Oxygen compounds in Titan's stratosphere as observed by Cassini CIRS

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AN ESTIMATE OF THE CHEMICAL COMPOSITION OF TITAN's LAKES (2009, unknown): “— (a)Owen & Niemann 2009; (b)Niemann et al. 2005; (c)De Kok et al. 2007.”
A photochemical model of Titan's atmosphere and ionosphere (2009, result): “, 2005) and ground-based observations in the millimeter range that were reviewed by de Kok et al. (2007). The model data on H2O and CO2 also agree with the ISO and CIRS observations, respectively.”
Vertical abundance profiles of hydrocarbons in Titan's atmosphere at 15° S and 80° N retrieved from Cassini/CIRS spectra (2007, background): “Vertical profiles of CO2 are presented in de Kok et al. (2006) .”
Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission I. Hydrocarbons, nitriles and CO2 vertical mixing ratio profiles (2010, result): “Our results are also consistent with those of de Kok et al. (2007) who inferred from nadir data acquired between 75 S and 30 N a constant mixing ratio value of 15 ppb.”
Negative ion chemistry in Titan's upper atmosphere (2008, background): “Dibeler et al. (1961) provide information about the magnitude at the peak of the resonance profiles relative to the total electron impact cross section of HC3N at 70 eV, with values of 0.”
The NEMESIS planetary atmosphere radiative transfer and retrieval tool (2008, unknown): “[20–24]).”