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Currently, 6 out of 30 known magnetars had pulsed radio emission detected. Inthis work, we evaluated the possibility of detecting radio transient eventsfrom magnetars with the telescopes of the Instituto Argentino deRadioastronom\'ia (IAR). To this aim, we made daily observations of themagnetar XTE~J1810$-$197 from 02-Sep-22 to 30-Nov-22.  We analysed the observations by applying ephemeris folding and single pulsesearches. We fitted a timing model to our observations and were able to detectthe magnetar on 6 of the 36 observing sessions with signal-to-noise ratios atthe limit of detectability, $3.3\leq \mathrm{S/N} \leq4.1$. We searched forindividual pulses in one of these 6 days and found 7 individual pulses with$8.5\leq \mathrm{S/N} \leq18.8$. The dispersion measure changed slightlybetween pulses within a range of $178 \leq \textrm{DM} \,[\mathrm{pc\,cm^{-3}}] \leq 182$. The pulse with $\mathrm{S/N}=18.8$ has an associated$\textrm{DM}$ of $180\,\mathrm{pc\, cm^{-3}}$. We confirmed that we can detectpulsed radio emission in the band of $1400-1456\, \mathrm{MHz}$ from magnetarswith a time resolution of $146\,\mu s$, being able to detect both integratedpulse profiles and individual pulses.

Prospects for Detecting Fast Transients with the Radio Telescopes of the Argentine Institute of Radio Astronomy