All Tables

• Table 1: Atomic parameters adopted for [O I] 6300 Å line, O I 7771-5 Å triplet and the near-UV OH lines.
• Table 2: Sensitivity of the three indicators [O I], O I and OH to changes of 100 K in effective temperature, 0.3 dex in gravity and metallicity, and 0.5 km s^-1 in microturbulence.
• Table 3: Average [O/H] values from the different indicators, with the corresponding dispersions, for the set of planet host stars and the comparison sample.
• Table 4: Oxygen abundances from [O I] line in a set of planet host stars.
• Table 5: Oxygen abundances from [O I] line in a set of comparison stars.
• Table 6: Oxygen abundances from OH band synthesis for a set of stars with planets and brown dwarf companions.
• Table 7: Oxygen abundances from OH band synthesis for a set of comparison stars (stars without giant planets).
• Table 8: Oxygen abundances from Triplet lines in a set of planet host stars.
• Table 9: Oxygen abundances from Triplet lines in a set of comparison stars.