Image Details
Caption: Fig. 3.
Example galaxy spectra for two of the brighter galaxies in the survey. The drop‐off in flux of galaxy 1081 at ﹩\lambda \approx 6770﹩ Å is due to the CCD edge. Also, the feature at ﹩\lambda \approx 3820﹩ Å is due to a series of bad columns on the CCD. The gray line traces the 1 σ error array.
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.