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Evidence of environmental dependencies of Type Ia supernovae from the Nearby Supernova Factory indicated by local H alpha

Aldering, G; Antilogus, P; Antilogus, Pierre; Aragon, C; Bailey, S; Baltay, C; Bongard, S; Buton, C; Canto, A; Cellier-Holzem, F; Childress, Michael; Chotard, N; Guy, J; Kim, Alex G; Kowalski, M; Nordin, J; Nugent, Peter; Rabinowitz, David; Scalzo, Richard; Thomas, R. C.; Copin, Y

Description

Context. Use of Type Ia supernovae (SNe Ia) as distance indicators has proven to be a powerful technique for measuring the dark-energy equation of state. However, recent studies have highlighted potential biases correlated with the global properties of th

dc.contributor.authorAldering, G
dc.contributor.authorAntilogus, P
dc.contributor.authorAntilogus, Pierre
dc.contributor.authorAragon, C
dc.contributor.authorBailey, S
dc.contributor.authorBaltay, C
dc.contributor.authorBongard, S
dc.contributor.authorButon, C
dc.contributor.authorCanto, A
dc.contributor.authorCellier-Holzem, F
dc.contributor.authorChildress, Michael
dc.contributor.authorChotard, N
dc.contributor.authorGuy, J
dc.contributor.authorKim, Alex G
dc.contributor.authorKowalski, M
dc.contributor.authorNordin, J
dc.contributor.authorNugent, Peter
dc.contributor.authorRabinowitz, David
dc.contributor.authorScalzo, Richard
dc.contributor.authorThomas, R. C.
dc.contributor.authorCopin, Y
dc.date.accessioned2015-12-13T22:32:58Z
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/75816
dc.description.abstractContext. Use of Type Ia supernovae (SNe Ia) as distance indicators has proven to be a powerful technique for measuring the dark-energy equation of state. However, recent studies have highlighted potential biases correlated with the global properties of th
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.titleEvidence of environmental dependencies of Type Ia supernovae from the Nearby Supernova Factory indicated by local H alpha
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume560
dc.date.issued2013
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB4806
local.type.statusPublished Version
local.contributor.affiliationAldering, G, Lawrence Berkeley National Laboratory
local.contributor.affiliationAntilogus, P, Universite Pierre et Marie Curie Paris
local.contributor.affiliationAntilogus, Pierre, Laboratoire de Physique Nucleaire des Hautes Energies
local.contributor.affiliationAragon, C, Lawrence Berkeley National Laboratory
local.contributor.affiliationBailey, S, Lawrence Berkeley National Laboratory
local.contributor.affiliationBaltay, C, Yale University
local.contributor.affiliationBongard, S, Université Pierre et Marie Curie Paris 6
local.contributor.affiliationButon, C, Universität Bonn
local.contributor.affiliationCanto, A, Université Pierre et Marie Curie Paris 6,
local.contributor.affiliationCellier-Holzem, F, Universite Pierre et Marie Curie Paris
local.contributor.affiliationChildress, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationChotard, N, Université de Lyon
local.contributor.affiliationGuy, J, Universite Pierre et Marie Curie Paris 6
local.contributor.affiliationKim, Alex G, Lawrence Berkeley National Laboratory
local.contributor.affiliationKowalski, M, Universitat Bonn
local.contributor.affiliationNordin, J, Lawrence Berkeley National Laboratory
local.contributor.affiliationNugent, Peter, Lawrence Berkeley National Laboratory
local.contributor.affiliationRabinowitz, David, Yale University
local.contributor.affiliationScalzo, Richard, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationThomas, R. C., Lawrence Berkeley National Laboratory
local.contributor.affiliationCopin, Y, Université de Lyon
local.description.embargo2037-12-31
local.identifier.doi10.1051/0004-6361/201322104
dc.date.updated2015-12-11T09:12:47Z
local.identifier.scopusID2-s2.0-84890081054
local.identifier.thomsonID000328754500066
CollectionsANU Research Publications

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