  We report here on the first results of a systematic monitoring of southern
glitching pulsars at the Argentine Institute of Radioastronomy that started in
the year 2019. We detected a major glitch in the Vela pulsar (PSR J0835$-$4510)
and two small-glitches in PSR J1048$-$5832. For each glitch, we present the
measurement of glitch parameters by fitting timing residuals. We then make an
individual pulses study of Vela in observations before and after the glitch. We
selected 6 days of observations around the major glitch on 2021 July 22 and
study their statistical properties with machine learning techniques. We use
Variational AutoEncoder (VAE) reconstruction of the pulses to separate them
clearly from the noise. We perform a study with Self-Organizing Maps (SOM)
clustering techniques to search for unusual behavior of the clusters during the
days around the glitch not finding notable qualitative changes. We have also
detected and confirm recent glitches in PSR J0742$-$2822 and PSR J1740$-$3015.
