GPU-based framework for detecting small Solar system bodies in targeted exoplanet surveys

Small Solar system bodies are pristine remnants of Solar system formation, which provide valuable insights for planetary science and astronomy. Their discovery and cataloguing also have strong practical implications to life on Earth as the nearest asteroids could pose a serious impact threat. Concurrently with dedicated observational projects, searches for small bodies have been performed on numerous archi v al data sets from different facilities. Here, we present a framework to increase the scientific return of an exoplanet transit-search survey by recovering serendipitous detections of small bodies in its daily and archi v al data using a GPU-based synthetic tracking algorithm. As a proof of concept, we analysed 12 x 12 arcmin(2) sky fields observed by the 1-m telescopes of the SPECULOOS surv e y. We analysed 90 sky fields distributed uniformly across the sky as part of the daily search for small bodies and 21 archi v al fields located within 5 deg from the ecliptic plane as part of the archi v al search (4.4 deg(2) in total). Overall, we identified 400 known objects of different dynamical classes from Inner Main-belt Asteroids to Jupiter Trojans and 43 potentially new small bodies with no priors on their motion. We were able to reach limiting magnitude for unknown objects of V = 23.8 mag, and a retrie v al rate of similar to 80 per cent for objects with V < 22 mag and V < 23.5 mag for the daily and archi v al searches, respectively. SPECULOOS and similar exoplanet surveys can thus serve as pencil-beam surveys for small bodies and probe parameter space beyond V = 22 mag.