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The energy resolution of the system, as obtained with several fluorescence X-ray lines, is described.
Kα X-ray lines were analysed except for lead (Mα lines).
The X-ray lines show considerable broadening, indicating the fine particle nature of the ferrite.
Nevertheless, the intensity of graphene X-ray lines is under possibility for quality Rietveld refinement.
Energy resolution is reported for two X-ray lines, 1.5 & 5.9 keV, at multiple temperatures between 150 and 210 K.
It is shown that intensities of various characteristic X-ray lines are well correlated with the respective elemental concentrations.
We calibrated the sensor with varying X-ray tube voltages and used tungsten X-ray lines to verify its accuracy.
Both X-ray lines will be monitored by new generation energy-resolved micropattern gas detectors with 1-D position reconstruction capability.
The shaded spectral region of interest ROI outlined by dotted lines represents the sum of Au + Hg Mα X-ray lines.
These calculations may provide an alternative explanation to the observed X-ray lines of early GRBs afterglows (such as GRB 011211).
I describe the different approaches applicable to low-resolution and high-resolution spectra, especially focusing on the new grating spectra with X-ray lines.
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