  Currently, 6 out of 30 known magnetars had pulsed radio emission detected. In
this work, we evaluated the possibility of detecting radio transient events
from magnetars with the telescopes of the Instituto Argentino de
Radioastronom\'ia (IAR). To this aim, we made daily observations of the
magnetar XTE~J1810$-$197 from 02-Sep-22 to 30-Nov-22.
  We analysed the observations by applying ephemeris folding and single pulse
searches. We fitted a timing model to our observations and were able to detect
the magnetar on 6 of the 36 observing sessions with signal-to-noise ratios at
the limit of detectability, $3.3\leq \mathrm{S/N} \leq4.1$. We searched for
individual 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 slightly
between 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 detect
pulsed radio emission in the band of $1400-1456\, \mathrm{MHz}$ from magnetars
with a time resolution of $146\,\mu s$, being able to detect both integrated
pulse profiles and individual pulses.
