/ftp/cats/aliases/K/./KHM31_3_



==========================================================================
J/PASP/125/636      Newly identified star clusters in M 31   (Krienke+, 2013)
The following files can be converted to FITS (extension .fit or fit.gz)
	table2.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/PASP/125/636
==========================================================================

drwxr-xr-x 9 cats archive 168 Feb 11 2015 [Up] drwxr-xr-x 4 cats archive 289 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 466 Dec 19 2022 .message -r--r--r-- 1 cats archive 3141 Mar 3 2015 ReadMe -rw-r--r-- 1 cats archive 607 Mar 3 2015 +footg5.gif -rw-r--r-- 1 cats archive 2223 Mar 3 2015 +footg8.gif -r--r--r-- 1 cats archive 5047 Jan 5 2015 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/PASP/125/636 Newly identified star clusters in M 31 (Krienke+, 2013) ================================================================================ Additional newly identified star clusters in M 31. Krienke K.O., Hodge P.W. <Publ. Astron. Soc. Pac., 125, 636-638 (2013)> =2013PASP..125..636K ================================================================================ ADC_Keywords: Galaxies, nearby ; Associations, stellar ; Photometry, HST Keywords: star clusters and associations Abstract: Using the HST archives, we have searched portions of the southern half and northwest quarter of the Andromeda Galaxy (M 31, NGC 224) for previously unrecognized star clusters. The result is a table of the characteristics of 71 newly identified star clusters. Most are moderately faint, low-mass clusters. Absolute magnitudes range from M(V)=-6.3 to -2.5. Description: Cluster photometry was carried out using a program written in IDL (Krienke & Hodge, 2007PASP..119....7K, Cat. J/PASP/119/7). Magnitudes were derived in the HST photometric system and transformed to the UBV system using the methods of Holtzman et al. (1995PASP..107.1065H) and Sirianni et al. (2005PASP..117.1049S).