Distant clusters of galaxies. I - Uniform photometry of 14 rich clusters

Astronomy and Astrophysics – Astrophysics

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Astronomical Photometry, Galactic Clusters, Calibrating, Colorimetry, Luminosity, Magnitude, Prisms, Red Shift, Space Density

Scientific paper

The photographic photometry of 14 clusters of galaxies in the redshift range from 0.18 to 0.39 is presented. Extreme care was taken to ensure that the observations were based on one photometric system using the limits of deep, prime-focus plates obtained with the Anglo-Australian and Cerro Tololo 4 m telescopes. It is found that the sub-beam prisms used in the observation appear to be achromatic and provide photometry which is linear over a range of at least 4.0 mag. The zero-point error in the observations was about + or - 0.04 in both magnitude and color, and the measurement error was equal to about 0.08 mag (BJ - RF), with 0.10 near the bright limit of 18.0 mag, and 0.18 at the faint limit of 22.0 mag. A series of tables is given which provides the number of density profiles, color magnitude arrays, and luminosity functions for each cluster.

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