  We study the dynamics of the quintom dark energy model using state-of-the-art
cosmological observations. The set of equations has been converted into an
autonomous system using suitable transformations of the variables. We have
discussed the fixed points of the model and the general phase-space behavior,
in particular, in finding the existence of the tracker solutions for this
model. The observations suggest that at late times the phantom field should
dominate the dark energy sector with an approximately 15% share to the
quintessence counterpart, and with both fields tracking the background at early
times. A Bayesian model comparison with LambdaCDM has also been done by
computing the Bayes factor and a positive preference has been obtained for the
quintom model. Although not fully resolved, the Hubble tension can be reduced
to 2.6{\sigma} when compared with the value of H0 reported in [1] and to
1.6{\sigma} when compared with that of [2].
