==========================================================================
J/A+A/430/471 UBV(RI)C photometry of Stock 16 (Vazquez+, 2005)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
table2.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/430/471
==========================================================================
drwxr-xr-x 25 cats archive 4096 Jan 29 2012 [Up]
drwxr-xr-x 2 cats archive 260 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 468 Dec 19 2022 .message
-r--r--r-- 1 cats archive 4852 Jul 19 2005 ReadMe
-rw-r--r-- 1 cats archive 1013 Sep 19 2007 +footg5.gif
-rw-r--r-- 1 cats archive 2932 Mar 5 2008 +footg8.gif Beginning of ReadMe :J/A+A/430/471 UBV(RI)c photometry of Stock 16 (Vazquez+, 2005)
================================================================================
Revisiting the area of the open cluster Stock 16.
Vazquez R.A., Baume G.L., Feinstein C., Nunez J.A., Vergne M.M.
<Astron. Astrophys., 430, 471-480 (2005)>
=2005A&A...430..471V
================================================================================
ADC_Keywords: Clusters, open ; Photometry, UBVRI ; Photometry, Cousins
Keywords: Galaxy: open clusters and associations: individual: WR 50 -
stars: luminosity function, mass function -
Galaxy: open clusters and associations: individual: WR 51 -
stars: imaging
Abstract:
Deep CCD UBV(RI)c photometry has been carried out in the area of the
open cluster Stock 16. The different photometric diagrams indicate the
presence of three superimposed stellar groups, all composed of early
type stars.
Description:
CCD UBV(RI)c imaging photometry was carried out in the field of Stock
16 along two observational runs at the University of Toronto Southern
Observatory, Las Campanas, Chile, using the Hellen Sawyer Hogg 60-cm
telescope: on the nights of 1994 April 13, 14 and 16, we obtained
UBVRI photometry for four frames with the nitrogen-cooled detector PM
METHACROME UV coated (0.45"/pix) covering 4' on a side; three more
frames were exposed on the nights of 1996 February 25 and 26 in the
UBV(I)c bands (this time, the detector was glycol-refrigerated).