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VIII/24  6C Survey of Radio Sources - V.                  (Hales+ 1993)

The 6C Survey of Radio Sources - V. The zones 6C-Va (48<Dec<68, 01h34<RA<06h14) and 6C-Vb (48<Dec<68, 17h16<RA<20h24) Hales S.E.G., Masson C.R., Warner P.J., Baldwin J.E., Green D.A. <Mon. Not. R. Astron. Soc. 262, 1057 (1993)> =1993MNRAS.262.1057H
ADC_Keywords: Radio sources ; Surveys Abstract: The 6th Cambridge Survey of radio sources covers most of the sky north of 30° with an angular resolution of 4.2x4.2cosecδ arcmin2 and a limiting flux density of 160mJy at 151MHz, with completeness achieved at 600mJy. This paper presents, in the declination ranges 48°<δ<68{dec} the zones Va (01h34<α<06h14) and Vb (17h16<α<20h24) Description: See the documentation by N. A. Oliversen, either in LaTeX (doc.tex), or in plain ascii (adc.doc) File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file adc.doc 76 216 Documentation by N. A. Oliversen adc.sty 78 68 LaTeX Style file doc.tex 76 199 LaTeX Documentation by N. A. Oliversen 6c5a.dat 47 2229 48<Dec<68, 01h34<RA<06h14 6c5b.dat 47 1229 48<Dec<68, 17h16<RA<20h24
See also: VIII/18 : I. (Dec>80) VIII/21 : II. (30<Dec<51 , 09h30<RA<17h30) VIII/22 : III. (48<Dec<68 , 05h25<RA<18h17) VIII/23 : IV. (67<Dec<82) Byte-by-byte Description of file: 6c5a.dat, 6c5b.dat
Bytes Format Units Label Explanations
1- 2 I2 h RAh Right Ascension B1950 (hours) 4- 5 I2 min RAm Right Ascension B1950 (minutes) 7- 10 F4.1 s RAs Right Ascension B1950 (seconds) 12 A1 --- DE- Declination B1950 (sign) 13- 14 I2 deg DEd Declination B1950 (degrees) 16- 17 I2 arcmin DEm Declination B1950 (minutes) 19- 20 I2 arcsec DEs Declination B1950 (seconds) 23- 27 F5.2 Jy F151p [0.19/79] Flux density (peak) 30- 34 F5.2 Jy F151i [0.46/79]? Flux density (integrated) 35 A1 --- n_F151i [*-] Reason for missing F151i (1) 37- 39 I3 --- Map [1/36] Contour map panel number 41- 47 A7 --- Field Contour map field name ("0300+58", "0500+58", or 1900+58")
Note (1): Meaning of the symbols: - (dash) = the peak was not strong enough to calculate the integrated flux * (asterisk) = the peak flux was strong enough to qualify for integration, but it has been integrated into a brighter adjoining peak.

(End) Francois Ochsenbein [CDS] 25-Nov-1993
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

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