Metallicity beats sSFR: the connection between superluminous supernova host galaxy environments and the importance of metallicity for their production
Abstract
ABSTRACT We analyse 33 Type I superluminous supernovae (SLSNe) taken from Zwicky Transient Facility (ZTF)’s Bright Transient Survey to investigate the local environments of their host galaxies. We use a spectroscopic sample of galaxies from the Sloan Digital Sky Survey (SDSS) to determine the large-scale environmental density of the host galaxy. Noting that SLSNe are generally found in galaxies with low stellar masses, high star formation rates (SFRs), and low metallicities, we find that SLSN hosts are also rarely found within high-density environments. Only $$3\substack{+9 \\ -1}$$ per cent of SLSN hosts were found in regions with two or more bright galaxies within 2 Mpc. For comparison, we generate a sample of 662 SDSS galaxies matched to the photometric properties of the SLSN hosts. This sample is also rarely found within high-density environments, suggesting that galaxies with properties required for SLSN production favour more isolated environments. Furthermore, we select galaxies within the IllustrisTNG simulation to match SLSN host galaxy properties in colour and stellar mass. We find that the fraction of simulated galaxies in high-density environments quantitatively match the observed SLSN hosts only if we restrict to simulated galaxies with metallicity 12 + log (O/H) ≤ 8.12. In contrast, limiting to only the highest specific star formation rate (sSFR) galaxies in the sample leads to an overabundance of SLSN hosts in high-density environments. Thus, our measurement of the environmental density of SLSN host galaxies appears to break the degeneracy between low metallicity and high sSFR as the driver for SLSN hosts and provides evidence that the most constraining factor on SLSN production is low metallicity.
- Publication Date:
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1992154
- Resource Type:
- Published Article
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 524 Journal Issue: 3; Journal ID: ISSN 0035-8711
- Publisher:
- Oxford University Press
- Country of Publication:
- United Kingdom
- Language:
- English
Citation Formats
Cleland, Cressida, McGee, Sean L., and Nicholl, Matt. Metallicity beats sSFR: the connection between superluminous supernova host galaxy environments and the importance of metallicity for their production. United Kingdom: N. p., 2023.
Web. doi:10.1093/mnras/stad2118.
Cleland, Cressida, McGee, Sean L., & Nicholl, Matt. Metallicity beats sSFR: the connection between superluminous supernova host galaxy environments and the importance of metallicity for their production. United Kingdom. https://doi.org/10.1093/mnras/stad2118
Cleland, Cressida, McGee, Sean L., and Nicholl, Matt. Fri .
"Metallicity beats sSFR: the connection between superluminous supernova host galaxy environments and the importance of metallicity for their production". United Kingdom. https://doi.org/10.1093/mnras/stad2118.
@article{osti_1992154,
title = {Metallicity beats sSFR: the connection between superluminous supernova host galaxy environments and the importance of metallicity for their production},
author = {Cleland, Cressida and McGee, Sean L. and Nicholl, Matt},
abstractNote = {ABSTRACT We analyse 33 Type I superluminous supernovae (SLSNe) taken from Zwicky Transient Facility (ZTF)’s Bright Transient Survey to investigate the local environments of their host galaxies. We use a spectroscopic sample of galaxies from the Sloan Digital Sky Survey (SDSS) to determine the large-scale environmental density of the host galaxy. Noting that SLSNe are generally found in galaxies with low stellar masses, high star formation rates (SFRs), and low metallicities, we find that SLSN hosts are also rarely found within high-density environments. Only $3\substack{+9 \\ -1}$ per cent of SLSN hosts were found in regions with two or more bright galaxies within 2 Mpc. For comparison, we generate a sample of 662 SDSS galaxies matched to the photometric properties of the SLSN hosts. This sample is also rarely found within high-density environments, suggesting that galaxies with properties required for SLSN production favour more isolated environments. Furthermore, we select galaxies within the IllustrisTNG simulation to match SLSN host galaxy properties in colour and stellar mass. We find that the fraction of simulated galaxies in high-density environments quantitatively match the observed SLSN hosts only if we restrict to simulated galaxies with metallicity 12 + log (O/H) ≤ 8.12. In contrast, limiting to only the highest specific star formation rate (sSFR) galaxies in the sample leads to an overabundance of SLSN hosts in high-density environments. Thus, our measurement of the environmental density of SLSN host galaxies appears to break the degeneracy between low metallicity and high sSFR as the driver for SLSN hosts and provides evidence that the most constraining factor on SLSN production is low metallicity.},
doi = {10.1093/mnras/stad2118},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 524,
place = {United Kingdom},
year = {Fri Jul 14 00:00:00 EDT 2023},
month = {Fri Jul 14 00:00:00 EDT 2023}
}
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