  We investigate the impact of a presumed axion-like-particle (ALP) emission in
a core-collapse supernova explosion on neutrino luminosities and mean energies
employing a relatively simple analytic description. We compute the nuclear
Bremsstrahlung and Primakoff axion luminosities as functions of the
protoneutron star (PNS) parameters and discuss how the ALP luminosities compete
with the neutrino emission, modifying the total PNS thermal energy dissipation.
Our results are publicly available in the python package ARtiSANS, which can be
used to compute the neutrino and axion observables for different choices of
parameters.
