“…In a previous work [21], we identified several hot transitions belonging to the band (m 4 + m 8 ) À m 4 , which were used in calculations aimed to determine the value of the intrinsic torsional splitting in the m 4 + m 8 state. Several features of this band, as some Q subbranches, stand out quite clearly even in moderate and low resolution spectra, and can be relevant in the examination of atmospheric spectra and planetary radiance spectra.…”