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We report the observations of the highly active FRb20201124A with theupgraded Giant Metrewave Radio Telescope at 550-750~MHz. These observations inthe incoherent array mode simultaneously provided an arcsecond localization ofbursts from \rss, the discovery of persistent radio emission associated withthe host galaxy, and the detection of 48 bursts. Using the brightest burst inthe sample ($F= 108~{\rm Jy~ms}$) we find a structure-maximizing dispersionmeasure of $410.8 \pm 0.5~{\rm pc~cm}^{-3}$. We find that our observations arecomplete down to a fluence level of $10~{\rm Jy~ms}$, above which thecumulative burst rate scales as a power-law $R(>\!F) = 10~{\rm hr}^{-1}\left(F/10\mathrm{~Jy~ms}\right)^{\gamma}$ with $\gamma = -1.2 \pm 0.2$. Wefind that the bursts are on average wider than those reported for otherrepeating FRBs. We find that the waiting time between bursts is wellapproximated by an exponential distribution with a mean of $\sim 2.9$ minduring our observations. We searched for periodicities using both a standardFourier domain method and the Fast Folding Algorithm, but found no significantcandidates. We measure bulk spectro-temporal drift rates between $-0.75$ and$-20~{\rm MHz~ms}^{-1}$. Finally, we use the brightest burst to set an upperlimit to the scattering time of 11.1~ms at 550~MHz. The localization ofFRB20201124A adds strength to the proof-of-concept method described in ourearlier work and serves as a potential model for future localizations andfollow-up of repeating FRBs with the uGMRT.

Burst properties of the highly active FRB 20201124A using uGMRT