Search Results - "Peterson, B. M."
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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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Spatially resolved rotation of the broad-line region of a quasar at sub-parsec scale
Published in Nature (London) (01-11-2018)“…The broadening of atomic emission lines by high-velocity motion of gas near accreting supermassive black holes is an observational hallmark of quasars 1 …”
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Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei
Published in The Astrophysical journal (01-02-2017)“…Broad (∼10,000 km s−1), double-peaked emission-line profiles of Balmer lines emitted by active galactic nuclei (AGN) are thought to originate in the outer…”
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APPLICATION OF STOCHASTIC MODELING TO ANALYSIS OF PHOTOMETRIC REVERBERATION MAPPING DATA
Published in The Astrophysical journal (10-03-2016)“…ABSTRACT We use both simulated and real quasar light curves to explore modeling photometric reverberation-mapping (RM) data as a stochastic process. We do this…”
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The First Swift Intensive AGN Accretion Disk Reverberation Mapping Survey
Published in The Astrophysical journal (10-01-2019)“…Swift intensive accretion disk reverberation mapping of four AGN yielded light curves sampled ∼200-350 times in 0.3-10 keV X-ray and six UV/optical bands…”
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Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei. II. A Homogeneous Analysis of a Large Reverberation-Mapping Database
Published in The Astrophysical journal (01-10-2004)“…We present improved black hole masses for 35 active galactic nuclei (AGNs) based on a complete and consistent reanalysis of broad emission-line…”
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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 Changing-look Quasar Mrk 590 Is Awakening
Published in The Astrophysical journal (20-10-2018)“…Mrk 590 was originally classified as a Seyfert 1 galaxy, but then it underwent dramatic changes: the nuclear luminosity dropped by over two orders of magnitude…”
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MUSE observations of a changing-look AGN – I. The reappearance of the broad emission lines
Published in Monthly notices of the Royal Astronomical Society (11-06-2019)“…ABSTRACT Optical changing-look Active Galactic Nuclei (AGN) are a class of sources that change type within a short time-scale of years or decades. This change…”
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A fast and long-lived outflow from the supermassive black hole in NGC 5548
Published in Science (American Association for the Advancement of Science) (04-07-2014)“…Supermassive black holes in the nuclei of active galaxies expel large amounts of matter through powerful winds of ionized gas. The archetypal active galaxy NGC…”
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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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Intensive Broadband Reverberation Mapping of Fairall 9 with 1.8 yr of Daily Swift Monitoring
Published in The Astrophysical journal (01-10-2024)“…Abstract We present 1.8 yr of near-daily Swift monitoring of the bright, strongly variable Type 1 active galactic nucleus (AGN) Fairall 9. Totaling 575…”
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Parsec-scale radio morphology and variability of a changing-look AGN: the case of Mrk 590
Published in Monthly notices of the Royal Astronomical Society (21-07-2016)“…We investigate the origin of the parsec-scale radio emission from the changing-look active galactic nucleus (AGN) of Mrk 590, and examine whether the radio…”
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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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Spectropolarimetry of NGC 3783 and Mrk 509: Evidence for powerful nuclear winds in Seyfert 1 Galaxies
Published in Monthly notices of the Royal Astronomical Society (01-10-2021)“…ABSTRACT We present results from high signal-to-noise optical spectropolarimetric observations of the Seyfert 1 galaxies NGC 3783 and Mrk 509 in the 3500–7000…”
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C IV LINE-WIDTH ANOMALIES: THE PERILS OF LOW SIGNAL-TO-NOISE SPECTRA
Published in The Astrophysical journal (20-09-2013)“…Comparison of six high-redshift quasar spectra obtained with the Large Binocular Telescope with previous observations from the Sloan Digital Sky Survey shows…”
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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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Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei. I. Comparing the Photoionization and Reverberation Techniques
Published in The Astrophysical journal (01-12-1999)Get full text
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The Radius-Luminosity Relationship for Active Galactic Nuclei: The Effect of Host-Galaxy Starlight on Luminosity Measurements
Published in The Astrophysical journal (10-06-2006)“…We have obtained high-resolution images of the central regions of 14 reverberation-mapped active galactic nuclei (AGNs) using the Hubble Space Telescope…”
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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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