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 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:
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FileName Lrecl Records Explanations
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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
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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/24 : V. (48<Dec<68 , 01h34<RA<06h14 , 17h16<RA<20h24)
Byte-per-byte Description of file: 6c4.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 [0.16/42] 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")
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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