| Issue |
A&A
Volume 693, January 2025
|
|
|---|---|---|
| Article Number | C4 | |
| Number of page(s) | 2 | |
| Section | Planets, planetary systems, and small bodies | |
| DOI | https://doi.org/10.1051/0004-6361/202453095e | |
| Published online | 14 January 2025 | |
Power of wavelets in analyses of transit and phase curves in the presence of stellar variability and instrumental noise
II. Accuracy of the transit parameters (Corrigendum)
1
ELTE Eötvös Loránd University, Doctoral School of Physics,
Budapest,
1117
Budapest Pázmány Péter sétány 1/A,
Hungary
2
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences,
Konkoly-Thege Miklós út 15–17,
1121
Budapest,
Hungary
3
CSFK, MTA Centre of Excellence,
1121
Budapest,
Konkoly Thege Miklós út 15–17,
Hungary
4
HUN-REN-ELTE Exoplanet Research Group,
9700 Szent Imre h. u. 112,
Szombathely,
Hungary
5
ELTE Eötvös Loránd University, Gothard Astrophysical Observatory,
9700
Szent Imre h. u. 112,
Szombathely,
Hungary
6
Deutsches Zentrum für Luft–und Raumfahrt, Institute of Planetary Research,
Rutherfordstrasse 2,
12489
Berlin,
Germany
★ Corresponding author; kalman.szilard@csfk.org
This article has no abstract.
Key words: methods: data analysis / techniques: photometric / planets and satellites: general / errata, addenda
© 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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