The three open clusters Be 15, Be 80 and NGC 2192 have been observed using CCD UBV(RI)C photometry at the San Pedro Martir Observatory, Mexico within the framework of our open-cluster survey. The fundamental parameters of interstellar reddening, distance and age have been derived, and also the metallicity for NGC 2192 (solar metallicity has been assumed for the other two).
Cone search capability for table J/MNRAS/401/621/table1 (Standard UBVRI CCD photometry and observing errors for the open cluster Be 15)
Cone search capability for table J/MNRAS/401/621/table2 (Standard UBVRI CCD photometry and observing errors for the open cluster for Be 80)
Cone search capability for table J/MNRAS/401/621/table3 (Standard UBVRI CCD photometry and observing errors for the open cluster for NGC 2192)