PISCO: The Pmas/ppak Integral-field Supernova hosts COmpilation

摘要: We present the Pmas/ppak Integral-field Supernova hosts COmpilation (PISCO) which comprises Integral Field Spectroscopy (IFS) of 232 supernova (SN) host galaxies, that hosted 272 SNe, observed over several semesters with 3.5m telescope at Calar Alto Observatory (CAHA). PISCO is largest collection SN galaxies wide-field IFS, totaling 466,347 individual spectra covering a typical spatial resolution $\sim$380 pc. While focused studies regarding specific Ia- related topics will be published elsewhere, this paper aims to properties environments stellar population (SP) synthesis and gas-phase ISM, providing additional results separating stripped-envelope SNe into their subtypes. With 11,270 HII regions detected in all we for first time an region statistical analysis, puts have context other SF clumps within galaxies. Ic are associated more metal-rich, higher EW(H{\alpha}) rate than mean each host, on contrary IIb occur most different compared CC types. find two clear components young old SP IIn locations. II fast-decliners (IIL) tend explode locations where {\Sigma}SFR intense. Finally, outline how future dedicated IFS survey parallel untargeted search would overcome biases current environmental studies.