/ftp/cats/J/A%252bA/420/173



==========================================================================
J/A+A/420/173       JK photometry of Omega Cen red giants    (Sollima+, 2004)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table2.dat
==========================================================================
Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/420/173
==========================================================================

drwxr-xr-x 19 cats archive 4096 Jun 26 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:58 [TAR file] -rw-r--r-- 1 cats archive 466 Jun 26 2004 .message -r--r--r-- 1 cats archive 3071 Jun 26 2004 ReadMe -rw-r--r-- 1 cats archive 1013 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2947 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 1307063 Mar 5 2004 table2.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/420/173 JK photometry of Omega Cen red giants (Sollima+, 2004) ================================================================================ IR photometric properties of red giants in omega Cen. Sollima A., Ferraro F.R., Origlia L., Pancino E., Bellazzini M. <Astron. Astrophys. 420, 173 (2004)> =2004A&A...420..173S ================================================================================ ADC_Keywords: Clusters, open ; Stars, giant ; Photometry, infrared Keywords: globular cluster: individual: Omega Cen - stars: Population II - stars: evolution - techniques: photometry - infrared: stars Description: The IR catalogue of omega Cen is based on ground-based observations using SOFI (Infrared Spectrograph and Imaging Camera on the NTT telescope at ESO, La Silla) and contains about 73000 stars covering an area of 13"x13" around the center of the cluster. The limiting magnitude is K<=17.5m and the positional accuracy is better than 0.2"

© UDS/CNRS

Contact