  We describe a survey of nearby core-collapse supernova (SN) explosion sites
using integral field spectroscopy (IFS) technique, which is an extension of the
work described in Kuncarayakti et al. (2013, AJ, 146, 30/31) . The project aims
to constrain the SN progenitor properties based on the study of the SN
immediate environment. The stellar populations present at the SN explosion
sites are studied by means of integral field spectroscopy, which enables the
acquisition of both spatial and spectral information of the object
simultaneously. The spectrum of the SN parent stellar population gives the
estimate of its age and metallicity. With this information, the initial mass
and metallicity of the once coeval SN progenitor star are derived. While the
survey is mostly done in optical, additionally the utilization of near-infrared
integral field spectroscopy assisted with adaptive optics (AO) enables us to
examine the explosion sites in high spatial details, down to a few parsecs.
This work is being carried out using multiple 2-8 m class telescopes equipped
with integral field spectrographs in Chile and Hawaii.
