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Table 2:

Dominant radiative transition data from the ground state of the recombining ion $3p^6\;({}^1S_{0})\to 3p^53d\;({}^1P_{1}^{{\rm o}})$, where $v_{(u)}^{\rm [\pm p]}$ denotes $v(u)\times 10^{\pm p}$.
\begin{displaymath}\begin{tabular}{c l l l l c l l l l}
...8 $ &$2.145 $ &TDCHF$^{f}$\, & & & & & \\

Notes. In the case of ${\rm Sc}^{3+}$and ${\rm Ti}^{4+}$ions, refer to Nikolic et al. (2010) and Nikolic et al. (2009), respectively.

References. Assigned uncertainties: $^{(\dag )}$ <18%, $^{(\ddag )}$  <25%; (a) present work: 2894-level MCBP results; (b) critically compiled experimental data of Shirai et al. (2000); (c) MCHF results of Froese-Fischer & Tachiev (2006); (d) 6284-level FAC results of Aggarwal et al. (2006); (e) CIV3 results of Verma et al. (2006); (f) single-config. TDCHF results of Ghosh & Mukherjee (1997); (g) semiempirical results of Loginov & Tuchkin (2002); (h) 6164-level FAC results of Aggarwal & Keenan (2008); (i) restricted CIV3 results of Verma et al. (2007); (j) 18-config. CIV3 LS results of Baluja (1986); $^{(\S)}$ extrapolated along the isoelectronic sequence.

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