/ftp/cats/J_ApJS/176/414



==========================================================================
J/ApJS/176/414           Galaxy clusters in the SDSS-DR5           (Yoon+, 2008)
The following files can be converted to FITS (extension .fit or fit.gz)
	table1.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/ApJS/176/414
==========================================================================

drwxr-xr-x 14 cats archive 241 Feb 22 2012 [Up] drwxr-xr-x 2 cats archive 244 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 469 Dec 19 2022 .message -r--r--r-- 1 cats archive 4165 Dec 2 2009 ReadMe -rw-r--r-- 1 cats archive 651 Dec 2 2009 +footg5.gif -rw-r--r-- 1 cats archive 5655 Dec 2 2009 +footg8.gif -r--r--r-- 1 cats archive 84630 Jul 6 2009 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/ApJS/176/414 Galaxy clusters in the SDSS-DR5 (Yoon+, 2008) ================================================================================ A spectrophotometric search for galaxy clusters in SDSS. Yoon J.H., Schawinski K., Sheen Y.-K., Ree C.H., Yi S.K. <Astrophys. J. Suppl. Ser., 176, 414-423 (2008)> =2008ApJS..176..414Y ================================================================================ ADC_Keywords: Clusters, galaxy ; Spectrophotometry Keywords: catalogs - galaxies: clusters: general - galaxies: general - surveys Abstract: Recent large-scale galaxy spectroscopic surveys, such as the Sloan Digital Sky Survey (SDSS), enable us to execute a systematic, relatively unbiased search for galaxy clusters. Such surveys make it possible to measure the 3D distribution of galaxies but are hampered by the incompleteness problem due to fiber collisions. In this study we aim to develop a density-measuring technique that alleviates the problem and derives densities more accurately by adding additional cluster member galaxies that follow optical color-magnitude relations for the given redshift. The new density measured with both spectroscopic and photometric data shows a good agreement with apparent information on cluster images and is supported by follow-up observations. By adopting this new method, a total of 924 robust galaxy clusters are found from the SDSS DR5 database in the redshift range 0.05<z<0.1, of which 212 are new. Local maximum-density galaxies successfully represent cluster centers. We provide the cluster catalog including a number of cluster parameters.