  We present new observations of the cataclysmic variable DW Cancri, after the
system recovered from a low state. We performed a power spectrum analysis that
reveals a clear signal of the 38 min spin period in our photometric data. Our
spectroscopic power spectrum search was consistent with studies performed
before the low state, showing the orbital and spin modulations. We also
conducted a Doppler Tomography study which exhibits a disc structure and an
enhanced emission region, possibly related to a hot spot component. Through a
wavelet transform analysis we also found evidence of the 70 min spin-orbit beat
period. We interpret these results as indication of a partial recovery of the
system. Nonetheless, DW Cnc does not yet show all the original photometric
modulations reported in 2004, before experiencing the low state. Namely, these
signals are a 38 min spin period, an 86 min orbital period, a 70 min beat
period between the latter modulations, and an unresolved 110 min period. Even
though our photometry shows a spin cycle modulation and a long 108 min period,
it lacks the beat and orbital period signals. Thus, we propose further
observations of DW Cancri, to elucidate if the mechanisms giving rise to the
signatures observed prior to the low state, require more time to reactivate.
