J/AJ/87/739         Active extragalactic objects I. (Condon+ 1982)

Complete samples of active extragalactic objects. I. A 1411-MHz VLA survey centered on alpha= 12h04min, delta= +11deg30min Condon J.J., Condon M.A., Hazard C. <Astron. J. 87, 739 (1982)> =1982AJ.....87..739C 1982AJ.....87..739C (SIMBAD/NED BibCode)
ADC_Keywords: Radio sources Abstract: As one part of a program to detect complete samples of active extragalactic objects, the 3.36x10-3sr field centered on alpha=12h04min, delta=+11deg30' (1950.0) was mapped with the Very Large Array at 1411MHz. Sixty-seven maps cover this field so that no point is more than 15arcmin from the nearest map center. The median map noise is 0.6mJy, and the 6sigma completeness limit is less than 6mJy over half of the survey field. The synthesized point-source response is an elliptical Gaussian 22x18arcsec between half-intensity points. The rms source-position uncertainties are ∼1arcsec in each coordinate so that reliable optical identifications can be made on the basis of radio-optical position coincidence alone. The sky density of sources with flux densities 5≤S<150mJy and the angular-size distribution of sources between 30 and 150mJy were determined. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1 52 67 Map parameters table2 91 178 Source list -------------------------------------------------------------------------------- See also: J/AJ/87/1429 : Active Extragalactic Objects II (Condon+ 1982) J/AJ/90/1437 : Active Extragalactic Objects III (Coleman+ 1985) Byte-by-byte Description of file: table1 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Map Map designation 8- 9 I2 h RAh Right ascension (B1950) 11- 12 I2 min RAm Right ascension (B1950) 14- 15 I2 s RAs Right ascension (B1950) 17 A1 --- DE- Declination sign 18- 19 I2 deg DEd Declination (B1950) 21- 22 I2 arcmin DEm Declination (B1950) 26- 29 F4.1 arcsec MajAxis Gaussian equivalent half-intensity major axis of the restoring beam 30 A1 --- --- [x] 31- 34 F4.1 arcsec MinAxis Gaussian equivalent half-intensity minor axis of the restoring beam 37- 41 F5.1 deg PA Major-axis position angle 44- 47 F4.2 mJy rms rms map noise 49- 52 F4.1 mJy mapSp Map peak flux density limit -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Source name 12- 13 I2 h RAh Right ascension (B1950) 15- 16 I2 min RAm Right ascension (B1950) 18- 22 F5.2 s RAs Right ascension (B1950) 25- 28 F4.2 s e_RAs rms uncertainty on right ascension 31- 32 I2 deg DEd Declination (B1950) 34- 35 I2 arcmin DEm Declination (B1950) 37- 40 F4.1 arcsec DEs Declination (B1950) 43- 45 F3.1 arcsec e_DEs rms uncertainty on declination 47- 51 F5.1 mJy S1411 Integrated flux density 53- 56 F4.1 mJy e_S1411 rms uncertainty on S1411 58- 59 I2 arcsec MajAxis ? Gaussian equivalent half-intensity axis (1) 60 A1 --- --- [x] 61- 62 I2 arcsec MinAxis ? Gaussian equivalent half-intensity axis (1) 64- 66 I3 deg PA ? Major-axis position angle 69- 72 F4.2 --- f Integrated attenuation factor 75- 78 F4.2 --- fp Peak attenuation factor 80- 84 F5.1 mJy mapSp Map peak flux density 87- 91 A5 --- Map Map designation -------------------------------------------------------------------------------- Note (1): the values are deconvolved for the telescope beam and beam smearing -------------------------------------------------------------------------------- Acknowledgements: We thank Heinz Andernach who communicated in February 1997 the errors he had detected in the scanned version of the tables. History: Prepared via OCR at CDS.
(End) James Marcout, Patricia Bauer [CDS] 14-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