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VIII/23  6C Survey of radio sources - IV.               (Hales+ 1991)

The 6C survey of radio sources - IV. The zone 67<Dec<82, 0h<RA<24h Hales S.E.G., Mayer C.J., Warner P.J., Baldwin J.E. <Mon. Not. R. Astron. Soc. 251, 46 (1991)> =1991MNRAS.251...46H
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 zone covers the declinations 67°--82° region 48°<δ<68°, 05h25m<α<18h17m. 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 6c4.dat 49 5421 The Catalogue (67<Dec<82) adc.doc 75 239 Documentation by N. A. Oliversen doc.tex 73 193 LaTeX documentation by N. A. Oliversen
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/24 : V. (48<Dec<68 , 01h34<RA<06h14 , 17h16<RA<20h24) Byte-by-byte Description of file: 6c4.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 [0.16/42] Flux density (peak) 30- 34 F5.2 Jy F151i [0.4/54]? Flux density (integrated) 35 A1 --- n_F151i [*-] Reason for missing F151i (1) 38- 39 I2 --- Map [1/32] Contour map panel number 41 A1 --- --- [:] The character ":" 43- 49 A7 --- Field Contour map field name ("0100+75", "0400+75", "0700+75", "1000+75", "1300+75", "1600+75", "1900+75" or "2200+75")
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] 24-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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