**Table 5:** List of shadowing observations. Comparison of previous data-analyses results with our SWCX model. Data results include mainly the LB O VII and O VIII line fluxes.
$\begin{displaymath}\begin{tabular}{lclccccccc} \hline \hline &&&&&&&&& \\ [-8pt]... ...0.02:: & 0:: & 0::\\ &&&&&&&&& \\ [-4pt] \hline \end{tabular}\end{displaymath}$ ^a Only Smith et al. (2007) OFF exposure with Suzaku includes O VII and O VIII strengths of LB and halo emission (see Sect. 4.1.2 for details). ^b Prefixes are x: for XMM-Newton, c: for CHANDRA, s: for SUZAKU. ^c1 Smith et al. (2005), ^c2 Smith et al. (2007). ^d1 HSK07 & ^d2 Henley & Shelton (2007) see Sect. 4.2 for details.

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