arXiv · astro-ph/0003360
Galaxy Morphologies in the Cluster CL1358+62 at z=0.33
Abstract
We describe the morphological composition of a sample of 518 galaxies in the field of CL1358+62 at z=0.33, drawn from a large HST mosaic covering 53 sq. arcmin. The sample is complete to I=22, corresponding to M_V=-18.5 in the rest frame. The galaxies have been independently classified by the authors of this paper and by Alan Dressler. For galaxies with I<21, the two sets of classifiers agree on the total early-type population, but disagree on the S0/E ratio. We discuss the constraints on morphological evolution and the implication of the differing S0/E ratios. We use our large body of spectra to make the correspondence between morphological and spectral type.
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D. Fabricant, M. Franx, P. van Dokkum. 2000-03-23. Galaxy Morphologies in the Cluster CL1358+62 at z=0.33. https://doi.org/10.1086/309269
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