/ftp/cats/VII/256



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VII/256             List of Groups of Galaxies              (Mahtessian++, 2010)
The following files can be converted to FITS (extension .fit or fit.gz)
	table1.dat table2.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VII/256
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drwxr-xr-x 257 cats archive 8192 Feb 8 10:28 [Up] drwxr-xr-x 2 cats archive 4096 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 473 Dec 19 2022 .message -r--r--r-- 1 cats archive 5756 Mar 18 2011 ReadMe -rw-r--r-- 1 cats archive 1562 Sep 24 2012 +footg5.gif -rw-r--r-- 1 cats archive 12186 Sep 24 2012 +footg8.gif -r--r--r-- 1 cats archive 529386 Dec 27 2009 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 137970 Dec 27 2009 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : VII/256 Groups of Galaxies from CfA2 Redshift Survey (Mahtessian++, 2010) ================================================================================ The List of Groups of Galaxies Based on CfA2 Redshift Survey. Mahtessian A.P., Movsessian V.G. <Astrophysics, 53, 70 (2010)> =2010Ap.....53...70M =2010Afz....53...83M ================================================================================ ADC_Keywords: Clusters, galaxy ; Galaxy catalogs ; Magnitudes ; Radial velocities ; Velocity dispersion Description: The catalog contains statistically homogeneous and physically well graunded groups of galaxies based on the CfA2 redshift survey (Cat. J/ApJS/121/287) in the area of space 1000km/s<=cz<=15000km/s, |bII|>=20deg. For identification of groups we used a modification of a friends of friends (FoF) method. Principles of friendship and definition of values of presented there free parameters described in Mahtessian (1988Afz....28..255M, 1997Ap.....40..285M). There are 1971 groups with 2 or more members, for a total of 6787 members (46.3%); 765 of the groups have 3 or more members with 4375 galaxies (28.1%). The others 8790 (56.4%) galaxies make a sample of "single" galaxies. The catalog includes group numbers, numbers of members, equatorial coordinates, Virgo-centric radial velocities, line-of-sight-velocity dispersions, integrated group luminosities, and relative quantity of false members.