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Journal articles
The Extinction Properties of and Distance to the Highly Reddened Type Ia Supernova SN 2012cu
X. Huang
Z. Raha
G. Aldering
P. Antilogus
1
S. Bailey
C. Baltay
K. Barbary
D. Baugh
K. Boone
S. Bongard
1
C. Buton
2
Jie Chen
N. Chotard
2
Y. Copin
2
P. Fagrelius
H. K. Fakhouri
U. Feindt
D. Fouchez
3
E. Gangler
4
B. Hayden
W. Hillebrandt
A. G. Kim
M. Kowalski
P. -F. Leget
4
S. Lombardo
J. Nordin
R. Pain
1
E. Pecontal
5
R. Pereira
2
S. Perlmutter
D. Rabinowitz
M. Rigault
D. Rubin
K. Runge
C. Saunders
G. Smadja
2
C. Sofiatti
A. Stocker
N. Suzuki
S. Taubenberger
C. Tao
3
R. C. Thomas
K. Boone
Author
S. Bongard 1
Author
C. Buton 2
Author
Jie Chen
Author Employer institution : City University of Hong Kong [Hong Kong]
N. Chotard 2
Author
Y. Copin 2
Mail :
Author IdHAL : yannick-copin arXiv : https://arxiv.org/a/ycopin ResearcherId : http://www.researcherid.com/rid/B-4928-2015 ORCID : https://orcid.org/0000-0002-5317-7518
P. Fagrelius
Author
H. K. Fakhouri
Author
C. Tao 3
Author
R. C. Thomas
Author
1
LPNHE - Laboratoire de Physique Nucléaire et de Hautes Énergies (Barre 12-22, 1er étage 4 Place Jussieu 75252 Paris Cedex 05 - France)
- UPMC - Université Pierre et Marie Curie - Paris 6 (4 place Jussieu - 75005 Paris - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- UPD7 - Université Paris Diderot - Paris 7 (5 rue Thomas-Mann - 75205 Paris cedex 13 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR7585 (France)
2
IPNL - Institut de Physique Nucléaire de Lyon (Campus LyonTech-la Doua
Bâtiment Paul DIRAC
4 Rue Enrico Fermi
69622 Villeurbanne Cedex - France)
- CNRS - Centre National de la Recherche Scientifique : UMR5822 (France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- UCBL - Université Claude Bernard Lyon 1 (43, boulevard du 11 novembre 1918, 69622 Villeurbanne cedex - France)
- Université de Lyon (92 rue Pasteur - CS 30122, 69361 Lyon Cedex 07 - France)
3
CPPM - Centre de Physique des Particules de Marseille (163, avenue de Luminy - Case 902 - 13288 Marseille cedex 09 - France)
- AMU - Aix Marseille Université : UMR7346 (Aix-Marseille Université Jardins du Pharo 58 Boulevard Charles Livon 13284 Marseille cedex 7 - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- CNRS - Centre National de la Recherche Scientifique : UMR7346 (France)
4
LPC - Laboratoire de Physique Corpusculaire - Clermont-Ferrand (Campus des Cézeaux / 24 avenue des Landais / BP 80026 / 63171 Aubière Cedex - France)
- UBP - Université Blaise Pascal - Clermont-Ferrand 2 (34, avenue Carnot - BP 185 / 63006 Clermont-Ferrand cedex - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- CNRS - Centre National de la Recherche Scientifique : UMR6533 (France)
5
CRAL - Centre de Recherche Astrophysique de Lyon (9 Avenue Charles André 69561 ST GENIS LAVAL CEDEX - France)
- CNRS - Centre National de la Recherche Scientifique : UMR5574 (France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- UCBL - Université Claude Bernard Lyon 1 (43, boulevard du 11 novembre 1918, 69622 Villeurbanne cedex - France)
- Université de Lyon (92 rue Pasteur - CS 30122, 69361 Lyon Cedex 07 - France)
- ENS Lyon - École normale supérieure - Lyon (15 parvis René Descartes - BP 7000 - 69342 Lyon Cedex 07 - France)
Abstract : Correction of Type Ia Supernova brightnesses for extinction by dust has proven to be a vexing problem. Here we study the dust foreground to the highly reddened SN 2012cu, which is projected onto a dust lane in the galaxy NGC 4772. The analysis is based on multi-epoch, spectrophotometric observations spanning 3,300 - 9,200 {\AA}, obtained by the Nearby Supernova Factory. Phase-matched comparison of the spectroscopically twinned SN 2012cu and SN 2011fe across 10 epochs results in the best-fit color excess of (E(B-V), RMS) = (1.00, 0.03) and total-to-selective extinction ratio of (RV , RMS) = (2.95, 0.08) toward SN 2012cu within its host galaxy. We further identify several diffuse interstellar bands, and compare the 5780 {\AA} band with the dust-to-band ratio for the Milky Way. Overall, we find the foreground dust-extinction properties for SN 2012cu to be consistent with those of the Milky Way. Furthermore we find no evidence for significant time variation in any of these extinction tracers. We also compare the dust extinction curve models of Cardelli et al. (1989), O'Donnell (1994), and Fitzpatrick (1999), and find the predictions of Fitzpatrick (1999) fit SN 2012cu the best. Finally, the distance to NGC4772, the host of SN 2012cu, at a redshift of z = 0.0035, often assigned to the Virgo Southern Extension, is determined to be 16.6$\pm$1.1 Mpc. We compare this result with distance measurements in the literature.
Document type :
Journal articles
Complete list of metadatas
http://hal.in2p3.fr/in2p3-01430546
Contributor : Sylvie Flores <>
Submitted on : Tuesday, January 10, 2017 - 8:36:05 AM
Last modification on : Saturday, April 11, 2020 - 1:53:32 AM
Contributor : Sylvie Flores <>
Submitted on : Tuesday, January 10, 2017 - 8:36:05 AM
Last modification on : Saturday, April 11, 2020 - 1:53:32 AM
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Identifiers
- HAL Id : in2p3-01430546, version 1
- ARXIV : 1701.01422
- DOI : 10.3847/1538-4357/836/2/157
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Citation
X. Huang, Z. Raha, G. Aldering, P. Antilogus, S. Bailey, et al.. The Extinction Properties of and Distance to the Highly Reddened Type Ia Supernova SN 2012cu. The Astrophysical Journal, American Astronomical Society, 2017, 836, pp.157. ⟨10.3847/1538-4357/836/2/157⟩. ⟨in2p3-01430546⟩
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