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.
Papers
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Journal ArticleDOI
A Near-Infrared and Optical Study of X-Ray Selected Seyfert Galaxies. II. Models and Interpretation
C. W. McAlary,George H. Rieke +1 more
TL;DR: In this article, a modele base sur la Courbe de croissance de la loi de Hubble, modifie par une relation couleur-type morphologique-ouverture, is constructed for decomposer l'emission nucleaire d'origine stellaire and non stellaires d'un echantillon de 16 galaxies de Seyfert de type I.
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Black Hole Accretion in Low-Mass Galaxies since z ~ 1
Yong Shi,George H. Rieke,Jennifer L. Donley,Michael C. Cooper,Christopher N. A. Willmer,Evan N. Kirby +5 more
TL;DR: In this article, a sample of X-ray-emitting active galactic nuclei (AGNs) in low-mass host galaxies was selected and compared to AGNs in more massive hosts, and it was found that the AGN spatial number density and the fraction of galaxies hosting AGNs depends strongly on the host mass.
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Spitzer observations of a 24 micron shadow: Bok Globule CB190
Amelia M. Stutz,John H. Bieging,George H. Rieke,Yancy L. Shirley,Zoltan Balog,Karl D. Gordon,Elizabeth M. Green,Jocelyn Keene,Brandon C. Kelly,Mark Rubin,Michael W. Werner +10 more
TL;DR: In this paper, a roughly circular 24 micron shadow with a 70 arcsec radius was observed and the extinction profile of this shadow matched the profile derived from 2MASS photometry at the outer edges of the globule and reaches a maximum of ~32 visual magnitudes at the center.
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Infrared Measurements of Uranus and Neptune
George H. Rieke,Frank J. Low +1 more
TL;DR: New measurements verify that Neptune is brighter than Uranus near 20 microns and show that both planets have increasing brightness temperature with decreasing wavelength between 34 and 22.5 microns as discussed by the authors.
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Spectral energy distributions of type 2 quasi-stellar objects: obscured star formation at high redshifts
D. Rigopoulou,Vincenzo Mainieri,Omar Almaini,A. Alonso-Herrero,J.-S. Huang,Günther Hasinger,George H. Rieke,J. Dunlop,Ingo Lehmann +8 more
TL;DR: In this paper, the authors presented new mid-infrared and submillimetre observations for a sample of eight high-redshift type 2 quasi-stellar objects (QSOs) located in the Chandra Deep Field-South.