Similar to Fig. 9, except that both panels are the predictions for observations with a 1 m class telescope. The upper panel is for a FWHM of 1.2 arcsec, while the lower panel is for a FWHM of 2.0 arcsec. As the quality of the new observations degrades, their contribution to the sample, as well as that using prior information, is displaced to brighter magnitudes. The gain from using the information in the catalog is relevant in both cases at the faintest bins, as in Fig. 9: at 19th magnitude we have 38 objects in the Bayesian scenario, and 25 objects in the parametric approach, i.e., an increase of more than 50% for the upper panel. In the lower panel the increase is even more important: 23 objects in the Bayesian approach and 12 from the catalog (equal to the number from MCR), an increase of ~90%.