Notes. Absolute magnitude and slope parameters (H, G) were retrieved from the Minor Planet Center. W1 through W4 indicate the number of observations used in each WISE band. When η could not be fitted, we show the negative value of the default η that we used. We took the geometry of observation for each epoch from the Miriade Ephemeris Generator. “MJD” refers to the modified Julian Date of the first observation, whereas r, Δ and α are the average values of heliocentric and geocentric distances and phase angle of each group of epochs. Minimum relative errors of 10%, 15%, and 20% should be considered for D, η, and p_V when η could be fitted to at least five measurements in bands W3 and W4. Otherwise, the minimum errors for the diameters would be 20% and 40% for the albedos (see Nugent et al. 2016). Here we provide a small set of results to illustrate the format of the full table, which can be downloaded from the CDS.