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The observational data of the near infrared bands (H and K) have been usedfor the modeling mean light curves. Also the visual observational data havebeen fitted the same. The infrared and visual mean light curves were compared.All parameters and Fourier-coefficients of the mean light curves were obtained.The periodogram analysis of the variation of the brightness have been carriedout.

The model parameters of the mean light curves of the variable red giant  stars in the near infrared colour-bands and compare them with the visual mean  light curves