  We present observations and analysis of SN 2020cxd, a Low luminous (LL),
long-lived Type IIP SN. This object was a clear outlier in the
magnitude-limited SN sample recently presented by the ZTF Bright Transient
Survey. We demonstrate that SN 2020cxd is an additional member of the group of
LL SNe, and discuss the rarity of LL SNe in the context of the ZTF survey, and
how further studies of these faintest members of the CC SN family might help
understand the underlying initial mass function for stars that explode.
