| Issue |
A&A
Volume 702, October 2025
|
|
|---|---|---|
| Article Number | C5 | |
| Number of page(s) | 1 | |
| Section | Planets, planetary systems, and small bodies | |
| DOI | https://doi.org/10.1051/0004-6361/202453045e | |
| Published online | 13 October 2025 | |
A new atmospheric characterization of the sub-stellar companion HR2562B with JWST/MIRI observations (Corrigendum)
1
Aix Marseille Université, CNRS, CNES, LAM,
Marseille,
France
2
Jet Propulsion Laboratory, California Institute of Technology,
Pasadena,
CA
91109,
USA
3
INAF – Osservatorio Astrofisico di Arcetri,
Largo E. Fermi 5,
50125,
Firenze,
Italy
4
Leiden Observatory, Leiden University,
Niels Bohrweg 2,
2333
CA
Leiden,
The Netherlands
5
LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Cité,
5 place Jules Janssen,
92195
Meudon,
France
6
University of Exeter, Astrophysics Group,
Physics Building, Stocker Road,
Exeter,
EX4 4QL,
UK
7
Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM,
91191,
Gif-sur-Yvette,
France
8
Université Paris-Saclay, UVSQ, CNRS, CEA, Maison de la Simulation,
91191,
Giſ-sur-Yvette,
France
★ Corresponding author: nicolas.godoy@lam.fr
Key words: instrumentation: high angular resolution / methods: data analysis / techniques: image processing / planets and satellites: atmospheres / infrared: planetary systems / errata, addenda
An error was found on the y-axis of Fig. 8 and a typographic error in Table 8 of the original paper (Godoy et al. 2024).
The original figure presents the detection limit in 5σ contrast in planet absolute magnitude units (i.e., the Vega system) instead of the contrast to the host star units. In the new Fig. 1, we have corrected the y-axis to match the correct definition of the contrast curve.
In addition, Table 8 in the original paper had a typographic error in one of the column titles. The original table presents the absolute magnitude in the J band (2MASS system) as MJup instead of MJ. In the new Table 1 we have corrected the column name.
These changes do not alter the results, science, or conclusions of the original article.
References
- Godoy, N., Choquet, E., Serabyn, E., et al. 2024, A&A, 689, A185 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© The Authors 2025
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
Colors and absolute magnitudes in the 2MASS and MIRI filters of HR 2562 B and VHS 1256 b.
All Figures
 |
Fig. 1 Smoothed contrast limits (i.e., contrast to the host star) for all JWST/MIRI observations (F1065C, F1140C, and F1550C). |
| In the text | |
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