We have extended the CfA Redshift Survey to low galactic latitudes to investigate the relation between the Great Wall in the North Galactic Cap and the Perseus-Pisces chain in the South Galactic Cap. We present redshifts for 2020 galaxies in the Catalogue of Galaxies and of Clusters of Galaxies (Zwicky et al. 1961-68, CGCG, Cat. ) in the following regions: 4h<=RA<=8h, 17h<=Dec.<=20h, 0deg<=Dec.<=45deg. In these regions, the redshift catalogue includes 1664 galaxies with B(0)15.5; of these, 148 were previously unmeasured. The CGCG samples the galaxy distribution down to b_(II)~10deg. In this paper, we discuss the acquisition and reduction of the spectra, and we examine the qualitative features of the redshift distribution. The Great Wall and the Perseus-Pisces chain are not simply connected across the Zone of Avoidance. These structures, which at first appear to be coherent on scales of ~100h^-1^Mpc or more, actually form the boundaries of neighboring voids of considerably smaller scale, approximately 50h^-1^Mpc. The structures delineated by our optically-selected sample are qualitatively similar to those detected by the far-infrared-selected IRAS 1.2 Jansky Survey (Fisher et al., 1995ApJS..100...69F). Although the IRAS survey probes more deeply into the Zone of Avoidance, our optically-selected survey provides better sampling of structures at b(II)>=10deg. (Copyright) 1996 American Astronomical Society.

Cone search capability for table J/AJ/112/1803/table1 (The Galactic Plane Survey [B(0)=15.5])