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The Changing Lyα Optical Depth in the Range 6 < z < 9 from the MOSFIRE Spectroscopy of Y-dropouts

  • Authors: Tommaso Treu, Kasper B. Schmidt, Michele Trenti, Larry D. Bradley, and Massimo Stiavelli

Treu et al. 2013 The Astrophysical Journal Letters 775 L29.

  • Provider: AAS Journals

Caption: Figure 3.

Inference results in the context of the patchy and smooth models described in the text. The parameter epsilon describes the change of the Lyα equivalent width distribution between z ~ 6 and z ~ 8. In the patchy model, at any given equivalent width, only a fraction epsilon p of the sources that are emitting at z ~ 6 are found to be emitters at z ~ 8. In the smooth model, the emission of each source is suppressed by a factor epsilon s . The evidence ratio Z p /Z s is inconclusive and does not favor any of the two models. The results shown are based on the eight objects in the primary MOSFIRE sample presented here as well as the three spectra analyzed by Treu et al. (2012).

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