========================================================================== VIII/35 Radio Sources observed with Culgoora Circular Array (Slee 1995) The following files can be converted to FITS (extension .fit .fit.Z .fgz) catalog ========================================================================== Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VIII/35 ==========================================================================
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Beginning of ReadMe : VIII/35 Radio Sources observed with Culgoora Circular Array (Slee 1995) ================================================================================ Radio Sources Observed with the Culgoora Circular Array (CCA) at 80 and 160 MHz Slee O.B. <Australian J. Phys., 48, 143-186 (1995)> =1995AuJPh..48..143S ================================================================================ ADC_Keywords: Radio sources Description: This is a final, updated and recalibrated list of sources that were observed with the Culgoora Circular Array (CCA) in the interval 1970-1984. The list contains all the sources that were published in the Culgoora-1,2,3 Lists plus additional sources resulting from a survey of 353 Abell clusters of galaxies. The observations were made at 80 MHz and 160 MHz with HPBW in RA of 3.70' and 1.85' respectively. The beamwidth in Dec is wider by sec(30.3 + Dec). This list brings together all CCA measurements of flux density, position, spectral index and angular size, with limiting flux densities of 4 Jy at 80 MHz and 2 Jy at 160 MHz. References to the original Culgoora publications are given for each source. The sources were selected for CCA observations from the Parkes, 4C and Ohio catalogues if an extrapolation of the then existing spectral data indicated that the 80 MHz flux density would be > 5 Jy. In addition, about 300 additional sources were added from lists of special classes of objects such as those discovered at higher frequencies from surveys of the galactic plane, lists of pulsars and supernova remnants, from a list of nearby bright galaxies and finally from a CCA survey of 353 Abell clusters of galaxies. An area of 16'x16' was surveyed about the centres of 3500 fields, resulting in a total survey area of about 0.1 sr at 80 MHz. Nomenclature Note: Sources from this catalogue are designated "Cul HHMM+DDd" in the literature. Note that the original Cul 1,2,3 lists have only HHMM+DD as a name, but the present names should be preferred.