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We present the Pmas/ppak Integral-field Supernova hosts COmpilation (PISCO)which comprises Integral Field Spectroscopy (IFS) of 232 supernova (SN) hostgalaxies, that hosted 272 SNe, observed over several semesters with the 3.5mtelescope at the Calar Alto Observatory (CAHA). PISCO is the largest collectionof SN host galaxies observed with wide-field IFS, totaling 466,347 individualspectra covering a typical spatial resolution of $\sim$380 pc. While focusedstudies regarding specific SN Ia- related topics will be published elsewhere,this paper aims to present the properties of the SN environments with stellarpopulation (SP) synthesis and the gas-phase ISM, providing additional resultsseparating stripped-envelope SNe into their subtypes. With 11,270 HII regionsdetected in all galaxies, we present for the first time an HII regionstatistical analysis, that puts HII regions that have hosted SNe in contextwith all other SF clumps within their galaxies. SNe Ic are associated to moremetal-rich, higher EW(H{\alpha}) and higher SF rate environments within theirhost galaxies than the mean of all HII regions detected within each host, oncontrary SNe IIb occur at the most different environments compared to other CCSNe types. We find two clear components of young and old SP at SNe IInlocations. We find that SNe II fast-decliners (IIL) tend to explode atlocations where {\Sigma}SFR is more intense. Finally, we outline how a futurededicated IFS survey of galaxies in parallel to an untargeted SN search wouldovercome the biases in current environmental studies.

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