Computer Science
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992daec.conf..179c&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. 179-183
Computer Science
Scientific paper
This paper reports on the galaxy distribution obtained from a redshift HI survey in the zone -17.5 deg <= delta <= 0 deg. The galaxy sample substantially complete down to an equivalent Zwicky magnitude m_z=14.5 allows to delineate the main distribution features up to V_r approx 6000 km/s (i.e. D=60 Mpc; a Hubble constant of H_0 = 100 km/s/Mpc is used throughout this paper). The redshift sample described below has been partly measured with the Nancay radiotelescope. The part of this zone located in the Southern galactic hemisphere has already been covered by an optical survey (Pellegrini et al. 1990) which allowed definitively to complete the whole southern galactic sky coverage (CfA plus Southern Sky Redshift Survey). However the second half of our zone located in the Northern galactic hemisphere was unexplored until now. Since this region is adjacent to that covered by the CfA survey at positive declinations, we will be particularly concerned here in large scale structure continuation through the CfA and our survey.
Chamaraux Pierre
Siemieniec G.
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