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MM_Mg-2013-11-10.tex
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MM_Mg-2013-11-10.tex
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\begin{table*}
\begin{center}
\caption{
Laboratory data for transitions of Mg of interest for quasar absorption-line varying-$\alpha$ studies described in \Sref{ssec:Mg}. See \Sref{ssec:tabs} for full descriptions of each column.
}
\label{tab:Mg}\vspace{-0.5em}
{\footnotesize
\begin{tabular}{:l;l;c;l;c;l;c;l;l;c;c;c;c}\hline
\multicolumn{1}{c}{Ion}&
\multicolumn{1}{c}{Tran.}&
\multicolumn{1}{c}{$A$}&
\multicolumn{1}{c}{$\omega_0$}&
\multicolumn{1}{c}{$X$}&
\multicolumn{1}{c}{$\lambda_0$}&
\multicolumn{1}{c}{$\delta v$}&
\multicolumn{1}{c}{Lower state}&
\multicolumn{1}{c}{Upper state}&
\multicolumn{1}{c}{ID}&
\multicolumn{1}{c}{IP$^-$, IP$^+$}&
\multicolumn{1}{c}{$f$ or {\it \%}}&
\multicolumn{1}{c}{$q$}\\
&
&
&
\multicolumn{1}{c}{[cm$^{-1}$]}&
&
\multicolumn{1}{c}{[\AA]}&
\multicolumn{1}{c}{[m\,s$^{-1}$]}&
&
&
&
\multicolumn{1}{c}{[eV]}&
&
\multicolumn{1}{c}{[cm$^{-1}$]}\\
\hline
Mg{\sc \,i} & 2026 & 24.3050 & 49346.772620(36)$^{}$ & 1 & 2026.4749788(15) & 0.2 & $3\rm{s}^2~^1\rm{S}_0 $ & $3\rm{s}4\rm{p}~^1\rm{P}_1^{\rm o} $ & Mg$^1_{2}$ & ---, 7.65 & 0.113 & $ 87^{a,b}(7) $\\
\rowstyle{\itshape} & & 26 & 49346.854173(40)$^{c}$ & 0 & 2026.4716298(16) & 0.2 & $ $ & $ $ & & & 11.01\% & $ ^{} $\\
\rowstyle{\itshape} & & 25 & 49346.807724(40)$^{c}$ & 0 & 2026.4735372(16) & 0.2 & $ $ & $ $ & & & 10.00\% & $ ^{} $\\
\rowstyle{\itshape} & & 24 & 49346.756809(35)$^{c}$ & 0 & 2026.4756281(14) & 0.2 & $ $ & $ $ & & & 78.99\% & $ ^{} $\\
& 2852 & 24.3050 & 35051.28076(19)$^{}$ & 1 & 2852.962797(15) & 1.6 & $ $ & $3\rm{s}3\rm{p}~^1\rm{P}_1^{\rm o} $ & Mg$^1_{1}$ & & 1.83 & $ 90^{a,b}(10) $\\
\rowstyle{\itshape} & & 26 & 35051.32015(25)$^{d}$ & 0 & 2852.959591(20) & 2.1 & $ $ & $ $ & & & 11.01\% & $ ^{} $\\
\rowstyle{\itshape} & & 25 & 35051.29784(25)$^{d}$ & 0 & 2852.961407(20) & 2.1 & $ $ & $ $ & & & 10.00\% & $ ^{} $\\
\rowstyle{\itshape} & & 24 & 35051.27311(17)$^{d}$ & 0 & 2852.963420(14) & 1.5 & $ $ & $ $ & & & 78.99\% & $ ^{} $\\
Mg{\sc \,ii} & 2796 & 24.3050 & 35760.85414(20)$^{}$ & 1 & 2796.353790(16) & 1.7 & $3\rm{s}~^2\rm{S}_{1/2} $ & $3\rm{p}~^2\rm{P}_{3/2}^{\rm o} $ & Mg$^2_{1}$ & 7.65, 15.04 & 0.6155 & $ 212^{e}(2) $\\
\rowstyle{\itshape} & & 26 & 35760.9403866(53)$^{f}$ & 0 & 2796.34704565(42) & 0.04 & $ $ & $ $ & & & 11.01\% & $ ^{} $\\
\rowstyle{\itshape} & & 25 & 35760.85850(64)$^{f,g,h}$ & 3 & 2796.353449(50) & 5.4 & $F=2 $ & $F=1,2,3 $ & & & 4.17\% & $ ^{} $\\
\rowstyle{\itshape} & & 25 & 35760.91502(64)$^{f,g,h}$ & 3 & 2796.349030(50) & 5.4 & $F=3 $ & $F=2,3,4 $ & & & 5.83\% & $ ^{} $\\
\rowstyle{\itshape} & & 24 & 35760.8373967(53)$^{f}$ & 0 & 2796.35509903(42) & 0.04 & $ $ & $ $ & & & 78.99\% & $ ^{} $\\
& 2803 & 24.3050 & 35669.30440(20)$^{}$ & 1 & 2803.530982(16) & 1.7 & $ $ & $3\rm{p}~^2\rm{P}_{1/2}^{\rm o} $ & Mg$^2_{2}$ & & 0.3058 & $ 121^{e}(2) $\\
\rowstyle{\itshape} & & 26 & 35669.3905712(53)$^{f}$ & 0 & 2803.52420938(42) & 0.04 & $ $ & $ $ & & & 11.01\% & $ ^{} $\\
\rowstyle{\itshape} & & 25 & 35669.30492(64)$^{f,g,h}$ & 3 & 2803.530941(50) & 5.4 & $F=2 $ & $F=2,3 $ & & & 4.17\% & $ ^{} $\\
\rowstyle{\itshape} & & 25 & 35669.36798(64)$^{f,g,h}$ & 3 & 2803.525985(50) & 5.4 & $F=3 $ & $F=2,3 $ & & & 5.83\% & $ ^{} $\\
\rowstyle{\itshape} & & 24 & 35669.2876697(53)$^{f}$ & 0 & 2803.53229720(42) & 0.04 & $ $ & $ $ & & & 78.99\% & $ ^{} $\\
\hline
\end{tabular}
}
{\footnotesize References:
$^{a}$\citet{Berengut:2005:044501};
$^{b}$\citet{Savukov:2008:042501};
$^{c}$\citet{Hannemann:2006:012505};
$^{d}$\citet{Salumbides:2006:L41};
$^{e}$\citet{Dzuba:2007:062510};
$^{f}$\citet{Batteiger:2009:022503};
$^{g}$\citet{Itano:1981:1364};
$^{h}$\citet{Sur:2005:25}.}
\end{center}
\end{table*}