Image Details
Caption: Fig. 1.
Spectral flux distribution. A fit of the data points with an extincted simple power law and a Lyα break returns two peaks of probability. The main one, covering a probability of 63%, is centered at ﹩z=4.6﹩ with a rest‐frame extinction of ﹩A_{V}=0.5\pm 0.2﹩ (top), and the secondary, covering a probability of 35%, is centered at ﹩z=1.7﹩ with ﹩A_{V}=1.1\pm 0.2﹩ (bottom).
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.