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William T. Reach
Researcher at Universities Space Research Association
Publications - 545
Citations - 95523
William T. Reach is an academic researcher from Universities Space Research Association. The author has contributed to research in topics: Galaxy & Interstellar medium. The author has an hindex of 131, co-authored 535 publications receiving 90496 citations. Previous affiliations of William T. Reach include California Institute of Technology & Space Telescope Science Institute.
Papers
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Journal ArticleDOI
DR 21: A Major Star Formation Site Revealed by Spitzer
A. P. Marston,William T. Reach,Alberto Noriega-Crespo,Jeonghee Rho,Howard A. Smith,Gary J. Melnick,Giovanni G. Fazio,George H. Rieke,Sean Carey,Luisa Rebull,James Muzerolle,Eiichi Egami,Dan M. Watson,Judy Pipher,William B. Latter,Karl R. Stapelfeldt +15 more
TL;DR: In this paper, the authors obtained images of the obscured massive star-forming region DR 21 using both the IRAC and Multiband Imaging Photometer for Spitzer (MIPS) instruments aboard the Spitzer Space Telescope.
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The mid-infrared spectrum of the zodiacal and exozodiacal light
TL;DR: In this paper, the authors observed the zodiacal light spectrum with the mid-infrared camera ISOCAM over the wavelength range 5-16 μm and a wide range of orientations relative to the Sun (solar elongations 68°-113°).
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Dust processing in Supernova Remnants: Spitzer MIPS SED and IRS Observations
TL;DR: In this paper, the authors present Spitzer MIPS SED and IRS observations of 14 Galactic supernova Remnants previously identified in the GLIMPSE survey and find evidence for SNR/molecular cloud interaction through detection of [OI] emission, ionic lines, and emission from molecular hydrogen.
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Survey of cometary CO2, CO, and particulate emissions using the Spitzer Space Telescope: Smog check for comets
TL;DR: In this article, the authors surveyed 23 comets using the Infrared Array Camera on the Spitzer Space Telescope in wide filters centered at 3.6 and 4.5 microns.
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Shock Processing of Interstellar Dust and Polycyclic Aromatic Hydrocarbons in the Supernova Remnant N132D
TL;DR: In this paper, the authors observed the oxygen-rich Large Magellanic Cloud (LMC) supernova remnant N132D (SNR 0525-69.6), using all instruments on board the Spitzer Space Telescope, IRS, IRAC, and MIPS (Infrared Spectrograph, Infrared Array Camera, and Multiband Imaging Photometer for Spitzer).