Fig. 8 from The Spitzer Survey of the Small Magellanic Cloud: S3MC Imaging and Photometry in the Mid‐ and Far‐Infrared Wave Bands

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The Spitzer Survey of the Small Magellanic Cloud: S³MC Imaging and Photometry in the Mid‐ and Far‐Infrared Wave Bands

Authors: Alberto D. Bolatto, Joshua D. Simon, Snežana Stanimirović, Jacco Th. van Loon, Ronak Y. Shah, Kim Venn, Adam K. Leroy, Karin Sandstrom, James M. Jackson, Frank P. Israel, Aigen Li, Lister Staveley-Smith, Caroline Bot, Francois Boulanger, and Mónica Rubio

Bolatto et al. 2007 The Astrophysical Journal 655 212.

Provider: AAS Journals

Caption: Fig. 8.

Spitzer infrared CMDs of the SMC. The wave band corresponding to the ordinate axis is indicated in each panel. The overlaid gray contours indicate densities of sources, and the assumed distance modulus is ﹩\mathrm{DM}\,=18.93﹩. Only sources detected with S/N greater than 10 in the wave bands used in each CMD are plotted. The right side scale on the last panel indicates apparent magnitude.

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