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K‐Corrections and Filter Transformations in the Ultraviolet, Optical, and Near‐Infrared

  • Authors: Michael R. Blanton and Sam Roweis

Blanton & Roweis 2007 The Astronomical Journal 133 734.

  • Provider: AAS Journals

Caption: Fig. 17.

Our galaxy stellar mass estimates, ﹩M_{*}﹩, compared to those of Kauffmann et al. (2003), ﹩M_{s,*}﹩, as a function of stellar mass (top) and of color (bottom). The gray scale is the conditional distribution ﹩M_{s,*}/ M_{*}﹩ on each quantity. The lines are the 10%, 25%, 50%, 75%, and 90% quantiles.

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