Spatially Resolved Properties of Supernova Host Galaxies in SDSS-IV MaNGA

Abstract

We crossmatch galaxies from Mapping Nearby Galaxies at Apache Point Observatory with the Open Supernova Catalog, obtaining a total of 132 SNe within MaNGA bundle. These 132 SNe can be classified into 67 Type Ia and 65 Type CC. We study the global and local properties of supernova host galaxies statistically. Type Ia SNe are distributed in both star-forming galaxies and quiescent galaxies, while Type CC SNe are all distributed along the star-forming main sequence. As the stellar mass increases, the Type Ia/CC number ratio increases. We find: (1) there is no obvious difference in the interaction possibilities and environments between Type Ia SN hosts and a control sample of galaxies with similar stellar mass and SFR distributions, except that Type Ia SNe tend to appear in galaxies which are more bulge-dominated than their controls. For Type CC SNe, there is no difference between their hosts and the control galaxies in galaxy morphology, interaction possibilities as well as environments; (2) the SN locations have smaller velocity dispersion, lower metallicity, and younger stellar population than galaxy centers. This is a natural result of radius gradients of all these parameters. The SN location and the its symmetrical position relative to the galaxy center, as well as regions with similar effective radii have very similar [Mg/Fe], gas-phase metallicity, gas velocity dispersion and stellar population age.

arXiv comment16 pages, 11 figures, Accepted for publication in Research in Astronomy and Astrophysics

References in corpus (45)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• The physical properties of star forming galaxies in the low redshift universe
• Stellar Masses and Star Formation Histories for 10^5 Galaxies from the Sloan Digital Sky Survey
• The 2.5 m Telescope of the Sloan Digital Sky Survey
• Parametric Recovery of Line-of-Sight Velocity Distributions from Absorption-Line Spectra of Galaxies via Penalized Likelihood
• The Formation of Galactic Disks
• Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
• Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
• Using Strong Lines to Estimate Abundances in Extragalactic HII Regions and Starburst Galaxies
• The Multi-Object, Fiber-Fed Spectrographs for SDSS and the Baryon Oscillation Spectroscopic Survey
• Differential Galaxy Evolution in Cluster and Field Galaxies at z=0.3
• WISeREP - An Interactive Supernova Data Repository
• Galaxy Zoo 2: detailed morphological classifications for 304,122 galaxies from the Sloan Digital Sky Survey
• The supernova rate per unit mass
• The MaNGA Integral Field Unit Fiber Feed System for the Sloan 2.5 m Telescope
• The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey
• An Open Catalog for Supernova Data
• Improving galaxy morphologies for SDSS with Deep Learning
• SDSS-IV MaNGA IFS Galaxy Survey --- Survey Design, Execution, and Initial Data Quality
• The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Overview
• Berkeley Supernova Ia Program I: Observations, Data Reduction, and Spectroscopic Sample of 582 Low-Redshift Type Ia Supernovae
• New Strong Line Abundance Diagnostics for \HII Regions: Effects of $\kappa$-Distributed Electron Energies and New Atomic Data
• Chemical abundances in high-redshift galaxies: A powerful new emission line diagnostic
• A Search for Environmental Effects on Type Ia Supernovae
• The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Emission-Line Modeling
• Optical and Infrared Spectroscopy of SN 1999ee and SN 1999ex
• An Explanation for the Observed Weak Size Evolution of Disk Galaxies
• Chemistry and Star Formation in the Host Galaxies of Type Ia Supervovae
• The Asiago Supernova Catalogue- 10 years after
• Optical Spectroscopy of Type Ia Supernovae
• SDSS-IV MaStar -- A Large and Comprehensive Empirical Stellar Spectral Library: First Release
• PISCO: The Pmas/ppak Integral-field Supernova hosts COmpilation
• Nearby supernova host galaxies from the CALIFA Survey: I. Sample, data analysis, and correlation to star-forming regions
• SDSS-IV MaNGA PyMorph Photometric and Deep Learning Morphological Catalogs and implications for bulge properties and stellar angular momentum
• Type II supernova energetics and comparison of light curves to shock-cooling models
• SDSS-IV MaNGA: stellar population gradients as a function of galaxy environment
• Comparisons of the radial distributions of core-collapse supernovae with those of young and old stellar populations
• Type Ia Supernova Properties as a Function of the Distance to the Host Galaxy in the SDSS-II SN Survey
• Hide-and-Seek with the Fundamental Metallicity Relation
• SDSS-IV MaNGA: Variations in the N/O -- O/H relation bias metallicity gradient measurements
• Type Ia Supernova host galaxies as seen with IFU spectroscopy
• Comparing the Host Galaxies of Type Ia, Type II and Type Ibc Supernovae
• The local properties of supernova explosions and their host galaxies
• The local and global properties of different types of supernova host galaxies