“…Moreover, hot bands, or the presence of much BF 3 and of minor other impurities, contributed to the congestion of the spectra. In addition, when this work was started, the available rotational parameters for the ground vibrational state of F 2 BOH were fully insufficient since only the A, B, and C rotational constants had been derived from low J transitions observed in the MW studies (2,3). Consequently, using these A, B, and C rotational constants (Table 2), GSCD needed for unambiguous assignments could not be calculated accurately enough except for transitions involving very low J and K a values (J < 10 and K a < 5).…”