Resumen
We used optical Integral Field Spectroscopy of nearby supernova (SN) host galaxies to look for correlations in the environmental parameters at the location of different SN types. Our sample consists of 47 galaxies observed by the Calar Alto Legacy Integrated Field Area (CALIFA) Survey, complemented with other 24 previously observed with the same instrument. We updated the analysis tools implemented in our pilot study (Stanishev et al. 2012) to derive stellar population and ionized gas parameters from the 3D datacubes. According to our results SNe Ib/c explode closer to the galactic core and are more associated with HII regions than SNe II. SNe Ia occur on average farther from the center of the galaxy and are associated with regions with lower current star formation and older stellar populations.
