The Horologium Supercluster

G. Chincarini, M. Tarenghi, H. Sol, P. Crane, J. Manousoyannaki, Jürgen Materne · Symposium - International Astronomical Union · 1983

We measured redshifts for a random subsample of 286 objects, m (Shapley) ≤ 16.5, drawn from the catalogue of the Horologium region published by Shapley. The distribution of the sample objects on the celestial sphere is shown in Fig. 1, the characteristics of the redshift distribution are represented in Figs. 2 and 3.

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