========================================================================== J/AJ/127/334 MACHO LMC first-overtone RR Lyrae variables (Alcock+, 2004) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table[12345].dat table6.dat ========================================================================== Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/AJ/127/334 ==========================================================================
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Beginning of ReadMe : J/AJ/127/334 MACHO LMC first-overtone RR Lyrae variables (Alcock+, 2004) ================================================================================ The MACHO project Large Magellanic Cloud variable-star inventory. XIII. Fourier parameters for the first-overtone RR Lyrae variables and the LMC distance. Alcock C., Alves D.R., Axelrod T.S., Becker A.C., Bennett D.P., Clement C.M., Cook K.H., Drake A.J., Freeman K.C., Geha M., Griest K., Lehner M.J., Marshall S.L., Minniti D., Muzzin A., Nelson C.A., Peterson B.A., Popowski P., Quinn P.J., Rodgers A.W., Rowe J.F., Sutherland W., Vandehei T., Welch D.L. <Astron. J., 127, 334-354 (2004)> =2004AJ....127..334A (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Magellanic Clouds ; Stars, variable Keywords: galaxies: distances and redshifts - Magellanic Clouds - RR Lyrae variable Abstract: Shapes of RR Lyrae light curves can be described in terms of Fourier coefficients that past research has linked with physical characteristics such as luminosity, mass, and temperature. Fourier coefficients have been derived for the V and R light curves of 785 overtone RR Lyrae variables in 16 MACHO fields near the bar of the LMC. Description: Our investigation is based on the RR Lyrae data from 16 LMC fields observed for the MACHO project. The LMC fields included are Nos. 2, 3, 5, 6, 10, 11, 12, 13, 14, 15, 18, 19, 47, 80, 81, and 82, all of which are close to the bar. The field of view for each field is 0.52deg^2^. An identification chart and a list of the right ascension and declination of the field centers are available at http://wwwmacho.mcmaster.ca .