Figure 6

Fig 6   Spatial imaging and energy resolution of an imaging strip detector with a Ta absorber, shown schematically in Fig 2.   The energy width is 13 eV, using fitting to the broadened line structure of the Ka1 and Ka2 pair of lines of the 55 Fe source. Many different grid spacings (energy binnings) were used and the results for D E for each grid spacing were averaged to avoid any false results due to binning of the data.