Number of SNe as a function of stellar mass (left) and SFR (right) considering the entire parent sample, colored by galaxy distance and considering galaxy integrated properties measured only within the MUSE field of view. These SN counts can also directly be converted to a SN frequency by assuming SNRs are visible in the optical for 10 000 yr. Lines of constant SN rate per unit mass (SNu) are also shown. The star markers represent the number for the parent sample while the circles are the number of SNRs. The line between them shows the range of possible true SNR numbers.