Redshift-magnitude bands and the evolution of galaxies. I – New observations

Abstract

Well-defined samples of galaxy redshifts and magnitudes for the Perseus and A1367 clusters are obtained from a combination of new and existing observations. For the Perseus cluster, identifications, 1950 positions, distance from cluster center in degrees, mp and V(6) magnitudes, redshifts corrected for earth orbital and galactic rotation, and comments are provided. Information for the 50 central A1367 galaxies includes identification, mp, redshift and redshift source, morphology, and comments.

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