Richard Mushotzky

Professor

University of Maryland

United States

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About

Richard Mushotzky is a Professor at the University of Maryland, United States. His research focuses on active galactic nuclei, X-ray astrophysics, and the processes regulating emissions in cosmic structures, as evidenced by his recent publications. Notable contributions include the analysis of the Fe Kα line in Centaurus A and investigations into the characteristics and emissions of highly luminous, obscured AGNs.

Articles (24)

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2020

Collaborators (13)

CHIN-SHIN CHANG

University of Geneva

SWITZERLAND

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Claudia Cicone

Associate Professor

University of Oslo

NORWAY

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Stuart Vogel

Professor

University of Maryland at College Park

UNITED STATES

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Takuma Izumi

助教/Assistant Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

JAPAN

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Shunsuke Baba

Specially Appointed Assistant Professor

Institute of Space Sciences

JAPAN

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Makoto Tashiro

Specially appointed Professor

Japan Aerospace Exploration Agency

JAPAN

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Mark Gurwell

Smithsonian Institution

UNITED STATES

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Jae-Young Kim

Assistant Professor

Kyungpook National University

SOUTH KOREA

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Krista Smith

Associate Professor

Texas A&M University

UNITED STATES

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Amelie Saintonge

University College London

UNITED KINGDOM

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Meg Urry

Israel Munson Professor of Physics and Astronomy

Yale University

UNITED STATES

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Amy Lien

Assistant Professor

University of Tampa

UNITED STATES

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Masatoshi Imanishi

助教/Assistant Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

JAPAN

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Richard Mushotzky

Research Interests

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About

Articles (24)

XRISM analysis of the complex Fe Kα line in Centaurus A

Erratum: “Superluminal Proper Motion in the X-Ray Jet of Centaurus A” (2024, ApJ, 974, 307)

BASS. LIII. The Eddington Ratio as the Primary Regulator of the Fraction of X-Ray Emission in Active Galactic Nuclei

BASS. XLIX. Characterization of Highly Luminous and Obscured AGNs: Local X-Ray and [Ne V]λ3426 Emission in Comparison with the High-redshift Universe

Cold Gas and Star Formation in the Phoenix Cluster with JWST

The 157 Month Swift/BAT All-sky Hard X-Ray Survey

BASS. XLVIII. [Ne V] λ3427 Emission in Powerful Nearby Active Galactic Nuclei

XRISM Reveals a Remnant Torus in the Low-luminosity AGN M81*

BASS. XLV. Quantifying Active Galactic Nuclei Selection Effects in the Chandra COSMOS-legacy Survey with BASS

BASS. XLVII. 22 GHz Radio Atlas of Swift-BAT Selected AGN

Redshifted Iron Emission and Absorption Lines in the Chandra X-Ray Spectrum of Centaurus A

A Tight Correlation between Millimeter and X-Ray Emission in Accreting Massive Black Holes from <100 mas Resolution ALMA Observations

BASS. XXXIV. A Catalog of the Nuclear Millimeter-wave Continuum Emission Properties of AGNs Constrained on Scales ≤ 100–200 pc

BASS. XLII. The Relation between the Covering Factor of Dusty Gas and the Eddington Ratio in Nearby Active Galactic Nuclei

BASS. XXXV. The M BH–σ* Relation of 105 Month Swift-BAT Type 1 AGNs

Hard X-Ray Emission in Centaurus A

BASS XXXII: Studying the Nuclear Millimeter-wave Continuum Emission of AGNs with ALMA at Scales ≲100–200 pc

BASS. XXI. The Data Release 2 Overview

BASS. XXIV. The BASS DR2 Spectroscopic Line Measurements and AGN Demographics

BASS. XXVI. DR2 Host Galaxy Stellar Velocity Dispersions

BAT AGN Spectroscopic Survey. XX. Molecular Gas in Nearby Hard-X-Ray-selected AGN Galaxies

Forward Modeling Populations of Flares from Tidal Disruptions of Stars by Supermassive Black Holes

Significant Suppression of Star Formation in Radio-quiet AGN Host Galaxies with Kiloparsec-scale Radio Structures

A Hard Look at Local, Optically Selected, Obscured Seyfert Galaxies

Collaborators (13)

CHIN-SHIN CHANG

Claudia Cicone

Stuart Vogel

Takuma Izumi

Shunsuke Baba

Makoto Tashiro

Mark Gurwell

Jae-Young Kim

Krista Smith

Amelie Saintonge

Meg Urry

Amy Lien

Masatoshi Imanishi

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