Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations (Corrigendum)

M. De Wilde; A. G. M. Pietrow; M. K. Druett; A. Pastor Yabar; J. Koza; I. Kontogiannis; O. Andriienko; A. Berlicki; A. R. Brunvoll; J. de la Cruz Rodríguez; J. Thoen Faber; R. Joshi; D. Kuridze; D. Nóbrega-Siverio; L. H. M. Rouppe van der Voort; J. Rybák; E. Scullion; A. M. Silva; Z. Vashalomidze; A. Vicente Arévalo; A. Wiśniewska; R. Yadav; T. V. Zaqarashvili; J. Zbinden; E. S. Øyre

doi:10.1051/0004-6361/202660990e

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A&A, 710 (2026) C1

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202554870]

Issue		A&A Volume 710, June 2026


Article Number		C1
Number of page(s)		1
Section		The Sun and the Heliosphere
DOI		https://doi.org/10.1051/0004-6361/202660990e
Published online		17 June 2026

A&A, 710, C1 (2026)

Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations (Corrigendum)

M. De Wilde¹, A. G. M. Pietrow²^,1^★, M. K. Druett¹^,24, A. Pastor Yabar³, J. Koza⁴, I. Kontogiannis⁵^,6, O. Andriienko³, A. Berlicki⁷^,8, A. R. Brunvoll⁹^,10, J. de la Cruz Rodríguez³, J. Thoen Faber⁹^,10, R. Joshi¹¹^,12^,10, D. Kuridze¹³^,14, D. Nóbrega-Siverio¹⁵^,16^,9^,10, L. H. M. Rouppe van der Voort⁹^,10, J. Rybák⁴, E. Scullion¹⁷, A. M. Silva¹⁸^,19, Z. Vashalomidze⁴, A. Vicente Arévalo²⁰, A. Wiśniewska⁴, R. Yadav¹³, T. V. Zaqarashvili²¹^,22^,14, J. Zbinden²³ and E. S. Øyre⁹^,10

¹ Centre for Mathematical Plasma Astrophysics, KU Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium
² Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
³ Inst. for Solar Physics, Dept. of Astronomy, Stockholm University, Albanova University Centre, SE-106 91 Stockholm, Sweden
⁴ Astronomical Institute, Slovak Academy of Sciences, Tatranská Lomnica, 059 60, Slovakia
⁵ ETH Zürich, Institute for Particle Physics and Astrophysics, Wolfgang-Pauli-Strasse 27, 8093 Zürich, Switzerland
⁶ Istituto Ricerche Solari Aldo e Cele Daccó (IRSOL), Locarno, Switzerland
⁷ Centre of Scientific Excellence – Solar and Stellar Activity, University of Wrocław, 50137 Wrocław, Poland
⁸ Astronomical Institute of the Czech Academy of Sciences, 251 65 Ondřejov, Czech Republic
⁹ Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern N-0315, Oslo, Norway
¹⁰ Rosseland Centre for Solar Physics, University of Oslo, P.O. Box 1029 Blindern N-0315, Oslo, Norway
¹¹ Department of Physics and Astronomy, George Mason University, Fairfax, VA 22030, USA
¹² Heliophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
¹³ National Solar Observatory, 3665 Discovery Drive, Boulder, CO 80303, USA
¹⁴ Evgeni Kharadze Georgian National Astrophysical Observatory, Mount Kanobili, 0301 Abastumani, Georgia
¹⁵ Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
¹⁶ Universidad de La Laguna, Dept. Astrofísica, E-38206 La Laguna, Tenerife, Spain
¹⁷ Northumbria University, NE1 8ST, Newcastle upon Tyne, UK
¹⁸ Instituto de Astrofísica e Ciências do Espaço, CAUP, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
¹⁹ Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto, Rua do Campo Alegre, Porto, Portugal
²⁰ Institut für Sonnenphysik (KIS), Georges-Köhler-Allee 401 A, Freiburg i.Br., Germany
²¹ Institute of Physics, University of Graz, Universitätsplatz 5, 8010 Graz, Austria
²² Department of Astronomy and Astrophysics at Space Research Center, Ilia State University, Tbilisi, Georgia
²³ Astronomical Institute of the University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland
²⁴ Plasma Dynamics Group, School of Electrical and Electronic Engineering, University of Sheffield, Sheffield S1 3JD, UK

^★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.

Key words: errata, addenda / line: profiles / methods: data analysis / Sun: atmosphere / Sun: chromosphere / Sun: flares

Erratum for: A&A, 700, A275 (2025), https://doi.org/10.1051/0004-6361/202554870

Table 2 of our paper and the corresponding equation are inconsistent in their treatment of flare emission versus bolometric energy. The table values for the intercepts correspond to log_e rather than log₁₀ as stated in the equation. We provide the corrected table in this erratum.

Table 1.

Correlation coefficients (R) and fitting parameters for the function log₁₀(C_peak) = b + alog₁₀(E) corresponding to the data in Fig. 22 of the original paper.

Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

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All Tables

Table 1.

Correlation coefficients (R) and fitting parameters for the function log₁₀(C_peak) = b + alog₁₀(E) corresponding to the data in Fig. 22 of the original paper.

In the text

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