Photometric Redshift Clickable Map
Click on any galaxy in the image to bring up its data, together with
thumbnail BVI and JHK images, the (unabsorbed) best-fit model
spectrum compared to the observed fluxes and the redshift Likelihood Function.
The observed wavelengths corresponding to the rest-frame Lyman-alpha and
Lyman-Limit are marked with dashed vertical lines in the high-redshift
objects.
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Alberto Fernández-Soto
Department of Physics and Astronomy
State University of New York at Stony Brook
Stony Brook, NY-11794-3800, USA
fsoto@sbastr.ess.sunysb.edu