Fig. 13.

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(a) Three stars in common between XSL (red) and MILES (black), smoothed to the MILES resolution. Residual spectra are in green. Top: BD-114126. Middle: HD 204543. Bottom: HD 130095. Wavelength scale is logarithmic. (b) Six stars that have the largest mismatch between MILES (black) and XSL (red), compared with PHOENIX theoretical star of similar stellar parameters (grey). The grey shaded areas on both sub-figures mark the UVB and VIS merging regions with possible dichroic contamination.
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