Notes. For each light curve anumerical “ID” is listed, then the Universal Time (UT) “Date” at the beginning of the night is given as well as the heliocentric (R_h) and geocentric (Δ) distances measured in AU, the solar phase angle (α), the observer centred ecliptic longitude (λ_O), the observer centred ecliptic latitude (β_O), “Total” length of the light curve, the apparent peak-to-peak “Amplitude”, and the “Observing facility” used to obtain the light curve. Where applicable a “Reference” to the already published work is given. Each line represents a single light curve (sometimes a few segments were observed on a single night). Circles in the “LC-only model” and “LC+radar model” columns indicate which light curves were selected for the light-curve-only and combined light curve and radar shape modelling, respectively, see Sects. 2.1 and 3. A subset of light curves used for the development of the “LC-only model” was selected for the rotational phase and observing geometry coverage, and S/N. For the “LC+radar model” we used only a few of the light curves closest to the radar observing dates. All of the light-curve data available were used for measuring phase offsets in the final stage of the spin-state analysis discussed in Sect. 4. Observing facility key (with MPC site code): (INT, 950), 2.5 m Isaac Newton Telescope, La Palma, Spain; (NTT, 809), European Southern Observatory 3.5 m New Technology Telescope, Chile; (PDS, U82), Palmer Divide Station, California, USA; (TMO, 673), Table Mountain Observatory, California, USA.

References. (1) Warner (2014); (2) Warner (2015).