Spectral evolution of galaxies. III - Cosmological predictions for the Space Telescope faint object camera

Mathematics – Logic

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Astronomical Photometry, Faint Object Camera, Galactic Evolution, Hubble Space Telescope, Spectral Energy Distribution, Astronomical Models, Brightness Distribution, Color, Cosmology, Red Shift, Ultraviolet Spectra

Scientific paper

The galactic spectral evolutionary models of Bruzual A. (1981) are employed to estimate parameters which will be observable by the wide-field camera and faint-object camera of the Space Telescope. The capabilities and bandpasses of the instruments are reviewed, and the results are presented in tables and graphs. Parameters calculated include the amplitude of the Lyman discontinuity at 912 A, stellar and galaxy rest-frame colors, color evolution, two-color diagrams as a function of redshift, luminosity evolution, surface brightness profiles, galaxy counts, and color and redshift distributions. In general, it is predicted that the space measurements will follow the trends noted in round-based observations.

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