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Rest‐Frame Ultraviolet‐to‐Optical Properties of Galaxies at z ≈ 6 and z ≈ 5 in the Hubble Ultra Deep Field: From Hubble to Spitzer

  • Authors: Haojing Yan, Mark Dickinson, Daniel Stern, Peter R. M. Eisenhardt, Ranga-Ram Chary, Mauro Giavalisco, Henry C. Ferguson, Stefano Casertano, Christopher J. Conselice, Casey Papovich, William T. Reach, Norman Grogin, Leonidas A. Moustakas, and Masami Ouchi

Yan et al. 2005 The Astrophysical Journal 634 109.

  • Provider: AAS Journals

Caption: Fig. 6.

Observed SEDs of the ﹩z\approx 5﹩ objects that have no NICMOS photometry, with their best‐fit models overplotted. The symbols are the same as in Fig. 5.

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