Colors and magnitudes predicted for high redshift galaxies

Details Colors and magnitudes predicted for high redshift galaxies Colors and magnitudes predicted for high redshift galaxies

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apjs...43..393c&link_type=abstract

Astrophysical Journal Supplement Series, vol. 43, July 1980, p. 393-416. Research sponsored by the Koninklijke Nederlandse Akad

Astronomy and Astrophysics

Astronomy

1111

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

Scientific paper

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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