CAH.ASC is a merged file of CAHXXYADIN.ASC, CAHAX.ASC, CAHBX.ASC, 
and CAHEXLI.ASC.  The data are from the literature and have been 
processed into Kurucz format.  I have not been able to get CAHDX to work. 


CAHXXYADIN.ASC

Yadin, B., Veness, T., Conti, P., Hill. C., Yurchenko, S.N., and 
     Tennyson, J. 2012.  M.N.R.A.S. 425, 34-43.  
     Truncated at 100 cm-1.    

CAHAX.ASC and CAHBX.ASC

Observed energy levels, and extrapolated Dunham fits for higher levels 
that I listed as negative, were taken from

Shayesteh, A., Ram, S.R., and Bernath, P.F. 2013.  JMS 288, 46-51.

I generated approximate Honl-London factors from the Dunham coefficients.

The spin-unresolved line lists from 

Weck, P.F., Stancil, P.C., Kirby, K. 2003.  J. Chem. Phys. 118, 9997-10005.

were divided into the actual lines at the observed positions using the 
Honl-London factors.
 
 
CAHEXLI.ASC

Li, G., Harrison, J.J., Ram, R.S., Western, C.M., and Bernath, P.F.  2012.  
    JQSRT 113, 67-74.


CAHDX 

     Unresolved f values are given by Weck, Stancil, and Kirby 2003.  I 
have determined the observed energies from the observed lines and the
known X energies given by Shayesteh, Ram, and Bernath 2013.  However none 
of the theoretical interpretations have produced reliable results.  

Gustavsson, T., Klynning, L., and Lindgren, B. 1985.  Phys. Scr. 31, 269-274.

suggest that the levels are a mixture of B and D and E states.