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On the Redshift Evolution of Mg II Absoprtion Systems

  • Authors: Jeremy L. Tinker and Hsiao-Wen Chen

TINKER & CHEN 2010 The Astrophysical Journal 709 1.

  • Provider: AAS Journals

Caption: Figure 1.

Redshift evolution of absorber counts. Points with error bars represent the measurements of Prochter et al. (2006a) broken into three bins of equivalent width. The dashed and dotted curves represent the radius and mass evolution models, respectively, described in Section 2. The solid curves represent the combined model, discussed in Section 5. The thick gray line in panel (a) shows its evolution of dark matter halo counts for M h >10 11 h −1M multiplied by a factor of 0.01 for comparison to the data.

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