We determined the C, N, and O abundances of 160 nearby F, G, and K dwarfs and subgiants by using spectra obtained with the HIDES spectrograph at Okayama Astrophysical Observatory, with the purposes of (1) establishing the runs of [C/Fe], [N/Fe], and [O/Fe] for these galactic disk stars in the metallicity range of -1<~[Fe/H]~<+0.4, (2) searching for any difference in the CNO abundances of planet-host stars as compared to non-planet-host stars, and (3) examining the consistency of the abundances derived from different lines to check the validity of the analysis. The non-LTE effect on the abundance determination was taken into consideration based on our extensive statistical-equilibrium calculations.

Cone search capability for table J/PASJ/57/65/fitabund (Abundance results of spectral fitting analyses)

Cone search capability for table J/PASJ/57/65/ackerman (Reanalysis of the data of Ackerman et al. (2004A&A...414..931A))

Cone search capability for table J/PASJ/57/65/tomkin92 (Reanalysis of the data of Tomkin et al. (1992AJ....104.1568T))

Cone search capability for table J/PASJ/57/65/tomkin95 (Reanalysis of the data of Tomkin et al. (1995AJ....109.2204T))