Bibcode
                                    
                            Di Cecco, A.; Bono, G.; Monelli, M.; Calamida, A.; Nonino, M.; Stetson, P. B.; Buonanno, R.; Caputo, F.; Corsi, C. E.; Ferraro, I.; Iannicola, G.; Pulone, L.
    Bibliographical reference
                                    Memorie della Società Astronomica Italiana, v.79, p.707 (2008)
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                        2008
            
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                            Description
                                    We present wide-field ground based photometry for the Galactic globular
cluster M92. Data were collected in the SDSS bands (u',g',r',i',z') with
the MegaCam@CFHT. We confirm the occurrence of cluster stars beyond the
tidal radius. Moreover, we find that the ratio between the Horizontal
Branch (HB) stars and Main Sequence (MS) stars across the turn-off
region clearly decreases by a factor of two when moving from the centre
to the outermost regions of the cluster.