Rotation period and pole direction distributions. Left: Normalized period distributions for the ASAS-SN models (760), TESS periods (9912, Pál et al. 2020), and LCDB periods (31 280, Warner et al. 2009). Middle: distribution of pole ecliptic longitudes λ for all asteroids and asteroids > 100 km derived from the ASAS-SN data. Right: distribution of orbital pole latitudes β_orb derived from ASAS-SN data for asteroids smaller than 30 km and for asteroids larger than 100 km.