/ftp/cats/aliases/K/KUG_3_



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VII/262 Comprehensive Catalogue of Kiso UV-X Galaxies (KUG2000) (Nakajima+ 2010)
The following files can be converted to FITS (extension .fit or fit.gz)
	catalog.dat
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Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=VII/262
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drwxr-xr-x 236 cats archive 4096 Apr 2 17:03 [Up] drwxr-xr-x 2 cats archive 4096 Dec 15 09:33 [TAR file] -rw-r--r-- 1 cats archive 461 Sep 25 2010 .message -r--r--r-- 1 cats archive 6869 Sep 25 2010 ReadMe -rw-r--r-- 1 cats archive 1348 Sep 25 2010 +footg5.gif -rw-r--r-- 1 cats archive 9784 Sep 25 2010 +footg8.gif -r--r--r-- 1 cats rsyncuser 861996 Sep 21 2010 catalog.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 212501 Sep 23 2010 notes.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats rsyncuser 52158 Aug 30 2010 notes.txt.gz [Uncompressed]
Beginning of ReadMe : VII/262 Comprehensive Catalogue of Kiso UV-X Galaxies (KUG2000) (Nakajima+ 2010) ================================================================================ Comprehensive Catalogue of Kiso Ultraviolet-Excess Galaxies Miyauchi-Isobe N., Maehara H., Nakajima K. <Publ. Natl. Astron. Obs. Japan, 13, 9 (2010)> =2010PNAOJ..13....9M ================================================================================ ADC_Keywords: Galaxies, UV-excess; Surveys Keywords: Ultraviolet-excess galaxies - Survey with Schmidt telescope - KUG Description: The referenced paper describes the compilation of the second Kiso UV-Excess galaxies survey as KUG2 catalogue. The result is shown in VII/261. The first survey catalogue KUG1 is shown in VII/179. As is described in the paper, there are some differences between KUG1 and KUG2, e.g. in photographic plates used and the observation condition in the surveys, such as emulsions, exposures or seeing sizes. The homogeneity of these KUG surveys is rather low, but their catalogues form a somewhat large collection of UV-excess/blue galaxies. In these circumstances, we intend to merge both catalogues, upon requests from investigators working in follow-up observations of these galaxies. In the process of catalogue merging, we met a systematic difference between the first (KUG1) and the second (KUG2) surveys in overall properties of objects, such as brightness, degree of UV-excess and morphological type. This mainly originates from differences in the observation condition and personal errors in the survey. We scrutinize and discuss those differences and errors, and finally merge into a comprehensive catalogue of KUGs (KUG2000) in the machine-readable form including near ten thousand UV-excess galaxies.

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