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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 17.

Empirical mass-to-light relation, ( M / L ), derived from WISE 3.4 μm in-band luminosity ( W1 − W2 color (left panel), W2 − W3 color (right panel)) and K s -derived stellar masses using the Zhu et al. (2010) relation (see also Figure 18). The color error bars represent the formal uncertainties (Table 2) and a 1.5% photometric calibration uncertainty. The linear trend (dashed line) is described by Equations (9) and (10). The dotted line (left panel) represents the ( M / L ) derived for nearby galaxies in the GAMA survey (see the text for details).

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