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:...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Journal article |
| Language: | English |
| Published: |
2010
|
| _version_ | 1797077379606118400 |
|---|---|
| author | Sullivan, M Conley, A Howell, D Neill, J Astier, P Balland, C Basa, S Carlberg, R Fouchez, D Guy, J Hardin, D Hook, I Pain, R Palanque-Delabrouille, N Perrett, K Pritchet, C Regnault, N Rich, J Ruhlmann-Kleider, V Baumont, S Hsiao, E Kronborg, T Lidman, C Perlmutter, S Walker, E |
| author_facet | Sullivan, M Conley, A Howell, D Neill, J Astier, P Balland, C Basa, S Carlberg, R Fouchez, D Guy, J Hardin, D Hook, I Pain, R Palanque-Delabrouille, N Perrett, K Pritchet, C Regnault, N Rich, J Ruhlmann-Kleider, V Baumont, S Hsiao, E Kronborg, T Lidman, C Perlmutter, S Walker, E |
| author_sort | Sullivan, M |
| collection | OXFORD |
| description | 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 (≃4.0σ) 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 ('β') between their luminosities and colours with ∼2.7σ 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 χ2 (3.8σ-4.5σ); 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. © 2010 The Authors. Journal compilation © 2010 RAS. |
| first_indexed | 2024-03-07T00:17:08Z |
| format | Journal article |
| id | oxford-uuid:7b3af623-768f-47d2-a873-cf44294a1d72 |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-07T00:17:08Z |
| publishDate | 2010 |
| record_format | dspace |
| spelling | oxford-uuid:7b3af623-768f-47d2-a873-cf44294a1d722022-03-26T20:49:16ZThe dependence of Type Ia Supernovae luminosities on their host galaxiesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:7b3af623-768f-47d2-a873-cf44294a1d72EnglishSymplectic Elements at Oxford2010Sullivan, MConley, AHowell, DNeill, JAstier, PBalland, CBasa, SCarlberg, RFouchez, DGuy, JHardin, DHook, IPain, RPalanque-Delabrouille, NPerrett, KPritchet, CRegnault, NRich, JRuhlmann-Kleider, VBaumont, SHsiao, EKronborg, TLidman, CPerlmutter, SWalker, EPrecision 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 (≃4.0σ) 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 ('β') between their luminosities and colours with ∼2.7σ 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 χ2 (3.8σ-4.5σ); 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. © 2010 The Authors. Journal compilation © 2010 RAS. |
| spellingShingle | Sullivan, M Conley, A Howell, D Neill, J Astier, P Balland, C Basa, S Carlberg, R Fouchez, D Guy, J Hardin, D Hook, I Pain, R Palanque-Delabrouille, N Perrett, K Pritchet, C Regnault, N Rich, J Ruhlmann-Kleider, V Baumont, S Hsiao, E Kronborg, T Lidman, C Perlmutter, S Walker, E The dependence of Type Ia Supernovae luminosities on their host galaxies |
| title | The dependence of Type Ia Supernovae luminosities on their host galaxies |
| title_full | The dependence of Type Ia Supernovae luminosities on their host galaxies |
| title_fullStr | The dependence of Type Ia Supernovae luminosities on their host galaxies |
| title_full_unstemmed | The dependence of Type Ia Supernovae luminosities on their host galaxies |
| title_short | The dependence of Type Ia Supernovae luminosities on their host galaxies |
| title_sort | dependence of type ia supernovae luminosities on their host galaxies |
| work_keys_str_mv | AT sullivanm thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT conleya thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT howelld thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT neillj thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT astierp thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT ballandc thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT basas thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT carlbergr thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT fouchezd thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT guyj thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT hardind thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT hooki thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT painr thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT palanquedelabrouillen thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT perrettk thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT pritchetc thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT regnaultn thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT richj thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT ruhlmannkleiderv thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT baumonts thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT hsiaoe thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT kronborgt thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT lidmanc thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT perlmutters thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT walkere thedependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT sullivanm dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT conleya dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT howelld dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT neillj dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT astierp dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT ballandc dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT basas dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT carlbergr dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT fouchezd dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT guyj dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT hardind dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT hooki dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT painr dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT palanquedelabrouillen dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT perrettk dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT pritchetc dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT regnaultn dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT richj dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT ruhlmannkleiderv dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT baumonts dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT hsiaoe dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT kronborgt dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT lidmanc dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT perlmutters dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies AT walkere dependenceoftypeiasupernovaeluminositiesontheirhostgalaxies |