Einstein A-coefficients and statistical weights for molecular absorption transitions in the HITRAN database

By Marie Šimečkováa, David Jacquemarta, Laurence S. Rothmana, Robert R. Gamacheb, Aaron Goldmanc. 2006

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ExoMol: molecular line lists for exoplanet and other atmospheres (2012, methodology): “We follow the HITRAN convention (Simeckova et al. 2006) and include the entire nuclear statistical weight g (i) ns of the molecule explicitly in gi and hence the partition function Z(T ).”
HITEMP, the high-temperature molecular spectroscopic database (2010, background): “[15] g00 Statistical weight of the lower state 7 Real See details in Ref.”
ROVIBRATIONAL LINE LISTS FOR NINE ISOTOPOLOGUES OF THE CO MOLECULE IN THE X1Σ+ GROUND ELECTRONIC STATE (2015, methodology): “First, the rovibrational matrix elements, Mv ′,J ′ v′′,J ′′ , are retrieved from the best available experimental measurements of rovibrational line intensities, using the equations in Šimečková et al. (2006).”