Notes. Osculating heliocentric orbital elements at epoch MJD 60,000.0 from the MPC catalog: semimajor axis a, eccentricity e, inclination I, longitude of node Ω, and argument of perihelion ω. singleopposition orbits are listed at the end of the table. The third column gives the absolute magnitude H. The last column indicates, whether the asteroid has been detected by CSS during the phase 2 operations (Y=yes). We note two very small, singleopposition asteroids 2016 PL51 and 2022 RB57, very likely members of the Datura family too. However, their orbits, based on observations spanning short arcs (less than a week in the case of 2016 PL51), are still very uncertain. We include (429988) 2013 PZ36 residing on a rather chaotic orbit (most likely interacting with the exterior E3/10 mean motion resonance with the Earth), such that proving its membership to the Datura family would require an extensive work beyond the scope of this paper (see also Fig. 1). Luckily, the results discussed in Sect. 4 are not overly sensitive to the decision about Datura membership of this body.