Apparent magnitudes of high-redshift galaxies in UBVRI and space telescope photometric systems

Details Apparent magnitudes of high-redshift galaxies in UBVRI and space telescope photometric systems Apparent magnitudes of high-redshift galaxies in UBVRI and space telescope photometric systems

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...74..185g&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 74, no. 2, Aug. 1988, p. 185-210.

Astronomy and Astrophysics

Astrophysics

57

Astronomical Photometry, Galactic Evolution, Hubble Space Telescope, Magnitude, Red Shift, Astronomical Models, Color-Magnitude Diagram

Scientific paper

Tables reporting predictions of apparent magnitudes and colors for distant galaxies are computed from a model of spectrophotometric evolution of high-redshift galaxies proposed by Guiderdoni and Rocca-Volmerange (1987). The template synthetic spectra used for these calculations are obtained from standard scenarios of galaxy evolution reproducing the range of observational properties for nearby galaxies of the Hubble sequence. The tables are given with two cosmological models Ho = 50 km/s/Mpc, Omega(0) = 0.1 and 1. The tabulated filters are UBVRI from Johnson's system, U+, J+, F+ N+ from Kron (1980) and Koo (1981), gr from Thuan and Gunn (1976), and some broad-band filters from the Faint Object Camera (FOC) and the Wide Field Camera (WFC) of the Hubble Space Telescope. Tables with the relative contributions of nebular emission and internal extinction are also given.

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