  The evolutionary pathways of core-collapse supernova progenitors at the
low-mass end of the spectrum are beset with major uncertainties. In recent
years, a variety of evolutionary channels has been discovered in addition to
the classical electron capture supernova channel of super-AGB stars. The few
available progenitor models at the low-mass end have been studied with great
success in supernova simulations as the peculiar density structure makes for
robust neutrino-driven explosions in this mass range. Detailed nucleosynthesis
calculations have been conducted both for models of electron capture supernovae
and low-mass iron core supernovae and revealed an interesting production of the
lighter trans-iron elements (such as Zn, Sr, Y, Zr) as well as rare isotopes
like Ca-48 and Fe-60. We stress the need to explore the low-mass end of the
supernova spectrum further and link various observables to understand the
diversity of explosions in this regime.
