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Uncovering the Near IR Dwarf Galaxy Population of the Coma Cluster with Spitzer IRAC

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Figure

Fig. 1.—DSS1 image of the Coma Cluster showing the location of the two Spitzer IRAC fields (solid boxes)
Fig. 2.—The 3.6 m Spitzer IRAC mosaic of the core (Coma 1, 0.733 deg 2 ) and off-center (Coma 3, 0.555 deg 2 ) regions of the Coma Cluster
Fig. 4.—IRAC color-color diagram of the confirmed Coma members detected in all four bands in both fields, defined in terms of the logarithms of flux  den-sities in the 5.8/3.6 and 8.0/4.5 m bands
Fig. 5.—Stellar concentration parameter, as defined by Fazio et al. (2004b) and Eisenhardt et al
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