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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First light and reionization : open questions in the post-JWST era
Massimo Stiavelli,John C. Mather,Mark Clampin,René Doyon,Kathy Flanagan,Marijn Franx,Jonathan P. Gardner,Matthew A. Greenhouse,Heidi B. Hammel,J. B. Hutchings,Peter Viggo Jakobsen,Simon J. Lilly,Mark J. McCaughrean,Matt Mountain,George H. Rieke,George Sonneborn,Rogier A. Windhorst,Gillian S. Wright +17 more
TL;DR: Mather et al. as discussed by the authors proposed the Mather-clampin-Clampin (GSFC, chair) and Doyon-Doyon (U.S. of A) as the GSFC chair.
Posted Content
Aromatic Features in M101 HII Regions and Starburst Galaxies
TL;DR: In this article, the behavior of the aromatic features as a function of metallicity/radiation field hardness in M101 HII regions and starburst galaxies is investigated using Spitzer/IRS spectra.
Proceedings ArticleDOI
Row and column artifacts in JWST MIRI’s Si:As blocked impurity band detectors
D. Dicken,George H. Rieke,Michael E. Ressler,Jane E. Morrison,Macarena Garcia Marin,Iaonnis Argyriou,Karl D. Gordon,Michael W. Regan,Christophe Cossou,Andras Gaspar,Alistair Glasse,Pierre Guillard,Alvaro Labiano,Gillian S. Wright +13 more
TL;DR: In this paper , the row-column effect in MIRI detector data has been investigated and it has been shown that rows and columns in which source signals are located can suffer from pull up or pull down in the flux image.
Journal ArticleDOI
Debris Disks in NGC 2547
N. Gorlova,Zoltan Balog,George H. Rieke,James Muzerolle,Kate Y. L. Su,Valentin D. Ivanov,Eric T. Young +6 more
TL;DR: In this paper, a survey of the 30 Myr-old cluster NGC 2547 for planetary debris disks using Spitzer was conducted. And the authors found that the inner 0.1-1 AU parts of disks around solar-type stars clear out very thoroughly by 30 Myrs of age.