Author Correction: The delay of shock breakout due to circumstellar material evident in most type II supernovae

Förster, F.; Moriya, T. J.; Maureira, J. C.; Anderson, J. P.; Blinnikov, S.; Bufano, F.; Cabrera-Vives, G.; Clocchiatti, A.; de Jaeger, T.; Estévez, P. A.; Galbany, L.; González-Gaitán, S.; Gräfener, G.; Hamuy, M.; Hsiao, E. Y.; Huentelemu, P.; Huijse, P.; Kuncarayakti, H.; Martínez, J.; Medina, G.; Olivares E., F.; Pignata, G.; Razza, A.; Reyes, I.; Martín, J. San; Smith, R. C.; Vera, E.; Vivas, A. K.; de Ugarte Postigo, A.; Yoon, S.-C.; Ashall, C.; Fraser, M.; Gal-Yam, A.; Kankare, E.; Le Guillou, L.; Mazzali, P. A.; Walton, N. A.; Young, D. R.

doi:10.1038/s41550-018-0641-7

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Author Correction
Published: 12 November 2018

Author Correction: The delay of shock breakout due to circumstellar material evident in most type II supernovae

Nature Astronomy volume 3, page 107 (2019)Cite this article

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The Original Article was published on 03 September 2018

Correction to: Nature Astronomy https://doi.org/10.1038/s41550-018-0563-4, published online 3 September 2018.

In the version of this Article originally published, the authors Pablo Huijse and Pablo Huentelemu were mistakenly affiliated with the University of California, Berkeley, and their affiliation to the University of Chile was omitted. Pablo Huijse’s affiliation to the Universidad Austral de Chile was also omitted.

Pablo Huijse’s affiliation has now been corrected to: Millennium Institute of Astrophysics, Santiago, Chile; Department of Electrical Engineering, University of Chile, Santiago, Chile; Instituto de Informática, Universidad Austral de Chile, Valdivia, Chile.

Pablo Huentelemu’s affiliation has now been corrected to: Department of Electrical Engineering, University of Chile, Santiago, Chile.

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Authors and Affiliations

Center for Mathematical Modeling, University of Chile, Santiago, Chile
F. Förster, J. C. Maureira, S. González-Gaitán, J. Martínez, J. San Martín & E. Vera
Millennium Institute of Astrophysics, Santiago, Chile
F. Förster, G. Cabrera-Vives, A. Clocchiatti, P. A. Estévez, M. Hamuy, P. Huijse, J. Martínez, F. Olivares E., G. Pignata & I. Reyes
Department of Astronomy, University of Chile, Santiago, Chile
F. Förster, M. Hamuy, J. Martínez, G. Medina, F. Olivares E. & A. Razza
Division of Theoretical Astronomy, National Astronomical Observatory of Japan, National Institutes of Natural Sciences, Tokyo, Japan
T. J. Moriya
European Southern Observatory, Santiago, Chile
J. P. Anderson & A. Razza
Kavli Institute for the Physics and Mathematics of the Universe, University of Tokyo, Tokyo, Japan
S. Blinnikov
Institute for Theoretical and Experimental Physics, Moscow, Russia
S. Blinnikov
All-Russia Research Institute of Automatics, Moscow, Russia
S. Blinnikov
INAF Catania Astrophysical Observatory, Catania, Italy
F. Bufano
Department of Computer Science, University of Concepción, Concepción, Chile
G. Cabrera-Vives
Department of Physics and Astronomy, Universidad Católica de Chile, Santiago, Chile
A. Clocchiatti
Department of Astronomy, University of California, Berkeley, Berkeley, USA
T. de Jaeger
Department of Electrical Engineering, University of Chile, Santiago, Chile
P. A. Estévez, P. Huentelemu, P. Huijse & I. Reyes
Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA, USA
L. Galbany
CENTRA, Instituto Técnico Superior, Universidade de Lisboa, Lisbon, Portugal
S. González-Gaitán
Argelander-Institut fur Astronomie, Bonn, Germany
G. Gräfener
Department of Physics, Florida State University, Tallahassee, FL, USA
E. Y. Hsiao
Instituto de Informática, Universidad Austral de Chile, Valdivia, Chile
P. Huijse
Finnish Centre for Astronomy with ESO, University of Turku, Turku, Finland
H. Kuncarayakti
Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Turku, Finland
H. Kuncarayakti
Departamento de Ciencias Fisicas, Universidad Andres Bello, Santiago, Chile
G. Pignata
Cerro Tololo Interamerican Observatory, La Serena, Chile
R. C. Smith & A. K. Vivas
CSIC Instituto de Astrofísica de Andalucía, Granada, Spain
A. de Ugarte Postigo
Dark Cosmology Centre, Niels Borh Institute, University of Copenhagen, Copenhagen, Denmark
A. de Ugarte Postigo
Department of Physics and Astronomy, Seoul National University, Seoul, Republic of Korea
S.-C. Yoon
Monash Centre for Astrophysics, School of Physics and Astronomy, Monash University, Melbourne, Australia
S.-C. Yoon
Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK
C. Ashall & P. A. Mazzali
School of Physics, O’Brien Centre for Science, University College Dublin, Dublin, Ireland
M. Fraser
Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel
A. Gal-Yam
Astrophysics Research Centre, School of Mathematics and Physics, Queens University Belfast, Belfast, UK
E. Kankare & D. R. Young
Sorbonne Université, Université Paris Diderot, CNRS, IN2P3, UMR 7585, LPNHE, Paris, France
L. Le Guillou
Max-Planck-Institut fur Astrophysik, Garching bei Munchen, Germany
P. A. Mazzali
Institute of Astronomy, University of Cambridge, Cambridge, UK
N. A. Walton

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F. Förster
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T. J. Moriya
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J. C. Maureira
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J. P. Anderson
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S. Blinnikov
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F. Bufano
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G. Cabrera-Vives
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A. Clocchiatti
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T. de Jaeger
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P. A. Estévez
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L. Galbany
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G. Gräfener
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M. Hamuy
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E. Y. Hsiao
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P. Huentelemu
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P. Huijse
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H. Kuncarayakti
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J. Martínez
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G. Medina
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F. Olivares E.
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G. Pignata
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A. Razza
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I. Reyes
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J. San Martín
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R. C. Smith
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E. Vera
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A. K. Vivas
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A. de Ugarte Postigo
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C. Ashall
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P. A. Mazzali
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N. A. Walton
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D. R. Young
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Correspondence to F. Förster.

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Förster, F., Moriya, T.J., Maureira, J.C. et al. Author Correction: The delay of shock breakout due to circumstellar material evident in most type II supernovae. Nat Astron 3, 107 (2019). https://doi.org/10.1038/s41550-018-0641-7

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Published: 12 November 2018
Issue Date: January 2019
DOI: https://doi.org/10.1038/s41550-018-0641-7

Author Correction: The delay of shock breakout due to circumstellar material evident in most type II supernovae

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