  The data of 8,852 and 2,927 variable stars detected by OGLE survey in the
Large and Small Magellanic Clouds are presented. They are cross-identified with
the SIRIUS JHK survey data, and their infrared properties are discussed.
Variable red giants are well separated on the period-J - K plane, suggesting
that it could be a good tool to distinguish their pulsation mode and type.
