========================================================================== J/A+A/462/811 Superclusters of galaxies from 2dF (Einasto+, 2007) The following files can be converted to FITS (extension .fit .fgz or .fiZ) scl2df* ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/462/811 ==========================================================================
drwxr-xr-x 21 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:59 [TAR file] -rw-r--r-- 1 cats archive 463 Mar 15 2007 .message -r--r--r-- 1 cats archive 6180 Oct 26 2012 ReadMe -rw-r--r-- 1 cats archive 413 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 3602 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 19398 Dec 4 2006 scl2dfna.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 8540 Dec 4 2006 scl2dfnb.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 26840 Dec 4 2006 scl2dfsa.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 11468 Dec 4 2006 scl2dfsb.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/462/811 Superclusters of galaxies from 2dF (Einasto+, 2007) ================================================================================ Superclusters of galaxies from the 2dF redshift survey. I. The catalogue. Einasto J., Einasto M., Tago E., Saar E., Hutsi G., Joeveer M., Liivamagi L.J., Suhhonenko I., Jaaniste J., Heinamaki P., Muller V., Knebe A., Tucker D. <Astron. Astrophys. 462, 811 (2007)> =2007A&A...462..811E ================================================================================ ADC_Keywords: Clusters, galaxy ; Morphology Keywords: cosmology: large-scale structure of the Universe - galaxies: clusters: general Abstract: We use the 2dF Galaxy Redshift Survey data to compile catalogues of superclusters for the Northern and Southern regions of the 2dFGRS, altogether 543 superclusters at redshifts 0.009<z<0.2. We apply the density field method using smoothing with an Epanechnikov kernel of radius 8Mpc. We derive positions of the highest luminosity density peaks and find the most luminous cluster in the vicinity of the peak, this cluster is considered as the main cluster and its brightest galaxy the main galaxy of the supercluster. In catalogues we give equatorial coordinates and distances of superclusters as determined by positions of their main clusters. We also calculate the expected total luminosities of the superclusters. Description: Tables contain data on superclusters, selected from the 2dFGRS survey. Catalogues consist of four lists, two for each Galaxy hemisphere, the main lists A for superclusters up to distance 520Mpc/h, and supplementary lists B for more distant systems. The lists are ordered according to increasing RA, a common id-numeration for lists A and B. Distance and sizes are given in Mpc/h, luminosities in Solar units L_sun_/h^2, where h is the Hubble constant in units of 100km/s/Mpc
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