  We present results from a systematic search for broad ($\geq$ 400 \kms) \ha\
emission in Integral Field Spectroscopy data cubes of $\sim$1200 nearby
galaxies obtained with PMAS and MUSE. We found 19 unique regions that pass our
quality cuts, four of which match the locations of previously discovered SNe:
one Type IIP, and three Type IIn, including the well-known SN 2005ip. We
suggest that these objects are young Supernova Remnants, with bright and broad
\ha\ emission powered by the interaction between the SN ejecta and dense
circumstellar material. The stellar ages measured at the location of these SNR
candidates are systematically lower by about 0.5 dex than those measured at the
location of core collapse SNe, implying that their progenitors might be shorter
lived and therefore more massive than a typical CC SN progenitor. The methods
laid out in this work open a new window into the study of nearby SNe with
Integral Field Spectroscopy.
