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J/other/PASAu/10.310 Parkes-Tidbinbilla radio sources (Duncan+ 1993)
A survey of 526 southern flat-spectrum radio sources with the Parkes-Tidbinbilla interferometer Duncan R.A., White G.L., Wark R., Reynolds J.E., Jauncey D.L., Norris R.P., Taaffe L., Savage A. <Proc. Astron. Soc. Australia, 10, 310 (1993)> =1993PASAu..10..310D (SIMBAD/NED BibCode)
ADC_Keywords: Radio sources ; Interferometry Abstract: We have measured the 2.3GHz total and correlated flux densities on a baseline of 275km of all sources in the Parkes catalogue which : (i) are south of declination +10deg, (ii) have a catalogued 2.7GHz total flux density exceeding 0.5Jy, and (iii) have a 2.7/5.0GHz spectral index flatter than -0.5. More than 14% of the sample showed visibility amplitudes greater than 0.9, and more than 72% showed visibility amplitudes greater than 0.5. Of the sources with optical or other identifications 79% were quasars. In this paper we briefly summarise the results of this survey. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 50 526 Optical attributes and total and correlated flux densities of 526 sources
See also: VIII/15 : Parkes Radio Sources Catalogue (PKSCAT90) (Wright+ 1990) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 8 A8 --- Name Source name (B1950) 10- 12 A3 --- ID Optical identification (1) 14- 17 F4.1 mag mag ? Optical magnitude 20- 24 F5.3 --- z ? Redshift 26- 27 I2 --- o_S2.7GHzc Number of independent observations of S2.7GHzc 29- 34 F6.3 Jy S2.7GHz ? Total flux density at 2.7GHz 37- 42 F6.3 Jy S2.7GHzc ? Correlated flux density at 2.7GHz 45- 50 F6.3 --- Vis ? Visibility (ratio of correlated to total flux densities)
Note (1): Q: Quasar G: Galaxy EF: Empty field Lac: BL Lac object PN: Planetary nebula HII: H II region SNR: Supernova remnant ?: Optically crowded or obscured field
Table 2: 2x2 contingency table of quasar visibility versus redshift -------------------------------------------------------------------------------- redshift Visibility <1.5 ≥1.5 -------------------------------------------------------------------------------- ≥0.5 123 78 <0.5 39 3 Table 3: 2x2 contingency table of quasar visibility versus spectral index -------------------------------------------------------------------------------- spectral index Visibility <0 ≥0 -------------------------------------------------------------------------------- ≥0.5 142 135 <0.5 51 8 History: Prepared via OCR at CDS. * 17-Oct-1997: 3 errors detected by H. Andernach were corrected.
(End) James Marcout, Patricia Bauer [CDS] 22-May-1997
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