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 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:
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FileName Lrecl Records Explanations
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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
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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
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Bytes Format Units Label Explanations
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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")
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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