T.D.S. spectroscopic databank for spherical tops: DOS version

Carbon Monoxide on Jupiter: Evidence for Both Internal and External Sources

“…Those for AsH 3 come from Dana et al (1993) and those for NH 3 come from Cottaz et al (2000). As concerns germane, we generated a linelist for the five isotopes of germanium using the TDS program (Tyuterev et al 1994) and calibrated the intensities with measurements of the R(0) and R(1) lines of 72 GeH 4 . We assumed telluric abundances for the germanium isotopes.…”

Meridional variations of temperature, C2H2 and C2H6 abundances in Saturn's stratosphere at southern summer solstice

“…The variation of saturnian airmass and gravity for each observed latitude was included in the calculation. Line positions, intensities and energies for NH 3 , CH 3 D, 12 C 2 H 2 , 12 C 13 CH 2 , 12 C 2 H 6 and 12 C 13 CH 6 were taken from the GEISA databank (Jacquinet-Husson et al, 1999), and those for 12 CH 4 and 13 CH 4 come from the TDS spectroscopic databank (Tyuterev et al, 1994). H 2 and He mole fractions were 0.877 and 0.118, respectively (Conrath and Gautier, 2000).…”

A Radiative Equilibrium Model of 51 Peg b

“…The atmosphere is finally considered to be composed of the gases (Tyuterev et al 1994) 0.071 0.55 Fink et al (1977) Strong et al (1993 For example, at T = 1000 K and P = 1 bar, q CO 5.5 × 10 −4…”

“…For the bands below 6000 cm −1 , a line list was calculated with the TDS computational code (Tyuterev et al 1994), specialized in the determination of highresolution spectroscopic data for spherical top molecules. All the rovibrational transitions between the first five vibration levels (ground state, dyad, pentad, octad, and tetradecad) for 12 CH 4 and 13 CH 4 have been included.…”