/ftp/cats/viii/50



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VIII/50      VLA Survey of Rich Clusters of Galaxies   (Slee+ 1996)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat catalog.dat
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drwxr-xr-x 103 cats archive 4096 Sep 6 17:04 [Up] drwxr-xr-x 2 cats archive 4096 Dec 15 2013 [TAR file] -rw-r--r-- 1 cats archive 317 Apr 26 1999 .message -r--r--r-- 1 cats archive 12595 Apr 26 1999 ReadMe -rw-r--r-- 1 cats archive 941 Sep 15 2011 +footg5.gif -rw-r--r-- 1 cats archive 4004 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 23832 May 27 1998 catalog.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 15982 Apr 8 1999 paper1.txt.gz [Uncompressed] -r--r--r-- 1 cats archive 2150 May 27 1998 table1.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : VIII/50 VLA Survey of Rich Clusters of Galaxies (Slee+ 1996) ================================================================================ A VLA survey of rich clusters of galaxies. I. Whole-cluster maps, source list and statistics. Slee O.B., Perley R.A., Siegman B.C. <Aust. J. Phys. 42, 633 (1989)> =1989AuJPh..42..633S A VLA Survey of Rich Clusters of Galaxies II. The Stronger Sources: Maps, Polarisations and Identifications Slee O.B., Roy A., Savage A. <Aust. J. Phys. 47, 145 (1994)> =1994AuJPh..47..145S A VLA Survey of Rich Clusters of Galaxies III. The Weaker Sources: Maps and Identifications Slee O.B., Roy A., Andernach H. <Aust. J. Phys. 49, 977 (1996)> =1996AuJPh..49..977S ================================================================================ ADC_Keywords: Clusters, galaxy ; Radio sources Keywords: galaxies: clusters of - radio continuum: galaxies; surveys - radio sources: optical identification Description: We observed 60 fields towards 57 Abell and one Zwicky cluster of galaxies using the Very Large Array (VLA) with scaled arrays at 1.5 and 4.9 GHz. The source catalogue contains radio and optical parameters for 994 sources up to a lower flux limit of 1.0 mJy at 1.5 GHz and comprises a complete sample above 2.5 mJy. The combined sky area within the half-power circle on the maps is 3.5x10^-3^ sr, and the cluster fields are distributed between +35 deg and -30 deg declination. The source catalogue list positions, angular size, spectral index and optical identification, magnitude and morphology, if available.

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