  The 4m International Liquid Mirror Telescope (ILMT) facility continuously
scans the same sky strip ($\sim$22$^\prime$ wide) on each night with a fixed
pointing towards the zenith direction. It is possible to detect hundreds of
supernovae (SNe) each year by implementing an optimal image subtraction
technique on consecutive night images. Prompt monitoring of ILMT-detected SNe
is planned under the secured target of opportunity mode using ARIES telescopes
(1.3m DFOT and 3.6m DOT). Spectroscopy with the DOT facility will be useful for
the classification and detailed investigation of SNe. During the commissioning
phase of the ILMT, supernova (SN) 2023af was identified in the ILMT field of
view. The SN was further monitored with the ILMT and DOT facilities.
Preliminary results based on the light curve and spectral features of SN 2023af
are presented.
