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THE STRIPE 82 MASSIVE GALAXY PROJECT. I. CATALOG CONSTRUCTION

  • Authors: Kevin Bundy, Alexie Leauthaud, Shun Saito, Adam Bolton, Yen-Ting Lin, Claudia Maraston, Robert C. Nichol, Donald P. Schneider, Daniel Thomas, and David A. Wake

2015 The Astrophysical Journal Supplement Series 221 15.

  • Provider: AAS Journals

Caption: Figure 14.

Comparison of public BOSS M* estimates from Maraston et al. (2013) and Chen et al. (2012) to those presented here (and labeled “near-IR”). Every panel plots the difference in ﹩\mathrm{log}{M}_{*}﹩ against near-IR M* in the left column, and against redshift in the right column. The 3σ-clipped averages (light gray circles) and 1σ standard deviation (gold lines) of the difference distributions are over-plotted. Shaded contours with levels separated by 0.3 dex increases in data density are displayed. The comparison is restricted to ﹩\mathrm{log}{M}_{*}/{M}_{\odot }\gt 11.2﹩ for the right-hand panels. Overall normalization differences at the 0.1 dex level are expected. Of greater importance are possible systematic trends that may confuse evolutionary interpretations. Differences in M* estimates display little or no systematic trends with M*, but biases, likely resulting from a number of factors, are more apparent as a function of redshift. See text for discussion.

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