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Ultraviolet Luminosity Functions from 132 z ∼ 7 and z ∼ 8 Lyman-break Galaxies in the Ultra-deep HUDF09 and Wide-area Early Release Science WFC3/IR Observations

  • Authors: R. J. Bouwens, G. D. Illingworth, P. A. Oesch, I. Labbé, M. Trenti, P. van Dokkum, M. Franx, M. Stiavelli, C. M. Carollo, D. Magee, and V. Gonzalez

Bouwens et al. 2011 The Astrophysical Journal 737 90.

  • Provider: AAS Journals

Caption: Figure 10.

Rest-frame UV LF determinations for galaxies at z ~ 7 (Section 6.1.1). Shown are the UV LF from this paper (red circles and red downward arrow) and from Bouwens et al. (2010c, open red circles), Oesch et al. (2010a, purple circles), Ouchi et al. (2009, black squares), Castellano et al. (2010b, green squares), McLure et al. (2010, blue squares), and Bouwens et al. (2008, black crosses). Constraints from Wilkins et al. (2011) are similar, but are not shown to reduce confusion. See Table 6 for a comparison of the Schechter parameters derived here for the z ~ 7 UV LF with those found in other analyses.

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