========================================================================== J/MNRAS/368/534 Near-infrared study of CIZA J1324.7-5736 (Nagayama+, 2006) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table1.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/MNRAS/368/534 ==========================================================================
drwxr-xr-x 12 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 10:00 [TAR file] -rw-r--r-- 1 cats archive 471 Dec 12 2006 .message -r--r--r-- 1 cats archive 4202 Dec 12 2006 ReadMe -rw-r--r-- 1 cats archive 613 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2175 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 6719 Oct 17 2006 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/MNRAS/368/534 Near-infrared study of CIZA J1324.7-5736 (Nagayama+, 2006) ================================================================================ Near-infrared study of CIZA J1324.7-5736, the second richest cluster of galaxies in the Great Attractor. Nagayama T., Woudt P.A., Wakamatsu K., Nishiyama S., Nagashima C., Kato D., Nagata T., Nakaya H., Sugitani K., Tamura M., Sato S. <Mon. Not. R. Astron. Soc., 368, 534-543 (2006)> =2006MNRAS.368..534N ================================================================================ ADC_Keywords: Clusters, galaxy ; X-ray sources ; Photometry, infrared Keywords: surveys - dust, extinction - galaxies: clusters: general - galaxies: clusters: individual: CIZA J1324.7-5736 - galaxies: fundamental parameters - infrared: galaxies Abstract: We present the result of a deep near-infrared survey of the newly identified X-ray luminous cluster of galaxies CIZA J1324.7-5736 in the Great Attractor (GA) region. In a 35x35arcmin^2^ region, 111 galaxy candidates with r(Ks20)>3arcsec are identified. Description: Our near-infrared survey of an extended region around CIZA1324 was carried out in 2003 April and May, during a total of six nights. The observation was made with the Simultaneous Three-Color Infrared Imager for Unbiased Survey (SIRIUS), a simultaneous imager in the J (1.26um), H (1.63um) and Ks (2.14um) bands, covering an area of 7.7x7.7arcmin^2^ with a pixel scale of 0.45arcsec on the InfraRed Survey Facility (IRSF) 1.4-m telescope at the Sutherland site of the South African Astronomical Observatory.
© UDS/CNRS