/ftp/cats/A+A/445/819



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J/A+A/445/819       Systems of galaxies in Shapley supercluster (Ragone+, 2006)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat table2.dat
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Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/445/819
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drwxr-xr-x 21 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:56 [TAR file] -rw-r--r-- 1 cats archive 479 Jan 11 2007 .message -r--r--r-- 1 cats archive 4177 Jan 11 2007 ReadMe -rw-r--r-- 1 cats archive 338 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2404 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 5490 Nov 14 2006 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3744 Nov 14 2006 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/445/819 Systems of galaxies in Shapley supercluster (Ragone+, 2006) ================================================================================ Identification and study of systems of galaxies in the Shapley supercluster. Ragone C.J., Muriel H., Proust D., Reisenegger A., Quintana H. <Astron. Astrophys., 445, 819-825 (2006)> =2006A&A...445..819R ================================================================================ ADC_Keywords: Clusters, galaxy ; Radial velocities ; Velocity dispersion Keywords: galaxies: clusters: general Abstract: Based on the largest compilation of galaxies with redshift in the region of the Shapley Supercluster (Proust et al., 2004 in prep., 2006A&A...447..133P), we identified 122 galaxy systems, 60 of which are new systems. Using the SuperCOSMOS catalogue, we have assigned b_j_ magnitudes to each galaxy in our compilation. The sample of galaxy systems was used to estimate the mass function of systems in the range 10^13^ to 10^15^M_sun/h^-1^. We computed a lower value to the total mass in the region of the Shapley Supercluster with this mass function. Using 15 mock catalogues we derived the mean mass that these kinds of systems have before comparing it with that obtained from the real data.

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