Solar log gf values for the spectral lines in the range λ λ 6209-6273 Å

Abstract

Utilizing Lieze solar atlas and solar photospheric models, we derived log gf values for the spectral lines in the wavelength range λλ 6209 - 6273 Å. These values, intended for use in a future study of high resolution reticon spectrum of the star gamma Draconis, are presented along with some recent results available in the literature