“…Many REases with star activity have been reported: AvaI (14), BamHI (15–20), BanI (21), Bme126I (22), BmrI (23), BspLU111III (24), BstI (25), BsuRI (26), BtsI (27), CeqI (28), CviJI (29,30), EcoRI (12,31–39), EcoRV (40–42), HaeIII (14), HhaI (20), HindIII (13,33,43), HinfI (44,45), KpnI (46), MamI (47), MboII (48), NcuI (49), NotI (50), PpiI (51), PstI (14,20,52), PvuII (17,43,53,54), RsrI (55,56), SacI (43), SalI (20), Sau3AI (57), SgrAI (58), SphI (59), SstI (20), TaqI (60–62), Tth111I (63) and XbaI (14,20). Experimentally, it has been found that the following general conditions may increase star activity: high glycerol concentration (>5% v/v) (18–20,34), high enzyme to DNA ratio (usually >100 U of enzyme per microgram of DNA) (12,17,20,34), low ionic strength (<25 mM salt) (12,17,20,34,35), high pH (>8.0) (41), the presence of organic solvents (such as DMSO, ethanol) (20,34,43) and substitution of Mg 2+ with other divalent cations (Mn 2+ , Co 2+ ) (15,33–35,64). It has been suggested that water-mediated interactions between the REase and DNA are the key differences between specific complexes and star complexes (17,38,65), but the actual situation may be even more complicated and remains to be clarified.…”