Answers are grounded in this paper and cite their sources.
This is the first in a series of papers discussing the properties of a complete set of radio sources selected near S_408_ = 1 Jy. We present optical or infrared identifications for a sample of 452 radio galaxies. The sources were selected from the 408 MHz Molonglo Reference Catalog, restricted only by flux density and position on the sky, as follows: S_408_ >= 0.95 Jy and -30^deg^ < decl. (1950) <-20^deg^, and 9^h^20^m^ < R.A.(1950) < 14^h^4^m^ or 20^h^20^m^ < R.A.(1950) < 6^h^14^m^. This complete sample, the MRC/1 Jy survey, contains 558 radio galaxies or quasars, of which six are occulted by bright stars or galaxies and two are multiple confused sources. Of the remaining 550 sources, 527, or 96%, are identified to an r magnitude of 25, and eight additional sources are identified to K = 19. Of the 17 unocculted objects that remain unidentified, 15 are sources for which we have either poor radio maps or inadequate optical/IR images. This paper presents finding charts and astrometric positions for the 452 sources that are not identified as either quasars or BL Lacertae objects. Magnitudes in the r passband accurate to typically 0.1 mag are given for 353 of the radio galaxy identifications. Redshifts for 268 of the galaxies are also listed; these have been derived from 450 spectroscopic observations. The radio observations, quasar and BL Lac identifications, spectroscopy, and near- IR images will be presented in subsequent papers in this series.
No takes yet. Share an insight, caveat, or question.
McCarthy et al. (1996) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: