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The Spectrometer/Telescope for Imaging X-Rays (STIX) onboard Solar Orbiter was designed to observe solar flares in the X-ray range of 4-150 keV, providing spectral, temporal and spatial information. Besides 30 imaging detectors, STIX has two additional detectors, the coarse flare locator (CFL) and the background (BKG) detector. Flares observed from Earth are classified using their peak X-ray flux observed by the GOES satellites. Roughly half of all flares observed by STIX are located on the backside of the Sun. These flares lack a GOES-class classification.\n  Aims. 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