\contentsline {figure}{\numberline {2.1}{\ignorespaces The BCS data compression algorithm}}{7}
\contentsline {figure}{\numberline {4.2}{\ignorespaces Factors that determine the SXT effective area. Panel (a) shows the double entrance filter transmission; panel (b) shows the mirror reflectivity including the obscuration from the support structures; panel (c) shows the CCD quantum efficiency. Panel (d) is the product of panels (a), (b), and (c). }}{18}
\contentsline {figure}{\numberline {4.3}{\ignorespaces The effective area of the SXT: The thick curve shows gives the effective area for the indicated filter. The thin curve is the open filter case (no analysis filter) effective area over-plotted for comparison. }}{19}
\contentsline {figure}{\numberline {4.4}{\ignorespaces The total SXT signal as a function of $\mathop {\mathgroup \symoperators log}\nolimits _{10}(T_e)$ for the open filter and the analysis filters as indicated. NOTE: Be and Al12 are mistakenly reversed in Tsuneta {\it et al.}, (1991). }}{20}
\contentsline {figure}{\numberline {4.5}{\ignorespaces Ratios of the SXT response functions. For the curve marked ``Be119/(2$\times $Al12)'' the effective observing time with the Al12 filter has been doubled with respect to the Be119 filter. For the curve marked ``$2\times $Al12/Al.1'' the effective observing time with the Al12 filter has again been doubled, this time with respect to the Al.1 filter. }}{21}
\contentsline {figure}{\numberline {4.6}{\ignorespaces Relative alignment of the X-ray and optical images (as of 1992 analysis). According to the final calibration in 2008, the NB and WB boresights are both in the NE of the X-ray boresight.}}{24}
\contentsline {figure}{\numberline {4.7}{\ignorespaces The effective area (or vignette function) as a function of off-axis angle. The solid curve was derived from \unhbox \voidb@x \hbox {C K} and \unhbox \voidb@x \hbox {Al K} data and the dashed curve from \unhbox \voidb@x \hbox {Ag L} data. }}{30}
\contentsline {figure}{\numberline {A.8}{\ignorespaces Timing of HXT data for Hi/Hi telemetry frames}}{41}
\contentsline {figure}{\numberline {A.9}{\ignorespaces Timing of HXT data for Med/Med telemetry frames}}{41}
\contentsline {figure}{\numberline {A.10}{\ignorespaces Timing of HXT data for Hi/Med telemetry frames}}{42}
\contentsline {figure}{\numberline {A.11}{\ignorespaces Timing of HXT data for Med/Hi telemetry frames}}{42}
\contentsline {figure}{\numberline {A.12}{\ignorespaces Timing of SXT data}}{43}
\contentsline {figure}{\numberline {A.13}{\ignorespaces Timing of WBS SXS-PH data}}{43}
\contentsline {figure}{\numberline {A.14}{\ignorespaces Timing of WBS HXS-PH data}}{44}
\contentsline {figure}{\numberline {A.15}{\ignorespaces Timing of WBS GRS-PHL data}}{44}
\contentsline {figure}{\numberline {A.16}{\ignorespaces Timing of WBS SXS-PC data}}{44}
\contentsline {figure}{\numberline {B.17}{\ignorespaces SXT CCD Pixel Layout}}{46}