# The local properties of supernova explosions and their host galaxies

## TL;DR

This study investigates the local and global properties of supernova host galaxies using integral field spectroscopy, revealing that most are metal-rich and that supernova types can occur in diverse galactic environments.

## Contribution

It provides detailed 2D maps of host galaxy properties at higher redshifts than previous studies, highlighting the relationship between metallicity, stellar mass, and supernova types.

## Key findings

- Most host galaxies are metal-rich with 12+log(O/H) > 8.5.
- A positive correlation exists between galaxy stellar mass and gas-phase oxygen abundance.
- Both SN Ia and SN II can occur in normal and interacting/merging galaxies.

## Abstract

We aim to understand the properties at the locations of supernova (SN) explosion in their host galaxies and compare with the global properties of the host galaxies. We use the integral field spectrograph (IFS) of Mapping Nearby Galaxies (MaNGA) at Apache Point Observatory (APO) to get the 2D maps of the parameter properties for eleven SN host galaxies. The sample galaxies are analyzed one by one in details on their properties of velocity field, star formation rate, oxygen abundance and stellar mass etc. This sample of SN host galaxies have redshifts around $z$ $\sim$ 0.03, which is higher than those of the previous related works. The higher redshift distribution allows us to obtain the properties of more distant SN host galaxies. Metallicity (gas-phase oxygen abundance) estimated from integrated spectra could represent the local metallicity at SN explosion sites with small bias. All the host galaxies in our sample are metal-rich galaxies (12+log(O/H) $>$ 8.5) except for NGC 6387, which means supernovae (SNe) may be more inclined to explode in rich-metallicity galaxies. There is a positive relation between global gas-phase oxygen abundance and the stellar mass of host galaxies. We also try to compare the differences of the host galaxies between SN Ia and SN II. In our sample, both SNe Ia and SNe II could explode in normal galaxies, while SNe II also could explode in an interactive or merger system, which has star formation in the galaxy.