1218\, \mu$m and Brγ flux distributions in the inner 0.04–2 kpc of a sample of 36 nearby active…”
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REVERBERATION MAPPING RESULTS FOR FIVE SEYFERT 1 GALAXIES
Published in The Astrophysical journal (10-08-2012)“…We present the results from a detailed analysis of photometric and spectrophotometric data on five Seyfert 1 galaxies observed as a part of a recent…”
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Space Telescope and Optical Reverberation Mapping Project. X. Understanding the Absorption-line Holiday in NGC 5548
Published in The Astrophysical journal (01-06-2019)“…The Space Telescope and Optical Reverberation Mapping Project (AGN STORM) on NGC 5548 in 2014 is one of the most intensive multiwavelength AGN monitoring…”
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The Cepheid Distance to the Narrow-line Seyfert 1 Galaxy NGC 4051
Published in The Astrophysical journal (01-05-2021)“…Abstract We derive a distance of D = 16.6 ± 0.3 Mpc ( μ = 31.10 ± 0.04 mag) to the archetypal narrow-line Seyfert 1 galaxy NGC 4051 based on Cepheid…”
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Space Telescope and Optical Reverberation Mapping Project. XIII. An Atlas of UV and X-Ray Spectroscopic Signatures of the Disk Wind in NGC 5548
Published in The Astrophysical journal (01-01-2021)“…Abstract The unusual behavior of the spectral lines of NGC5548 during the STORM campaign demonstrated a missing piece in the structure of AGNs. For a two-month…”
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