“…Due to the limitations of narrow bandgap (typically Si) X-ray spectrometers commonly in use today [1,2], a variety of wide bandgap materials, such as GaAs [3][4][5][6][7], diamond [8,9], SiC [10][11][12], In0.5Ga0.5P [13,14], Al0.52In0.48P [15][16][17], and AlxGa1-xAs [18][19][20][21], have been investigated as potential X-ray detector replacements. The cooling systems and radiation shielding often required for Si X-ray spectrometers [22] place substantial burdens on spacecraft mass, volume, and power consumption, limiting their suitability for certain space science applications (e.g.…”