Same as Fig. 1, but for the ~2270 fainter MB targets, with H between 11 and 13 mag (source: LCDB). There are ~270 large-amplitude targets (from those on the right side of the chart) with available spin and shape model, while only a few low-amplitude targets with a model (left side). Judging from the sample of only those small asteroids that have available shape models, and not taking into consideration the distribution of the amplitudes of all asteroids, can create a false impression that almost all small asteroids are strongly elongated.