  The division between stripped-envelope supernovae (SE-SNe) and superluminous
supernovae (SLSNe) is not well defined in either photometric or spectroscopic
space. While a sharp luminosity threshold has been suggested, there remains an
increasing number of transitional objects that reach this threshold without the
spectroscopic signatures common to SLSNe. In this work we present data and
analysis on four SNe transitional between SE-SNe and SLSNe; the He-poor SNe
2019dwa and 2019cri, and the He-rich SNe 2019hge and 2019unb. Each object
displays long-lived and variable photometric evolution with luminosities around
the SLSN threshold of $M_r < -19.8$ mag. Spectroscopically however, these
objects are similar to SE-SNe, with line velocities lower than either SE-SNe
and SLSNe, and thus represent an interesting case of rare transitional events.
