Notes. The full version of the table is available in electronic form at the CDS. The albedos were computed from the absolute asteroid magnitudes H taken from Oszkiewicz et al. (2011). Entries with “True” in the “Fit” column indicate that the beaming parameter was fitted; otherwise, the value was computed from Eq. (1). On the other hand, the diameters were always fitted. Columns n₉ and n₁₈ refer to the number of observationsfitted in the 9-μm and 18-μ bands, and r, Δ, and α are the heliocentric and geocentric distances and phase angle, respectively. MJD is the modified Julian date of the last observation of the group. Typical minimum uncertainties are higher when the beaming parameter could not be fitted, as discussed in the main text.