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Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (SAGE). I. Overview and Initial Results
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 theExpand
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Infrared standard stars
The results of an observational program aimed at setting up a network of faint near-infrared standards of sufficient accuracy are reported. The network covers both northern and southern hemispheresExpand
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M supergiants in the Milky Way and the Magellanic Clouds Colors, spectral types, and luminosities
On presente une nouvelle photometrie BVRI pour 116 candidates supergeantes rouges dans le Petit Nuage de Magellan et 11 supergeantes rouges lumineuses dans le Grand Nuage de Magellan. On presenteExpand
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The asymptotic giant branch of Magellanic cloud clusters
The present search for carbon and M-type asymptotic giant branch (AGB) stars in the 39 clusters of the Magellanic Clouds has yielded identifications and near-IR photometry for about 400 such stars.Expand
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Photometric studies of composite stellar systems. I - CO and JHK observations of E and S0 galaxies
Multiaperture infrared photometric observations of the central regions of 51 early-type galaxies and of the integrated light of five globular clusters are presented. These data are compared withExpand
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M giants in Baade's window: infrared colors, luminosities, and implications for the stellar content of E and S0 galaxies
On presente des observations IR JHKL, [10], CO et H 2 O de 185 geantes M1-9 dans la fenetre de Baade. Les variables de longue periode (VLP) ont des indices et des couleurs IR qui leur donnent desExpand
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The Frequency of Barred Spiral Galaxies in the Near-Infrared*
We have determined the fraction of barred galaxies in the H-band for a statistically well-defined sample of 186 spirals drawn from the Ohio State University Bright Spiral Galaxy Survey. We find 56%Expand
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The Hubble Space Telescope Wide Field Camera 3 Early Release Science Data: Panchromatic Faint Object Counts for 0.2-2 μm Wavelength
We describe the Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) Early Release Science (ERS) observations in the Great Observatories Origins Deep Survey (GOODS) South field. The new WFC3 ERSExpand
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