References for Mg X

.elvlc file (energy levels)

% produced as part of the atomic database collaboration CHIANTI
% E. Landi - July 1999
%energy levels (1-24):  Martin, W. C., and Zalubas, R., 1980, J. Phys. Chem.  Ref. Data, 9, 1.
%Theoretical energy levels (1-24): Zhang,H.L., Sampson,D.H., Fontes,C.J., ADNDT, 44, 31.
%Innershell energy levels:  NIST database
%Innershell theoretical energy levels: Goett, S.J., Sampson, D.H., 1983, ADNDT, 29, 535
%

.splups file (collision data)

% filename: mg_10.splups
% produced as part of the atomic database collaboration CHIANTI
%collision strengths: Zhang, Sampson, Fontes, 1990, ADNDT, 44, 31
% Collision strengths innershell transitions: Goett, S.J., Sampson, D.H., 1983, ADNDT, 29, 535
%produced as part of the Arcetri/Cambridge/NRL atomic data base collaboration 'CHIANTI'
%
% E.Landi and K.P.Dere - July 1999

.wgfa file (radiative data)

% produced as part of the atomic data base collaboration CHIANTI
% E. Landi - July 1999, K. Dere - Nov 1999
%energy levels: Martin,W.C., Zalubas,R., 1980, J.Phys.Chem.Ref.Data, 9, 1.
 % Theoretical energy levels: Zhang,H.L., Sampson,D.H., Fontes,C.J., 1990, ADNDT, 44, 31.
 %oscillator strengths:  H.L.Zhang, D.H.Sampson, C.J.Fontes, 1990, ADNDT, 44, 31
 %oscillator strengths:  Martin, I., Karwowski, J., Diercksen, G.H.F., Barrientos, C., 1993, A&AS, 100, 595.
 % Innershell radiative data: Goett, S.J., Sampson, D.H., 1983, ADNDT, 29, 535
 %Comment: Other radiative data were calculated using SUPERSTRUCTURE with a 23 configuration model
%A values (autoionizing): Vainshtein, L.A., Safronova, U.I., 1978, ADNDT, 21, 49-68.
   and 1980, ADNDT, 25, 311 - updated by U.I. Safronova, 1999
%comment: unobserved lines
    2   25        -9.5974      7.530e-03      2.725e+11   1s2.(1S).2p 2P0.5 -         1s.2s2 2S0.5                 
    3   25        -9.6010      1.401e-02      5.066e+11   1s2.(1S).2p 2P1.5 -         1s.2s2 2S0.5