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Extending the Nearby Galaxy Heritage with WISE: First Results from the WISE Enhanced Resolution Galaxy Atlas

  • Authors: T. H. Jarrett, F. Masci, C. W. Tsai, S. Petty, M. E. Cluver, Roberto J. Assef, D. Benford, A. Blain, C. Bridge, E. Donoso, P. Eisenhardt, B. Koribalski, S. Lake, James D. Neill, M. Seibert, K. Sheth, A. Stanford, and N. Wright

Jarrett et al. 2013 The Astronomical Journal 145 6.

  • Provider: AAS Journals

Caption: Figure 10.

WISE W3 comparison with GALEX NUV of M 83 (NGC 5236). The left panel shows a log-stretch of the WISE W3 image, the middle panel shows a log-stretch of the GALEX NUV image, and the right panel is the flux ratio between the two bands. Dark gray-scale values indicate strong NUV, while light values indicate relatively strong W3; e.g., the arrow points to high NUV and low W3. The nucleus is denoted with a × symbol.

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