========================================================================== J/A+A/487/33 Velocities of Abell 610, 725 and 796 members (Boschin+, 2008) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table[15].dat table4.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/487/33 ==========================================================================
drwxr-xr-x 20 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:57 [TAR file] -rw-r--r-- 1 cats archive 481 Feb 16 2009 .message -r--r--r-- 1 cats archive 5585 Feb 16 2009 ReadMe -rw-r--r-- 1 cats archive 1033 Feb 16 2009 +footg5.gif -rw-r--r-- 1 cats archive 2265 Feb 16 2009 +footg8.gif -r--r--r-- 1 cats archive 8666 Sep 15 2008 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1050 Sep 12 2008 table4.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1937 Sep 15 2008 table5.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/487/33 Velocities of Abell 610, 725 and 796 members (Boschin+, 2008) ================================================================================ Optical analysis of the poor clusters Abell 610, Abell 725, and Abell 796, containing diffuse radio sources. Boschin W., Barrena R., Girardi M., Spolaor M. <Astron. Astrophys., 487, 33-46 (2008)> =2008A&A...487...33B ================================================================================ ADC_Keywords: Clusters, galaxy ; Radial velocities ; Photometry, SDSS Keywords: galaxies: clusters: general - galaxies: clusters: individual: Abell 610, Abell 725, Abell 796 - galaxies: distances and redshifts - cosmology: observations Abstract: We study the dynamical status of the poor, low X-ray luminous galaxy clusters Abell 610, Abell 725, and Abell 796 (at z=0.1, 0.09, and 0.16, respectively), containing diffuse radio sources (relic, relic, and possible halo, respectively). Our analysis is based on new spectroscopic data obtained at the William Herschel Telescope for 158 galaxies, new photometry obtained at the Isaac Newton Telescope with the addition of data recovered from the Data Release 5 of the Sloan Digital Sky Survey. We use statistical tools to select 57, 36, and 26 cluster members and to analyze the kinematics of cluster galaxies, as well as to study the 2D cluster structure. Description: We carried out multi-object spectroscopic observations of A610, A725, and A796 in November 2004 and January 2005. We used AF2/WYFFOS, the multi-object, wide-field, fiber spectrograph working at the prime focus of the 4.2m William Herschel Telescope (WHT, Island of La Palma, Spain).
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