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We propose a line list that may be useful for the abundance analysis ofG-type stars in the wavelength range 4080 -- 6780 A. It is expected that theline list will be useful for surveys/libraries with overlapping spectralregions (e.g. ELODIE/SOPHIE libraries, UVES-580 setting of Gaia-ESO), and inparticular for the analysis of F- and G-type stars in general. The atomic dataare supplemented by detailed references to the sources. We estimated the Solarabundances using stellar lines and the high-resolution Kitt Peak NationalObservatory (KPNO) spectra of the Sun to determine the uncertainty in the loggf values. By undertaking a systematic search that makes use of the lowerexcitation potential and gf-values and using revised multiplet table as aninitial guide, we identified 363 lines of 24 species that have accurategf-values and are free of blends in the spectra of the Sun and a Solar analoguestar, HD 218209 (G6V), for which accurate and up-to-date abundances wereobtained from both ELODIE and PolarBASE spectra of the star. For the commonlines with the Gaia-ESO line list v.6 provided by the Gaia-ESO collaboration,we discovered significant inconsistencies in the gf-values for certain lines ofvarying species.

An Updated Line List for Spectroscopic Investigation of G Stars- I: Redetermination of the Abundances in the Solar Photosphere