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Diversity in extinction laws of Type Ia supernovae measured between 0.2 and 2 mu m
Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC). Stockholm University, Faculty of Science, Department of Physics.
Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC). Stockholm University, Faculty of Science, Department of Physics.
Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC). Stockholm University, Faculty of Science, Department of Physics.
Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC). Stockholm University, Faculty of Science, Department of Physics.
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Number of Authors: 39
2015 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 453, no 3, 3300-3328 p.Article in journal (Refereed) Published
Abstract [en]

We present ultraviolet (UV) observations of six nearby Type Ia supernovae (SNe Ia) obtained with the Hubble Space Telescope, three of which were also observed in the near-IR (NIR) with Wide-Field Camera 3. UV observations with the Swift satellite, as well as ground-based optical and NIR data provide complementary information. The combined data set covers the wavelength range 0.2-2 mu m. By also including archival data of SN 2014J, we analyse a sample spanning observed colour excesses up to E(B - V) = 1.4 mag. We study the wavelength-dependent extinction of each individual SN and find a diversity of reddening laws when characterized by the total-to-selective extinction R-V. In particular, we note that for the two SNe with E(B - V) greater than or similar to 1 mag, for which the colour excess is dominated by dust extinction, we find R-V = 1.4 +/- 0.1 and R-V = 2.8 +/- 0.1. Adding UV photometry reduces the uncertainty of fitted R-V by similar to 50 per cent allowing us to also measure R-V of individual low-extinction objects which point to a similar diversity, currently not accounted for in the analyses when SNe Ia are used for studying the expansion history of the Universe.

Place, publisher, year, edition, pages
2015. Vol. 453, no 3, 3300-3328 p.
Keyword [en]
circumstellar matter, supernovae: general, supernovae: individual: SNe 2012cg, supernovae: individual: 2012cu, dust, extinction
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Physical Sciences
Identifiers
URN: urn:nbn:se:su:diva-123790DOI: 10.1093/mnras/stv1505ISI: 000363649000085OAI: oai:DiVA.org:su-123790DiVA: diva2:944924
Available from: 2016-06-30 Created: 2015-12-07 Last updated: 2016-06-30Bibliographically approved

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Amanullah, RahmanJohansson, JoelGoobar, ArielFerretti, RaphaelPapadogiannakis, SeméliPetrushevska, TanjaHangard, LauraLundqvist, PeterSandberg, AndreasTaddia, FrancescoÖstlin, GöranAsadi, Saghar
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The Oskar Klein Centre for Cosmo Particle Physics (OKC)Department of PhysicsDepartment of Astronomy
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Monthly notices of the Royal Astronomical Society
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