S
Stephen S. Murray
Researcher at Johns Hopkins University
Publications - 67
Citations - 6234
Stephen S. Murray is an academic researcher from Johns Hopkins University. The author has contributed to research in topics: Galaxy & Luminosity. The author has an hindex of 33, co-authored 67 publications receiving 5959 citations. Previous affiliations of Stephen S. Murray include Harvard University & Smithsonian Astrophysical Observatory.
Papers
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Journal ArticleDOI
Mid-Infrared Selection of Active Galaxies
Daniel Stern,Peter R. Eisenhardt,Varoujan Gorjian,Christopher Kochanek,Nelson Caldwell,Daniel J. Eisenstein,Mark Brodwin,Michael J. I. Brown,R. Cool,Arjun Dey,Paul J. Green,Buell T. Jannuzi,Stephen S. Murray,Michael A. Pahre,Steven P. Willner +14 more
TL;DR: In this article, the Spitzer Space Telescope mid-infrared colors, derived from the IRAC Shallow Survey, of nearly 10,000 spectroscopically identified sources from the AGN and Galaxy Evolution Survey, were used to identify active galaxies.
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Chandra Cluster Cosmology Project. II. Samples and X-Ray Data Reduction
Alexey Vikhlinin,R. A. Burenin,Harald Ebeling,William R. Forman,Allan Hornstrup,Christine Jones,Andrey V. Kravtsov,Stephen S. Murray,Daisuke Nagai,Hernan Quintana,A. Voevodkin +10 more
TL;DR: In this paper, the evolution of the galaxy cluster mass functions at z 0.05 and z0.5 using high-quality Chandra observations of samples derived from the ROSAT PSPC All-Sky and 400 deg2 surveys is discussed.
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Chandra Temperature Profiles for a Sample of Nearby Relaxed Galaxy Clusters
Alexey Vikhlinin,Maxim Markevitch,Stephen S. Murray,Christine Jones,William R. Forman,L. van Speybroeck +5 more
TL;DR: The authors presented Chandra gas temperature profiles at large radii for a sample of 13 nearby, relaxed galaxy clusters and groups, which includes A133, A262, A383, A478, A907, A1413, A1795, A1991, A2029, A2390, MKW 4, RX J1159+5531, and USGC S152.
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A Moving Cold Front in the Intergalactic Medium of A3667
TL;DR: In this paper, a Chandra observation of the central region of the galaxy cluster A3667 with emphasis on the prominent sharp X-ray brightness edge spanning 0.5 Mpc near the cluster core is presented.
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Chandra High-Resolution Camera observations of the luminous X-ray source in the starburst galaxy M82
Philip Kaaret,Andrea Prestwich,Andreas Zezas,Stephen S. Murray,Dong-Woo Kim,Roy Kilgard,Eric M. Schlegel,Martin Ward +7 more
TL;DR: In this paper, Chandra high-resolution camera observations of the starburst galaxy M82 were used to find a position for the most luminous X-ray source with a 1s radial error of 0.7 arcsec.