All Tables

• Table 1: Measured levels and excitation schemes in Os II.
• Table 2: Measured levels and excitation schemes in Os I.
• Table 3: Experimental and theoretical radiative lifetimes (in ns) for odd-parity levels of Os I.
• Table 4: Experimental and theoretical radiative lifetimes (in ns) for odd-parity levels of Os II.
• Table 7: Os I lines previously observed in the Sun and the stars. Lines between parentheses turn out to be unsuitable for Os abundance determination, because they are either too weak or heavily blended in the sun or in metal-poor stars.
• Table 8: Lines used to derive the solar Os abundance. Abundances are derived using either the Holweger-Müller or MARCS models.
• Table 5: Branching fractions (BF), transition probabilities (gA in 10⁶ s^-1) and oscillator strengths (log gf) for transitions depopulating odd-parity levels in Os I.
• Table 6: Branching fractions (BF), transition probabilities (gA, in 10⁶ s^-1) and oscillator strengths (log gf) for transitions depopulating the odd-parity levels of Os II.