Masseron, T., Plez, B., Van Eck, S., Colin, R. et al. 2014.
CH in stellar atmospheres: an extensive linelist.
Astron. Astrophys. 571, A47, 29pp.


Reformatted into Kurucz format for X-X, A-X, B-X, C-X
The energy levels have been shifted by 14.+ cm-1 (varying with band) 
so that the lowest level has zero energy.

These are the observed limits in V and J that we have adopted from the 
papers listed in CHJORGENSEN.README and in Masseron et al. above.

12CH
X00e1 39.5 X00f1 39.5 X00e2 39.5 X00f2 39.5
X01e1 39.5 X01f1 39.5 X01e2 39.5 X01f2 39.5
X02e1 31.5 X02f1 31.5 X02e2 31.5 X02f2 31.5
X03e1 31.5 X03f1 31.5 X03e2 31.5 X03f2 31.5
X04e1 27.5 X04f1 27.5 X04e2 27.5 X04f2 27.5
X05e1 11.5 X05f1 11.5 X05e2 11.5 X05f2 11.5
A00e1 34.5 A00f1 34.5 A00e2 34.5 A00f2 34.5
A01e1 32.5 A01f1 32.5 A01e2 32.5 A01f2 32.5
A02e1 31.5 A02f1 31.5 A02e2 31.5 A02f2 31.5
A03e1 27.5 A03f1 27.5 A03e2 27.5 A03f2 27.5
A04e1 23.5 A04f1 23.5 A04e2 23.5 A04f2 23.5
A05e1 16.5 A05f1 16.5 A05e2 16.5 A05f2 16.5
B00f1 22.5 B00e2 22.5 
B01f1 14.5 B01e2 14.5
C00e1 15.5 C00f2 16.5 
C01e1 13.5 C01f2 13.5
C02e1 16.5 C02f2 16.5 

13CH  
X00e1 25.5 X00f1 25.5 X00e2 25.5 X00f2 25.5
X01e1 26.5 X01f1 26.5 X01e2 26.5 X01f2 26.5
X02e1 14.5 X02f1 14.5 X02e2 14.5 X02f2 14.5
X03e1  9.5 X03f1  9.5 X03e2  9.5 X03f2  9.5
A00e1 25.5 A00f1 25.5 A00e2 25.5 A00f2 25.5
A01e1 26.5 A01f1 26.5 A01e2 26.5 A01f2 26.5
A02e1 14.5 A02f1 14.5 A02e2 14.5 A02f2 14.5
A03e1  9.5 A03f1  9.5 A03e2  9.5 A03f2  9.5
B00f1 20.5 B00e2 20.5 
B01f1 12.5 B01e2 12.5
C00e1 20.5 C00f2 20.5 

Levels above these ranges are marked as negative.  Extroplated levels 
can have large errors.