  We propose a line list that may be useful for the abundance analysis of
G-type stars in the wavelength range 4080 -- 6780 A. It is expected that the
line list will be useful for surveys/libraries with overlapping spectral
regions (e.g. ELODIE/SOPHIE libraries, UVES-580 setting of Gaia-ESO), and in
particular for the analysis of F- and G-type stars in general. The atomic data
are supplemented by detailed references to the sources. We estimated the Solar
abundances using stellar lines and the high-resolution Kitt Peak National
Observatory (KPNO) spectra of the Sun to determine the uncertainty in the log
gf values. By undertaking a systematic search that makes use of the lower
excitation potential and gf-values and using revised multiplet table as an
initial guide, we identified 363 lines of 24 species that have accurate
gf-values and are free of blends in the spectra of the Sun and a Solar analogue
star, HD 218209 (G6V), for which accurate and up-to-date abundances were
obtained from both ELODIE and PolarBASE spectra of the star. For the common
lines 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 of
varying species.
