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Galaxy Growth by Merging in the Nearby Universe

  • Authors: Tao Jiang, David W. Hogg, and Michael R. Blanton

Jiang, Hogg, & Blanton 2012 The Astrophysical Journal 759 140.

  • Provider: AAS Journals

Caption: Figure 24.

Comparison of our f 7.1–28.6  h 70 −1 kpc pair at 0.03 < z < 0.15 with the f 7.1–28.6  h 70 −1 kpc pair of three recent results (Patton & Atfield 2008; Kitzbichler & White 2008; Bundy et al. 2009) at 0.4 < z < 0.7. The open diamonds on the thick solid lines are the results of Bundy et al. (2009), and the open triangles on the thick dashed lines are our results. The thin horizontal solid lines show the results of Patton & Atfield (2008), and the thin horizontal dashed lines show the results of Kitzbichler & White (2008). Please note that the f 7.1–28.6  h 70 −1 kpc pairs of Patton & Atfield (2008) and Kitzbichler & White (2008) are calculated by f pair = R mg × T mg/ C mg.

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