/ftp/cats/aliases/M//MWSC_5_



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J/A+A/585/A101  Milky Way global survey of star clusters. V. (Kharchenko+, 2016)
The following files can be converted to FITS (extension .fit or fit.gz)
	catalog.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/585/A101
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drwxr-xr-x 39 cats archive 4096 Mar 3 2017 [Up] drwxr-xr-x 3 cats archive 252 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 470 Dec 19 2022 .message -r--r--r-- 1 cats archive 4613 Dec 23 2015 ReadMe -rw-r--r-- 1 cats archive 1000 Dec 23 2015 +footg5.gif -rw-r--r-- 1 cats archive 8981 Dec 23 2015 +footg8.gif -r--r--r-- 1 cats archive 349890 Jun 21 2015 catalog.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/585/A101 Milky Way global survey of star clusters. V. (Kharchenko+, 2016) ================================================================================ Global survey of star clusters in the Milky Way. V. Integrated JHKs parameters of 3208 Galactic star clusters. Kharchenko N.V., Piskunov A.E., Schilbach E., Roeser S., Scholz R.-D. <Astron. Astrophys. 585, A101 (2016)> =2016A&A...585A.101K (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Clusters, open ; Photometry, UBV ; Photometry, infrared Keywords: Galaxy: evolution - Galaxy: open clusters and associations: general - solar neighbourhood - Galaxy: stellar content Abstract: We determined the integrated magnitudes of 3208 star clusters in the 2MASS near-infrared (JHKs) passbands. Description: The catalogue presents integrated parameters in near-infrared (JHKs) passbands for 3208 Galactic star clusters. The integrated magnitudes are based on the most probable cluster members selected from the high-precision, homogeneous all-sky catalogue 2MAst that is constructed on the basis of catalogues PPMXL (Roeser et al., 2010, Cat. I/317) and 2MASS (Cutri et al., 2003, Cat. II/246). The integrated magnitudes are computed by adding the individual luminosities of the most secure cluster members. In order to put the computed magnitudes into a uniform and unbiased system they were corrected for the effect of unseen stars in the 2MAst. The clusters in the catalogue are sorted according to their numbers in the MWSC.