J/AcA/58/163    VI light curves of LMC classical Cepheids     (Soszynski+, 2008)
The following files can be converted to FITS (extension .fit or fit.gz)
	list.dat catalog.dat remarks.dat
Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/AcA/58/163

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Beginning of ReadMe : J/AcA/58/163 VI light curves of LMC classical Cepheids (Soszynski+, 2008) ================================================================================ The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. I. Classical Cepheids in the Large Magellanic Cloud. Soszynski I., Poleski R., Udalski A., Szymanski M.K., Kubiak M., Pietrzynski G., Wyrzykowski L., Szewczyk O., Ulaczyk K. <Acta Astron. 58, 163 (2008)> =2008AcA....58..163S ================================================================================ ADC_Keywords: Magellanic Clouds ; Stars, variable ; Magnitudes Keywords: Cepheids - stars: oscillations - Magellanic Clouds Abstract: We present the first part of a new catalog of variable stars (OIII-CVS) compiled from the data collected in the course of the third phase of the Optical Gravitational Lensing Experiment (OGLE-III). In this paper we describe the catalog of 3361 classical Cepheids detected in the  40 square degrees area in the Large Magellanic Cloud. The sample consists of 1848 fundamental-mode (F), 1228 first-overtone (1O), 14 second-overtone (2O), 61 double-mode F/1O, 203 double-mode 1O/2O, 2 double-mode 1O/3O, and 5 triple-mode classical Cepheids. This sample is supplemented by the list of 23 ultra-low amplitude variable stars which may be Cepheids entering or exiting instability strip Description: The catalog data include VI high-quality photometry collected since 2001, and for some stars supplemented by the OGLE-II photometry obtained between 1997 and 2000. We provide basic parameters of the stars: coordinates, periods, mean magnitudes, amplitudes and parameters of the Fourier light curve decompositions. Our sample of Cepheids is cross-identified with previously published catalogs of these variables in the LMC. Individual objects of particular interest are discussed, including single-mode second-overtone Cepheids, multiperiodic pulsators with unusual period ratios or Cepheids in eclipsing binary systems.

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