HIGHER Js AND Vs ARE NEEDED. THE LINE LISTS HAVE TO BE FILLED OUT WITH PREDICTED LINES. These are new linelists taken from the literature and put into Kurucz format. MGH.ASC all the lists merged MGHAX.ASC merged MGHAXGSB24.ASC, MGHAXHINKLE25.ASC, MGHAXHINKLE26.ASC MGHAXGSB24.ASC GharibNezhad, E., Shayesteh, A., and Bernath, P.F. 2013. MNRAS 432, 2043-2047. energies from Shayesteh, A., Henderson, R.D.E., LeRoy, R.J., and Bernath, P.F. 2007. J. Phys. Chem. A 111, 12495. MGHAXHINKLE25.ASC energies from MGHAXHINKLE26.ASC Hinkle, K.H., Wallace, L., Ram, R.S., Bernath, P.F., Sneden, C., and Locatello, S. 2013. Ap.J.Supp. 207, 26 (7pp) gf values from GharibNezhad, E., Shayesteh, A., and Bernath, P.F. 2013. MNRAS 432, 2043-2047. 25,26 = 24 MGHBXGSB24.ASC GharibNezhad, E., Shayesteh, A., and Bernath, P.F. 2013. MNRAS 432, 2043-2047. No 25,26 energies from Shayesteh, A., Henderson, R.D.E., LeRoy, R.J., and Bernath, P.F. 2007. J. Phys. Chem. A 111, 12495. MGHXXYADIN.ASC merged MGHXXYADIN24.ASC,MGHXXYADIN25.ASC,MGHXXYADIN25.ASC MGHXXYADIN24.ASC Yadin, B., Veness, T., Conti, P., Hill, C., Yurchenko, S., MGHXXYADIN25.ASC and Tennyson, J. 2012. MNRAS 425, 34-43. MGHXXYADIN26.ASC 25MgH and 26MgH B-X can be predicted but I have not yet done it. Radiative damping including predissociation can be included but I have not yet done it.