“…The fit of Melen et al [34] included rotational lines in v=0-3, from both their assignments of an ATMOS (1985) [39] solar spectrum and laboratory measurements, and rovibrational laboratory data from Maillard et al [13]. Hyperfine rotational data in v=0-3 from several other studies [40,41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58] were also included in the fit by Melen et al [34]. Despite hyperfine structure not being included in the results of Bernath and Colin [33], they took some of this information into account by adding pseudotransitions to the fit, between e and f parity levels and various J levels ("Λ-doubling data"), based on the term values calculated by Melen et al [34].…”