VIII/22 6C Survey of Radio Sources - III. (Hales+ 1990)
The 6C survey of radio sources - III. The zone 48<Dec<68, 05h25<RA<18h17
Hales S.E.G., Masson C.R., Warner P.J., Baldwin J.E.
<Mon. Not. R. Astron. Soc. 246, 256 (1990)>
=1990MNRAS.246..256H 1990MNRAS.246..256H
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 8749 sources in the 1950deg2
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:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
adc.doc 80 225 Documentation by N. A. Oliversen
adc.sty 78 68 Required to process doc.tex
doc.tex 73 200 LaTeX Documentation by N. A. Oliversen
6c3.dat 47 8749 The Catalogue (48<Dec<68 , 05h25<RA<18h17)
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See also:
VIII/18 : I. (Dec>80)
VIII/21 : II. (30<Dec<51 , 09h30<RA<17h30)
VIII/23 : IV. (67<Dec<82)
VIII/24 : V. (48<Dec<68 , 01h34<RA<06h14 , 17h16<RA<20h24)
Byte-by-byte Description of file: 6c3.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 [0.16/91] Flux density (peak)
30- 34 F5.2 Jy F151i [0.3/90]? Flux density (integrated)
35 A1 --- n_F151i [-*] Reason for missing F151i (1)
37- 39 I3 --- Map [1/32] Contour map panel number
40 A1 --- --- [:] The character ":"
41- 47 A7 --- Field Contour map field name ("0700+58", "0900+58",
"1100+58", "1300+58", "1500+58" or "1700+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] 24-Nov-1993