/ftp/cats/aliases/O/OGLE_27_/.



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J/AcA/59/239    VI light curves of LMC long-period variables  (Soszynski+, 2009)
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=J/AcA/59/239
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drwxr-xr-x 11 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Dec 15 09:35 [TAR file] -rw-r--r-- 1 cats archive 466 Apr 7 2010 .message -r--r--r-- 1 cats archive 6681 May 22 2012 ReadMe -rw-r--r-- 1 cats archive 1019 Apr 7 2010 +footg5.gif -rw-r--r-- 1 cats archive 3207 Apr 7 2010 +footg8.gif -r--r--r-- 1 cats archive 3635005 Jan 28 2010 catalog.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/AcA/59/239 VI light curves of LMC long-period variables (Soszynski+, 2009) ================================================================================ The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. IV. Long-period variables in the Large Magellanic Cloud. Soszynski I., Udalski A., Szymanski M.K., Kubiak M., Pietrzynski G., Wyrzykowski L., Szewczyk O., Ulaczyk K., Poleski R. <Acta Astron., 59, 239-253 (2009)> =2009AcA....59..239S ================================================================================ ADC_Keywords: Magellanic Clouds ; Stars, variable ; Magnitudes Keywords: stars: AGB and post-AGB - stars: late-type - stars: oscillations - Magellanic Clouds Abstract: The fourth part of the OGLE-III Catalog of Variable Stars presents 91 995 long-period variables (LPVs) in the Large Magellanic Cloud (LMC). This sample consists of 79200 OGLE Small Amplitude Red Giants (OSARGs), 11128 semiregular variables (SRVs) and 1667 Mira stars. The catalog data include basic photometric and astrometric properties of these stars, long-term multi-epoch VI photometry and finding charts. Description: We describe the methods used for the identification and classification of LPVs. The distribution of I-band amplitudes for carbon-rich stars shows two maxima, corresponding to Miras and SRVs. Such a distinction between Miras and SRVs is not obvious for oxygen-rich stars. We notice additional period-luminosity sequence located between Wood's sequences C and C' and populated by SRVs.

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