“…Using a 6.5-m focal length grating with dispersion of 1.2 A/mm, he obtained the rotational structure of the 4-11, 5-13, 6-15, 7-16, 8-17, 9-19, 10-20, and 10-21 bands. Gero further reported [74] rotational structure for the 9-18, 11-20, 12-22, and [13][14][15][16][17][18][19][20][21][22][23][24] [74] believed that the appearance of these bands was due to accidental accumulation of lines, where strong overlapping is observed.…”