Redshift survey in Per-Psc and Pav-Ind (di Nella+ 1996)

Details Redshift survey in Per-Psc and Pav-Ind (di Nella+ 1996) Redshift survey in Per-Psc and Pav-Ind (di Nella+ 1996)

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..72830367d&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/283/367. Originally published in: 1996MNRAS.283..367D

Physics

Galaxies: Optical, Redshifts

Scientific paper

The list of the measured galaxies is given in Table 3 together with COSMOS coordinates and apparent magnitude. These parameters (plus diameter, axis ratio and position angle) were used to perform cross-identification with the PGC/LEDA objects after reduction to the RC3 system (de Vaucouleurs et al., 1990, see cat. ). Both cross correlation results (from `rvsao') and emission line results (from `emsao') are presented. A few galaxies with published redshifts were also observed to derive our external error (see section 3 of the paper). (1 data file).

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