J/AJ/90/1437        Active Extragalactic Objects III  (Coleman+ 1985)

Complete samples of active extragalactic objects. III. A 1411 MHz VLA survey. Coleman P.H., Condon J.J., Hazard C. <Astron. J. 90, 1437 (1985)> =1985AJ.....90.1437C 1985AJ.....90.1437C (SIMBAD/NED BibCode)
ADC_Keywords: Radio sources Abstract: Three selected fields were observed with the Very Large Array (VLA) at 1411MHz as part of an ongoing project to compile complete samples of active extragalactic objects. The radio-source list for the field "A" centered on alpha=08h54m, delta=+17d30' is presented. 67 maps cover the area 3x3deg so that every point lies within at least one primary half-power beamwidth. The median map noise is 0.5mJy and the 6σ completeness level is less than 6mJy over half the field. The synthesized point-source response is an elliptical Gaussian approximately 20x17" between half-intensity points. The areal density of sources with flux densities in the range 5<S<150mJy was determined. Optical identifications based on position coincidences with 90 objects brighter than B≃21.5 in the A and B survey fields are reported. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 81 208 List of radio sources table4.dat 45 97 Optical identifications -------------------------------------------------------------------------------- See also: J/AJ/87/739 : Active Extragalactic Objects I. (Condon+ 1982) J/AJ/87/1429 : Active Extragalactic Objects II (Condon+ 1982) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Source name 12- 13 I2 h RAh Right Ascension 1950 (hours) 14- 15 I2 min RAm Right Ascension 1950 (minutes) 16- 20 F5.2 s RAs Right Ascension 1950 (seconds) 22- 24 F3.2 s e_RAs Mean error on RAs 26 A1 --- DE- Declination 1950 (sign) 27- 28 I2 deg DEd Declination 1950 (degrees) 29- 30 I2 arcmin DEm Declination 1950 (minutes) 31- 34 F4.1 arcsec DEs Declination 1950 (seconds) 36- 38 F3.1 arcsec e_DEs Mean error on DEs 40- 44 F5.1 mJy S1411MHz Integrated Flux Density 46- 49 F4.1 mJy e_S1411MHz Mean error on S1411MHz 51- 52 I2 arcsec MajAxis ? Half-intensity major axis 54- 55 I2 arcsec MinAxis ? Half-intensity minor axis 57- 59 I3 deg PA ? MajAxis position angle 61- 64 F4.2 --- f Integrated attenuation factor 66- 69 F4.2 --- fp Peak attenuation factor 71- 75 F5.1 mJy mapSp Map Peak flux density 77- 81 A5 --- Map Map designation (parameters in table1 of paper) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Source name, as in tabl2 14- 15 A2 --- IDdir *[GS?: ] Identification by direct observation 19- 22 A4 --- IDop *[GS?:QO ] Identification by objective prism 24- 27 F4.1 mag Bmag ? Blue magnitude determined by the APM 28 A1 --- u_Bmag Uncertainty flag (:) on Bmag 30- 34 F5.2 s dRA Offset in Right Ascension 36- 40 F5.1 arcsec dDE Offset in Declination 42- 45 F4.1 --- m *Normalized position difference -------------------------------------------------------------------------------- Note on IDdir, IDop: the symbols are G = Galaxy ; S = star-like object ; QSO = quasar ? = object of unknown nature Note on m: difference between optical and radio positions divided by the errors in each; see Mitchell et al. (1981PASP...93..647M 1981PASP...93..647M) for details on m definitions and statistics. -------------------------------------------------------------------------------- Acknowledgements: We thank Heinz Andernach who scanned and proofread the tables (numbered R196 in his archive)
(End) Francois Ochsenbein [CDS] 13-Feb-1997
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line