The upcoming 4-m International Liquid Mirror Telescope (ILMT) facility will
perform deep imaging (in single scan g′∼22 mag.) of a narrow strip of
sky each clear night in the Time Delayed Integration mode. A cadence of one day
observation will provide unique opportunities to discover different types of
supernovae (SNe) along with many other types of variable sources. We present
the approach to discover SNe with the ILMT and discuss the follow-up strategy
in the context of other existing observational facilities. The advantages of
the ILMT observations over the traditional glass mirror telescopes are also
discussed.Comment: 8 pages, 3 figures, to appear in proceedings of the First
Belgo-Indian Network for Astronomy & Astrophysics (BINA) Worksho