We report the results of our analysis of new high-resolution spectra of 30 late-F to early-G dwarf field stars for the purpose of deriving their Li abundances. They were selected from the subsample of stars in the Valenti and Fischer compilation that are lacking detected planets. These new data serve to expand our comparison sample used to test whether stars with Doppler-detected giant planets display Li abundance anomalies. Our results continue to show that Li is deficient among stars with planets when compared to very similar stars that lack such planets. This conclusion is strengthened when we add literature data to ours in a consistent way. We present a table of stars with planets paired with very similar stars lacking planets, extending the recent similar results of Delgado Mena et al. (2014A&A...562A..92D, Cat. J/A+A/562/A92).

Cone search capability for table J/MNRAS/446/1020/table1 (Parameters of the programme stars determined from our spectroscopic analyses)

Cone search capability for table J/MNRAS/446/1020/table2 (The SWPs from the literature data set as well as the most similar non-SWP for each SWP)