/ftp/cats/aliases/K/./KMR2006



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J/AJ/131/407      BV photometry of stars in the LMC             (Kaluzny+, 2006)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat table2.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/AJ/131/407
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drwxr-xr-x 82 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 298 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 481 Dec 19 2022 .message -r--r--r-- 1 cats archive 5412 Apr 18 2007 ReadMe -rw-r--r-- 1 cats archive 1012 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2932 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 101809 Nov 2 2006 table1.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 590 Mar 28 2007 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/AJ/131/407 BV photometry of stars in the LMC (Kaluzny+, 2006) ================================================================================ Variable stars in the Large Magellanic Cloud: discovery of extragalactic W UMa binaries. Kaluzny J., Mochnacki S., Rucinski S.M. <Astron. J., 131, 407-413 (2006)> =2006AJ....131..407K ================================================================================ ADC_Keywords: Magellanic Clouds ; Stars, variable ; Photometry, UBV Keywords: binaries: general - galaxies: individual (Large Magellanic Cloud) - galaxies: star clusters - Magellanic Clouds - techniques: photometric Abstract: We observed a field in the disk of the LMC on two consecutive nights in search of rapid variable stars. We found two pulsating stars of type RRab and Scuti and four binary stars; among the latter we found one sdB or cataclysmic variable below the LMC blue main sequence and three very close binary systems on the main sequence. Description: We used the Magellan/Baade 6.5m telescope with the TEK5 CCD 2Kx2K camera, which had a focal scale of 0.069"/pixel. The observations were made on two nights, 2002 January 4/5 and 5/6. We conducted 6.2hr of variability monitoring on the first night and 7.3hr on the second night. The nights can be characterized as gray time, with fractions of the illuminated area of the Moon disk of 61% and 50%, respectively.