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A. Hornstrup is a leading figure in astrophysics, specializing in microlensing detection and X-ray astronomy. Their most prominent contribution lies in the real-time identification of weak microlensing anomalies, exemplified by the 2012 study of OGLE-2008-BLG-510. This work, which has garnered 25 citations, demonstrated the first automated detection of a subtle asymmetric light-curve peak using the ARTEMiS system, distinguishing between a brown dwarf and a stellar binary. Hornstrup’s expertise extends to the high-energy universe, as shown in their 2004 work on the XEUS mission, which explored the evolution of hot cosmic phenomena. While their citation counts reflect focused impact, their innovative use of automated real-time analysis has advanced exoplanet and stellar astrophysics, offering a template for rapid anomaly detection. Hornstrup’s research bridges observational precision and technological automation, making them a key contributor to microlensing surveys and X-ray cosmology. Their work continues to inspire students and researchers seeking to unravel the universe’s faintest signals.