Tables of internal partition functions and thermodynamic properties of high-temperature Mars-atmosphere species from 50K to 50000K

High-temperature thermodynamic properties for Mars-atmosphere components (Ar, Ar⁺, Ar²⁺, Ar³⁺, Ar⁴⁺, C, C⁺, C²⁺, C³⁺, C⁴⁺, C^-, C₂, C²⁺, C₂^-, C₃, CN, CN⁺, CN^-, CO, CO⁺, CO₂, CO ₂⁺, e^-, N, N⁺, N²⁺, N³⁺, N⁴⁺, N^-, N₂, N₂ ⁺, N₂^-, N₃, NO, NO⁺, NO₂, N₂O, N₂O⁺, CNO, O, O ⁺, O²⁺, O³⁺, O⁴⁺, O^-, O₂, O₂⁺, O₂^-, O ₃, O₃^-,C₂N, C₂O, CO ₂^-) are presented and discussed. The present report is divided into two parts: in the first one, theoretical aspects of the calculation are described. Results are discussed and compared with previous works including aspects such as quasi-bound rotational states for molecules and cut-off criteria and autoionasing states for atomic species. The second part provides tables of spectroscopic data used in the calculation and thermodynamic properties in the temperature range from 50 K to 50000 K at P=1 bar. Finally, fitting coefficients for nondimensional specific heat are included.