Notes. The observational material for the determination of osculating orbits is described in Cols. [4]−[8] and [11], and Col. [9] gives Q^* (see KD13) for the GR model of motion, and the resulting orbit quality assessment (orbital class) is given in Col. [10]. The second and third columns show an osculating perihelion distance and perihelion time. The data distribution relative to a perihelion passage is presented in Cols. [7] and [8], where “pre” (“post”) means that all observations were taken before (after) the perihelion passage; “pre+” (“post+”) means that considerablymore pre-perihelion (post-perihelion) measurements were available, and additional “+” means a drastic dominance of data before (after) perihelion. Column [12] shows references, where “new” means solutions obtained here, MPC – taken from the Minor Planet Center https://www.minorplanetcenter.net/db_search, NK – Nakano Notes, PB – Królikowska & Dybczyński (2016). Values of 1∕a_ori and 1∕a_fut represent original and future semimajor axes of barycentric orbits at the distance of 250 au before entering and after leaving the inner part of the Solar System, respectively. The full table is available at the CDS.