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Title:
Colors and magnitudes predicted for high redshift galaxies
Authors:
Coleman, G. D.; Wu, C.-C.; Weedman, D. W.
Affiliation:
AA(Dyer Observatory, Nashville, Tenn.), AB(Computer Sciences Corp., Greenbelt, Md.), AC(Pennsylvania State University, University Park, Pa.)
Publication:
Astrophysical Journal Supplement Series, vol. 43, July 1980, p. 393-416. Research sponsored by the Koninklijke Nederlandse Akademie van Wetenschappen; (ApJS Homepage)
Publication Date:
07/1980
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
Galactic Clusters, Hertzsprung-Russell Diagram, Red Shift, Spectral Energy Distribution, Ultraviolet Astronomy, Ultraviolet Spectra, Astronomical Photometry, Continuous Spectra, Cosmology, Elliptical Galaxies, Spiral Galaxies, Ubv Spectra, Visible Spectrum
DOI:
10.1086/190674
Bibliographic Code:
1980ApJS...43..393C

Abstract

Ultraviolet observations of nearby galaxies with the ANS are used to derive ultraviolet spectra for different galaxy types. These spectra are used with existing visible spectrophotometry to calculate K-corrections, and to predict colors and magnitudes for various galaxy types as a function of redshifts, to z = 2. No evolutionary effects are considered. It appears that the first-ranked cluster galaxies on blue emulsions should be spirals for z greater than or approximately equal to 0.5.

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