'Irac' diaporamas de présentation

Galaxies as Sources of Reionization

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Spitzer/IRAC Observations of the Active Merger Remnant NGC 6240

Spitzer/IRAC Observations of the Active Merger Remnant NGC 6240. Stephanie Bush Advisor: Giovanni Fazio Collaborators: Zhong Wang & Margarita Karovska. Why are we interested in nearby Interacting Galaxies?. Galaxy interactions affect a wide range of astrophysical applications:

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Mid-Infrared Observations of Nearby Interacting/Starburst Galaxies

Mid-Infrared Observations of Nearby Interacting/Starburst Galaxies with the Spitzer Space Telescope Zhong Wang For Giovanni Fazio and the IRAC Science Team. Science Goals:

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Spitzer observations of Lyman Break Galaxies

Extreme Starbursts: Near and Far, 14-20 August, Lijiang, China. Spitzer observations of Lyman Break Galaxies. Dimitra Rigopoulou (Oxford,UK) J.-S. Huang, G. Fazio,(CfA, Harvard),& the IRAC team C. Papovich, E. Egami (Arizona, MIPS). The observations

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PAIRITEL Photometry of Dwarfs from the IRAC GTO sample

PAIRITEL Photometry of Dwarfs from the IRAC GTO sample. Joseph L. Hora Brian Patten, Massimo Marengo Harvard-Smithsonian Center for Astrophysics 2 nd Annual PAIRITEL Workshop. IRAC M/L/T Dwarf Program. IRAC bands at 3.6, 4.5, 5.8, and 8 ? m

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Cross-Calibration Between All Three Instruments

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Overview of the Interagency Risk Assessment Consortium

Overview of the Interagency Risk Assessment Consortium. Isabel Walls, Ph.D. National Program Leader, Epidemiology of Food Safety USDA NIFA Chair, IRAC Technical Committee. Overview. Purpose Goals Background Membership Recent accomplishments Current projects. Purpose.

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Lecture 13: Projects

Lecture 13: Projects. October 5, 2011. Spitzer Space Telescope. 0.85 meter infrared telescope Launched in August 2003 Cooled to ~1.5 K Warm (2009-); IRAC 3.6, 4.5 ?m. IRS PI : Houck (Cornell) 4 Spectrographs 5.3-38 ?m Short -hi, short-lo Long -hi, long-lo. MIPS

152 views • 7 slides