Erratum: "Non-local Thermodynamic Equilibrium Radiative Transfer Simulations of Sub-Chandrasekhar-mass White Dwarf Detonations" (2021, ApJL, 909, L18)

Ken J. Shen, Stéphane Blondin, Daniel Kasen, Luc Dessart, Dean M.

Townsley, Samuel Boos, D. John Hillier

► To cite this version:

Ken J. Shen, Stéphane Blondin, Daniel Kasen, Luc Dessart, Dean M. Townsley, et al.. Erratum: "Non-local Thermodynamic Equilibrium Radiative Transfer Simulations of Sub-Chandrasekhar-mass White Dwarf Detonations" (2021, ApJL, 909, L18). 2023, 10.3847/2041-8213/ad148e. insu-04479027

HAL Id: insu-04479027

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Submitted on 10 Mar 2024

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Distributed under a Creative Commons Attribution 4.0 International License
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# Erratum: “Non-local Thermodynamic Equilibrium Radiative Transfer Simulations of Sub-Chandrasekhar-mass White Dwarf Detonations” (2021, ApJL, 909, L18)

Ken J. Shen¹, Stéphane Blondin²,³,⁴, Daniel Kasen¹,⁵,⁶, Luc Dessart⁷, Dean M. Townsley⁸, Samuel Boos⁸, and D. John Hillier⁹

¹Department of Astronomy and Theoretical Astrophysics Center, University of California, Berkeley, CA 94720, USA; kenshen@astro.berkeley.edu

²Unidad Mixta Internacional Franco-Chilena de Astronomía, CNRS/INSU UMI 3386, Chile

³Instituto de Astrofísica, Pontificia Universidad Católica de Chile, Santiago, Chile

⁴Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France

⁵Department of Physics, University of California, Berkeley, CA 94720, USA

⁶Lawrence Berkeley National Laboratory, Berkeley, CA, USA

⁷Institut d'Astrophysique de Paris, CNRS-Sorbonne Université, 98 bis boulevard Arago, F-75014 Paris, France

⁸Department of Physics & Astronomy, University of Alabama, Tuscaloosa, AL, USA

⁹Department of Physics and Astronomy & Pittsburgh Particle Physics, Astrophysics, and Cosmology Center (PITT PACC), University of Pittsburgh, Pittsburgh, PA 15260, USA

Received 2023 December 6; published 2023 December 27

Figures 2 and 6 of the published article mistakenly included the *R*-band light curve of SN 1999dq in the *I*-band panels. The correct versions of these figures are shown here in the revised Figures 2 and 6.

<figure><img src="image_3.png" /><figcaption>**Figure 2.** Multiband non-LTE light curves of 50/50 C/O mass ratio WD detonations. Masses are as labeled, with brighter peak *B*-band magnitudes as the mass increases. CMFGEN results are represented by solid lines; Sedona snapshots are demarcated with circles. Open diamonds, circles, and squares show observations of SNe 1999dq, 2011fe, and 1999by, respectively. Note that the observed “bolometric” light curves only consider UVOIR flux and are thus up to ~20% lower than the true bolometric luminosities.</figcaption></figure>

<figure><img src="image_4.png" /></figure>

Original content from this work may be used under the terms of the [Creative Commons Attribution 4.0 licence](https://creativecommons.org/licenses/by/4.0/). Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
<figure><img src="image_5.png" /><figcaption>**Figure 6.** Same as Figure 2, but for C/O mass ratios of 30/70.</figcaption></figure>

ORCID iDs

Ken J. Shen https://orcid.org/0000-0002-9632-6106

Stéphane Blondin https://orcid.org/0000-0002-9388-2932

Luc Dessart https://orcid.org/0000-0003-0599-8407

Dean M. Townsley https://orcid.org/0000-0002-9538-5948

D. John Hillier https://orcid.org/0000-0001-5094-8017