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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. 1.

Image stamps of the IRAC‐detected ﹩z\approx 6﹩ objects. The ACS z850‐band "stamps" in the left panels are ﹩1\farcs 5\times 1\farcs 5﹩ in size and show the morphological details of these objects. The images in the other three columns of panels (﹩12^{\prime \prime }\times 12^{\prime \prime }﹩ in size) show the matching of these sources from ACS z850 to IRAC 3.6 μm. NICMOS J110 stamps are also shown when available. The IDs of these objects are taken from Yan & Windhorst (2004b). Object 1ab has a spectroscopically measured redshift ﹩z=5.83﹩.

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