“…Our spectroscopic identifications were used by other groups to (i) build the luminosity function of BL Lacs (Ajello et al, 2013); (ii) select potential targets for the Cherenkov Telescope Array (CTA; Arsioli et al, 2015); (iii) obtain stringent limits on the dark matter annihilation in sub-halos (e.g., Berlin et al, 2014); (iv) search for counterparts of new flaring γ-ray sources (Bernieri et al, 2013); (v) test new γ-ray detection algorithms (Campana et al, 2016); (vi) perform population studies on the UGSs (e.g., Acero et al, 2013) and (vii) discover the new subclass of radio weak BL Lacs (e.g., Massaro et al, 2017). All the above studies confirm the legacy value of our results thus motivating the prosecution of our BCU follow up campaign.…”