/ftp/cats/8/32



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VIII/32            Extragalactic sources at 5GHz             (Jenkins+ 1977)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat notes.dat table2.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VIII/32
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drwxr-xr-x 112 cats archive 4096 Nov 7 15:27 [Up] drwxr-xr-x 2 cats archive 324 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 482 Dec 19 2022 .message -r--r--r-- 1 cats archive 8069 Jan 15 2004 ReadMe -rw-r--r-- 1 cats archive 563 Sep 24 2012 +footg5.gif -rw-r--r-- 1 cats archive 3860 Sep 24 2012 +footg8.gif -r--r--r-- 1 cats archive 7109 Jan 15 2004 notes.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 26265 Jan 15 2004 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3563 Dec 5 2003 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : VIII/32 Extragalactic sources at 5GHz (Jenkins+ 1977) ================================================================================ Observations of 104 extragalactic radio sources with the Cambridge 5-km telescope at 5 GHz. Jenkins C.J., Pooley G.G., Riley J.M. <Mem. R. Astron. Soc., 84, 61 (1977)> =1977MmRAS..84...61J ================================================================================ ADC_Keywords: Radio sources Abstract: One hundred and four radio sources from the 3C and 4C catalogues have been mapped with a resolution of 2arcsec in RA and 2cosecdeltaarcsec in DE. The results are presented here as contour maps and in tabular form, with accurate measurements of the positions of optical objects in the fields. Description: A complete sample of 3CR sources has now been observed with the 5-km telescope at 5GHz. The sample was selected according to the following criteria: (a) The flux density of each individual source at 178MHz is greater than or equal to 10Jy according to the compilation given by Kellermann et al. (1969ApJ...157....1K). (b) DE>10deg. (c) |b|>10deg. There are 166 sources in this sample of which one, 3C 326, was not observed as it was originally thought to be galactic. Since it now seems likely to be extragalactic we have included it in the sample. The sample is listed in Table 2.