G
George H. Rieke
Researcher at Steward Health Care System
Publications - 904
Citations - 79885
George H. Rieke is an academic researcher from Steward Health Care System. The author has contributed to research in topics: Galaxy & Luminous infrared galaxy. The author has an hindex of 128, co-authored 870 publications receiving 75262 citations. Previous affiliations of George H. Rieke include University of Arizona & Planetary Science Institute.
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Search for IR Emission from Intracluster Dust in A2029
TL;DR: In this paper, the authors search for IR emission from the intracluster dust (ICD) in the galaxy cluster A2029 and obtain upper limits for the extended ICD emission at both 24 and 70 micron.
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Ice in Comet Bowell
TL;DR: In this article, it was shown that only H2O ice is a plausible identification at the heliocentric distance of Comet Bowell during the observations (3.4 AU) since only H 2O grains are stable enough to have produced the observed absorption.
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The spatial extent of the 3.3 micron emission feature in the Seyfert galaxy NGC 7469
TL;DR: In this paper, the 3.3-micron emission line region is extended, with a significant fraction of the luminosity of the line originating at distances greater than 240 pc from the nucleus.
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Spitzer Spectroscopy of Infrared-Luminous Galaxies: Diagnostics of AGN and Star Formation and Contribution to Total Infrared Luminosity
Heath V. Shipley,Casey Papovich,George H. Rieke,Arjun Dey,Buell T. Jannuzi,John Moustakas,Benjamin J. Weiner +6 more
TL;DR: In this article, the authors used Spitzer IRS spectroscopy to study the nature 65 IR-luminous galaxies at 0.02 1.2mJy and found that in both the IRAGN and non-IRAGN samples, the PAH luminosities correlate strongly with the [Ne II] emission.
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The Far-infrared Emission of the First Massive Galaxies
TL;DR: In this article, the authors modeled the resulting far-infrared spectral energy distributions (SEDs), demonstrating that they are shifted substantially to bluer (warmer) wavelengths relative to the best fitting ones at z ~ 3, and with strong outputs in the 10 - 40 micron range.