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Paper: Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy’s Evolution (SAGE)
Volume: 381, The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution
Page: 115
Authors: Meixner, M.; the SAGE Team
Abstract: We are performing a uniform and unbiased imaging survey of the Large Magellanic Cloud (LMC, ∼7°× 7°), using the IRAC (3.6, 4.5, 5.8 and 8 μm) and MIPS (24, 70, and 160 μm) instruments on board the Spitzer Space Telescope (SST). Our SST survey of the LMC is surveying the agents of a galaxy’s evolution (SAGE), the ISM and stars. In this paper, we present an overview of the project and some initial results from the N79/N83 region.
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