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The dependence of Type Ia supernovae luminosities on their host galaxies

The dependence of Type Ia supernovae luminosities on their host galaxies
The dependence of Type Ia supernovae luminosities on their host galaxies
Precision cosmology with Type Ia supernovae (SNe Ia) makes use of the fact that SN Ia luminosities depend on their light-curve shapes and colours. Using Supernova Legacy Survey (SNLS) and other data, we show that there is an additional dependence on the global characteristics of their host galaxies: events of the same light-curve shape and colour are, on average, 0.08 mag (?4.0?) brighter in massive host galaxies (presumably metal-rich) and galaxies with low specific star formation rates (sSFR). These trends do not depend on any assumed cosmological model, and are independent of the SN light-curve width: both fast and slow-declining events show the same trends. SNe Ia in galaxies with a low sSFR also have a smaller slope (‘?’) between their luminosities and colours with ?2.7? significance, and a smaller scatter on SN Ia Hubble diagrams (at 95 per cent confidence), though the significance of these effects is dependent on the reddest SNe. SN Ia colours are similar between low-mass and high-mass hosts, leading us to interpret their luminosity differences as an intrinsic property of the SNe and not of some external factor such as dust. If the host stellar mass is interpreted as a metallicity indicator using galaxy mass–metallicity relations, the luminosity trends are in qualitative agreement with theoretical predictions. We show that the average stellar mass, and therefore the average metallicity, of our SN Ia host galaxies decreases with redshift. The SN Ia luminosity differences consequently introduce a systematic error in cosmological analyses, comparable to the current statistical uncertainties on parameters such as w, the equation of state of dark energy. We show that the use of two SN Ia absolute magnitudes, one for events in high-mass (metal-rich) galaxies and the other for events in low-mass (metal-poor) galaxies, adequately corrects for the differences. Cosmological fits incorporating these terms give a significant reduction in ?2 (3.8?–4.5?); linear corrections based on host parameters do not perform as well. We conclude that all future SN Ia cosmological analyses should use a correction of this (or similar) form to control demographic shifts in the underlying galaxy population.
0035-8711
782-802
Sullivan, M.
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Conley, A.
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Howell, D.A.
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Neill, J.D.
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Astier, P.
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Balland, C.
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Basa, S.
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Carlberg, R.G.
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Fouchez, D.
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Guy, J.
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Hardin, D.
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Hook, I.M.
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Pain, R.
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Palanque-Delabrouille, N.
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Perrett, K.M.
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Pritchet, C.J.
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Regnault, N.
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Rich, J.
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Ruhlmann-Kleider, V.
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Baumont, S.
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Hsiao, E.
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Kronborg, T.
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Lidman, C.
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Perlmutter, S.
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Walker, E.S.
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Sullivan, M.
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Conley, A.
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Howell, D.A.
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Neill, J.D.
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Astier, P.
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Balland, C.
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Basa, S.
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Carlberg, R.G.
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Fouchez, D.
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Guy, J.
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Hardin, D.
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Hook, I.M.
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Pain, R.
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Palanque-Delabrouille, N.
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Perrett, K.M.
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Pritchet, C.J.
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Regnault, N.
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Rich, J.
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Ruhlmann-Kleider, V.
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Baumont, S.
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Hsiao, E.
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Kronborg, T.
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Lidman, C.
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Perlmutter, S.
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Walker, E.S.
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Sullivan, M., Conley, A., Howell, D.A., Neill, J.D., Astier, P., Balland, C., Basa, S., Carlberg, R.G., Fouchez, D., Guy, J., Hardin, D., Hook, I.M., Pain, R., Palanque-Delabrouille, N., Perrett, K.M., Pritchet, C.J., Regnault, N., Rich, J., Ruhlmann-Kleider, V., Baumont, S., Hsiao, E., Kronborg, T., Lidman, C., Perlmutter, S. and Walker, E.S. (2010) The dependence of Type Ia supernovae luminosities on their host galaxies. Monthly Notices of the Royal Astronomical Society, 406 (2), 782-802. (doi:10.1111/j.1365-2966.2010.16731.x).

Record type: Article

Abstract

Precision cosmology with Type Ia supernovae (SNe Ia) makes use of the fact that SN Ia luminosities depend on their light-curve shapes and colours. Using Supernova Legacy Survey (SNLS) and other data, we show that there is an additional dependence on the global characteristics of their host galaxies: events of the same light-curve shape and colour are, on average, 0.08 mag (?4.0?) brighter in massive host galaxies (presumably metal-rich) and galaxies with low specific star formation rates (sSFR). These trends do not depend on any assumed cosmological model, and are independent of the SN light-curve width: both fast and slow-declining events show the same trends. SNe Ia in galaxies with a low sSFR also have a smaller slope (‘?’) between their luminosities and colours with ?2.7? significance, and a smaller scatter on SN Ia Hubble diagrams (at 95 per cent confidence), though the significance of these effects is dependent on the reddest SNe. SN Ia colours are similar between low-mass and high-mass hosts, leading us to interpret their luminosity differences as an intrinsic property of the SNe and not of some external factor such as dust. If the host stellar mass is interpreted as a metallicity indicator using galaxy mass–metallicity relations, the luminosity trends are in qualitative agreement with theoretical predictions. We show that the average stellar mass, and therefore the average metallicity, of our SN Ia host galaxies decreases with redshift. The SN Ia luminosity differences consequently introduce a systematic error in cosmological analyses, comparable to the current statistical uncertainties on parameters such as w, the equation of state of dark energy. We show that the use of two SN Ia absolute magnitudes, one for events in high-mass (metal-rich) galaxies and the other for events in low-mass (metal-poor) galaxies, adequately corrects for the differences. Cosmological fits incorporating these terms give a significant reduction in ?2 (3.8?–4.5?); linear corrections based on host parameters do not perform as well. We conclude that all future SN Ia cosmological analyses should use a correction of this (or similar) form to control demographic shifts in the underlying galaxy population.

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Published date: 1 August 2010
Organisations: Astronomy Group

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Local EPrints ID: 350437
URI: https://eprints.soton.ac.uk/id/eprint/350437
ISSN: 0035-8711
PURE UUID: ad07215d-14e0-4e7f-b47f-f3e4cd4eae86
ORCID for M. Sullivan: ORCID iD orcid.org/0000-0001-9053-4820

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Date deposited: 26 Mar 2013 16:46
Last modified: 07 Aug 2019 00:34

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Contributors

Author: M. Sullivan ORCID iD
Author: A. Conley
Author: D.A. Howell
Author: J.D. Neill
Author: P. Astier
Author: C. Balland
Author: S. Basa
Author: R.G. Carlberg
Author: D. Fouchez
Author: J. Guy
Author: D. Hardin
Author: I.M. Hook
Author: R. Pain
Author: N. Palanque-Delabrouille
Author: K.M. Perrett
Author: C.J. Pritchet
Author: N. Regnault
Author: J. Rich
Author: V. Ruhlmann-Kleider
Author: S. Baumont
Author: E. Hsiao
Author: T. Kronborg
Author: C. Lidman
Author: S. Perlmutter
Author: E.S. Walker

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