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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. 5.

Best‐fit models to the three ﹩z\approx 5﹩ objects that have NICMOS photometry. Symbols are the same as in Fig. 3. Object 6ab can be well fitted by single‐component models. Object 15ab is problematic because of its abnormally blue ﹩( i_{775}-z_{850}) ﹩ color. If we ignore the i775 band as justified in § 6.2 (see also Fig. 8), reasonably high quality fits can be obtained using single‐component models. Object 48ab, on the other hand, seems to need two‐component models. However, we consider the fit to this object uncertain (see § 6.1 for details).

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