OHAXUPDATE
 
New observed energies for A and X and new extrapolations for A
yield improved wavelengths
 
Coxon, J.A. 1980.  Can. J. Phys. 58, 933-949. A0-A3
 
Coxon, J.A., Sappey, A.D., and Copeland, R.A. 1991.
           J. Mol. Spectr. 145, 41-55.  A4-A9
 
Bernath, P.F. and Colin, R. 2009.  J. Mol. Spectr. 257, 20-23.  X0-X13
 
Stark, G., Brault, J.W., Abrams, M.C. 1994.  J. Opt. Soc. Am. B 11, 3-32.
   Not used for this revision.  Provides line list for low V.  Energies
   need to be rereduced for A state using Bernath et al. X energy levels.
   Many low J weak lines in Stark et al. are missing from Kurucz (1982)
   OHAX.ASC (and in this revision).  OH A-X should be recomputed.
 
 
OHXXGOLDMAN.ASC also should be updated. It was taken from HITRAN96.
 
 
            PARTIAL UPDATE JUNE 2019
Yousefi, M., Bernath, P.F., Hodges, J. and Masseron, T. 2018.  JQSRT 217, 416-424,
 
16OH AX lines replaced by Yousefi lines where they exist.
18OH AX lines are unchanged
16OH AX lines are in the range 204-537 nm X10,A07, loggf > -8.
OHYousefi lines are in the range 230-637 nm X09,A04, loggf > -15.