Multiple object redshift determinations in clusters of galaxies using OCTOPUS

Details Multiple object redshift determinations in clusters of galaxies using OCTOPUS Multiple object redshift determinations in clusters of galaxies using OCTOPUS

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987msngr..47...41m&link_type=abstract

ESO Messenger (ISSN 0722-6691), March 1987, v. 47, p. 41,42.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Galactic Clusters, Red Shift, Spectrum Analysis, Data Reduction, Elliptical Galaxies, Galactic Structure, Radial Velocity, Universe

Scientific paper

The ESO multiobject facility, Octopus, was used to observe a sample of galaxy clusters such as SC2008-565 in an attempt to collect a large set of individual radial velocities. A dispersion of 114 A/mm was used, providing spectral coverage from 3800 to 5180 A. Octopus was found to be a well-adapted instrument for the rapid and simultaneous determination of redshifts in cataloged galaxy clusters.

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