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
The quantum efficiency and diffractive image artifacts of Si:As IBC mid-IR detector arrays at 5 $-$ 10 $\mu$m: Implications for the JWST/MIRI detectors.
Andras Gaspar,George H. Rieke,Pierre Guillard,Daniel Dicken,Stacey Alberts,Jane E. Morrison,Michael E. Ressler,Ioannis Argyriou,Alistair Glasse +8 more
TL;DR: In this article, the authors analyzed the parameters leading to high quantum efficiency for the MIRI devices between 5 and 10 µm, and also modeled the cross-shaped artifact that was first noticed in the 5.7 and 7.8 µm Spitzer/IRAC images and has since also been imaged at shorter wavelengths.
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Completing the Census of AGN in GOODS-S/HUDF: New Ultra-Deep Radio Imaging and Predictions for JWST.
TL;DR: In this article, the authors identify AGN within faint radio populations at cosmic noon selected from new ultra-deep, high resolution imaging from the Karl G. Jansky Very Large Array at 6 and 3 GHz.
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Protoplanetary and transitional disks in the open stellar cluster ic 2395
Zoltan Balog,Nick Siegler,George H. Rieke,László L. Kiss,James Muzerolle,Robert A. Gutermuth,Cameron P. M. Bell,Jozsef Vinko,Kate Y. L. Su,Erick T. Young,Andras Gaspar +10 more
TL;DR: In this article, the Lendulet Young Researchers Program of the Hungarian Academy of Sciences (Lendulet-Young Researchers Program) was used to train a team of Hungarian researchers.
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The Dusty Heart of NGC 4151 Revealed by λ ∼ 1-40 μm Reverberation Mapping and Variability: A Challenge to Current Clumpy Torus Models
Jianwei Lyu,George H. Rieke +1 more
TL;DR: In this article, the authors investigated the dusty environment of the archetypical type-1 AGN in NGC 4151 with comprehensive IR reverberation mapping over several decades, in J ($\sim1.22~\mu$m), H ($βγγγδδγγ), L ($ βγγ-γγβδαγγαγ), K ($γγ βγ-βγβαγ)-γγ-, L ($γβγ-3.19~γγ, L$3.45~γ
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Debris disks in main sequence binary systems
David Trilling,John Stansberry,Karl R. Stapelfeldt,George H. Rieke,Kate Y. L. Su,Richard O. Gray,Christopher J. Corbally,Geoffrey Bryden,Christine Chen,Andrew F. Boden,Chas Beichman +10 more
TL;DR: In this article, the authors observed 69 A3-F8 main sequence binary star systems using the Multiband Imaging Photometer for Spitzer onboard the Spitzer Space Telescope and found that approximately half of the excess emissions are derived from circumbinary planetesimal belts.