We have performed the Fourier decomposition analysis of 8- and 13-yr V-band light curves of a carefully selected sample of 454 fundamental-mode RR Lyrae variables (RRab type), detected in an ~=14 square degree area of the Small Magellanic Cloud (SMC) and listed in the Optical Gravitational Lensing Experiment, phase III, Catalogue of Variable Stars. The Fourier decomposition parameters were used to derive metal abundances and distance moduli, following the methodology described by Kapakos, Hatzidimitriou & Soszynski, Paper I (2011, Cat. J/MNRAS/415/1366).
Cone search capability for table J/MNRAS/426/2063/table1 (Fourier decomposition parameters for 1887 RRab stars derived from data of the OGLE phases II and III in the V band)
Cone search capability for table J/MNRAS/426/2063/table2 (Fourier decomposition parameters for 169 RRc stars derived from data of the OGLE phases II and III in the V band)