“…Like YbO, the high density of states found in the spectrum of CrN displayed in Figure is likely due to ion pair states, in this case diabatically correlating to Cr + 3d 5 , 6 S g + N – , 2p 4 , and 3 P g , which drop down into the energetic region spanned in Figure . Indeed, previous spectroscopic work has identified the A 4 Π and B 4 Σ – states near 13,500 cm –1 and 20,500 cm –1 , respectively. , These states leave the 4s-like 9σ orbital of CrN vacant and probably correlate diabatically to the Cr + 3d 5 , 6 S g + N – , 2p 4 , 3 P g ion pair limit. Additional ion pair states deriving from the Cr + 3d 4 4s 1 , 6 D g + N – , 2p 4 , 3 P g ion pair limit, approximately 12,000 cm –1 higher in energy, also undoubtedly drop into the region spanned by Figure .…”