Detection of faint clusters of galaxies by superimposing digitized Schmidt plates

Details Detection of faint clusters of galaxies by superimposing digitized Schmidt plates Detection of faint clusters of galaxies by superimposing digitized Schmidt plates

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992daec.conf..219a&link_type=abstract

In Distribution of Matter in the Universe, 2nd DAEC mtg, ed. G.A. Mamon and D. Gerbal (Meudon: Obs. de Paris) p. 219-220

Physics

Scientific paper

We have modeled giant luminous arcs (Fig. 1) found by Lavery and Henry
(1988) in the cluster Abell 963 (Fig. 2). There is, at least, three
times more lensing mass associated to the cluster than to the galaxies.
The source is probably a very faint galaxy (L <= 0.1 L*) which may be
a small spiral at z=0.77.

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