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Cosmology with the Space Schmidt Telescope - Galaxy Colors and Color Distributions

Published online by Cambridge University Press:  12 April 2016

A. Gustavo Bruzual
A. Gustavo Bruzual*
Affiliation:
Centro de Investigaciones de Astronomía (CIDA), A.P. 264, Mérida 5101-A, Venezuela

Abstract

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Galaxy spectral evolutionary models are used to compute the following quantities in optical and UV bandpasses: (a) galaxy color, luminosity, two-color diagrams, and surface brightness profiles as functions of redshifty and (b) galaxy counts, and color and redshift distributions as functions of apparent magnitude. These predictions may be used as a guide to prepare and interpret observing runs with the Space Telescope, the Space Schmidt Telescope, and the Starlab Observatory.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 78: Astronomy with Schmidt-type telescopes , 1984 , pp. 527 - 532
Copyright
Copyright © Reidel 1984

References

Bruzual, A. G. 1981, Ph.D. thesis, University of California, Berkeley.Google Scholar
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Bruzual, A. G., and Kron, R.G. 1980, Ap. J., 241, p. 25.Google Scholar
Koo, D.C. 1981, Ph.D. thesis, University of California, Berkeley.Google Scholar