The local and global properties of different types of supernova host
  galaxies
  By using Data Analysis Pipeline (DAP) products of Mapping Nearby Galaxies at
Apache Point Observatory (MaNGA), which are publicly available from the SDSS
Data Release 15, we analyze the local properties at the SN explosion sites and
global properties of different types of SN host galaxies to explore the
explosion environments of different types of SNe. In our sample, there are 67
SN host galaxies in the field of view of MaNGA, including 32 Type Ia, 29 CCSNe,
1 super-luminous SN (SLSN), 1 Type I and 4 unclassified type of SNe, with which
we can perform the K-S test for analysis and derive statistically robust
results. Due to the limited sample size, we couldn't remove the mass dependence
in this work, which is likely the true driver of the trends for the properties
presented in this work. The global star formation rate (SFR) and EW(H$\alpha$)
for SN Ia hosts is slightly lower than that for CCSN hosts on average. SN Ia
host galaxies are $\sim$ 0.3 dex more massive than CCSN hosts, which implies
that the number ratio of CCSNe to Type Ia SNe will decrease with the increasing
of stellar mass of host galaxies. The stellar population age of SN Ia host
galaxies is older than that of CCSN hosts on average. There is no significant
difference between different types of SN hosts for some properties, including
local SFR density ($\Sigma \rm SFR$), local and global gas-phase oxygen
abundance. For most galaxies in our sample, the global gas-phase oxygen
abundance estimated from the integrated spectra of SN hosts can represent the
local gas-phase oxygen abundance at the SN explosion sites with small bias.
