  Ram pressure stripping (RPS) is one of the most invoked mechanisms to explain
the observed differences between cluster and field galaxies. In the local
Universe, its effect on the galaxy star forming properties has been largely
tackled and the general consensus is that this process first compresses the gas
available in the galaxy disks, boosting the star formation for a limited amount
of time, and then removes the remaining gas leading to quenching. Much less is
known on the effect and preponderance of RPS at higher redshift, due to the
lack of statistical samples. Exploiting VLT/MUSE observations of galaxies at
0.2<z<0.55 and the catalog of ram pressure stripped galaxies by Moretti et al.,
we compare the global star formation rate-mass (SFR-M*) relation of 29 cluster
galaxies undergoing RPS to that of 26 field and cluster undisturbed galaxies
that constitute our control sample. Stripping galaxies occupy the upper
envelope of the control sample SFR-M* relation, showing a systematic
enhancement of the SFR at any given mass. The boost is >3sigma when considering
the SFR occurring in both the tail and disk of galaxies. The enhancement is
retrieved also on local scales: considering spatially resolved data, ram
pressure stripped galaxies overall have large {\Sigma}SFR values, especially
for Sigma_*>10^7.5M_sun kpc~2. RPS seems to leave the same imprint on the
SFR-M* and Sigma_SFR-Sigma_* relations both in the Local Universe and at
z~0.35.
