Comparisons between our uncorrected solar relative abundances and those from literature values. The gray dash-dotted line at zero is for reference, and the blue dashed line shows a fit to the mean weighted offset. Higher abundances at temperatures above solar are generally related to our improved gravity determinations. While our uncorrected abundances show a temperature-dependent trend toward underabundance at lower temperatures, comparisons here with literature values generally show good agreement. This indicates that other studies are also systematically underestimating abundances for lower-temperature stars, probably due to errors in the stellar atmosphere models.