The CARMENES search for exoplanets around M dwarfs

A. Kaminski; S. Sabotta; J. Kemmer; P. Chaturvedi; R. Burn; J. C. Morales; J. A. Caballero; I. Ribas; A. Reiners; A. Quirrenbach; P. J. Amado; V. J. S. Béjar; S. Dreizler; E. W. Guenther; A. P. Hatzes; Th. Henning; M. Kürster; D. Montes; E. Nagel; E. Pallé; V. Pinter; S. Reffert; M. Schlecker; Y. Shan; T. Trifonov; M. R. Zapatero Osorio; M. Zechmeister

doi:10.1051/0004-6361/202555107e

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A&A, 702 (2025) C3

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202453381]

Issue		A&A Volume 702, October 2025


Article Number		C3
Number of page(s)		2
Section		Planets, planetary systems, and small bodies
DOI		https://doi.org/10.1051/0004-6361/202555107e
Published online		01 October 2025

A&A, 702, C3 (2025)

Occurrence rates of Earth-like planets around very low-mass stars (Corrigendum)

A. Kaminski¹^★, S. Sabotta¹, J. Kemmer¹, P. Chaturvedi²^,3, R. Burn⁴, J. C. Morales⁵^,6, J. A. Caballero⁷, I. Ribas⁵^,6, A. Reiners⁸, A. Quirrenbach¹, P. J. Amado⁹, V. J. S. Béjar¹⁰^,11, S. Dreizler⁸, E. W. Guenther³, A. P. Hatzes³, Th. Henning⁴, M. Kürster⁴, D. Montes¹², E. Nagel⁸, E. Pallé¹⁰^,11, V. Pinter¹³, S. Reffert¹, M. Schlecker¹⁴, Y. Shan⁸^,15, T. Trifonov¹^,16, M. R. Zapatero Osorio⁷ and M. Zechmeister⁸

¹ Landessternwarte, Zentrum für Astronomie der Universität Heidelberg, Königstuhl 12, 69117 Heidelberg, Germany
² Department of Astronomy and Astrophysics, Tata Institute of Fundamental Research, Mumbai 400005, India
³ Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany
⁴ Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
⁵ Institut de Ciències de l’Espai (CSIC), c/ de Can Magrans s/n, Campus UAB, 08193 Bellaterra, Barcelona, Spain
⁶ Institut d’Estudis Espacials de Catalunya, 08860 Castelldefels, Barcelona, Spain
⁷ Centro de Astrobiología (CSIC-INTA), Camino Bajo del Castillo s/n, 28692 Villanueva de la Cañada, Madrid, Spain
⁸ Institut für Astrophysik und Geophysik, Georg-August-Universität, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany
⁹ Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la Astronomía s/n, 18008 Granada, Spain
¹⁰ Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain
¹¹ Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
¹² Departamento de Física de la Tierra y Astrofísica & IPARCOS Instituto de Física de Partículas y del Cosmos, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, Plaza de Ciencias 1, 28400 Madrid, Spain
¹³ Centro Astronómico Hispano en Andalucía, Observatorio Astronómico de Calar Alto, Sierra de los Filabres, 04550 Gérgal, Almería, Spain
¹⁴ Department of Astronomy/Steward Observatory, The University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA
¹⁵ Centre for Planetary Habitability, Department of Geosciences, Universitetet i Oslo, Sem Sælands vei 2b, 0315 Oslo, Norway
¹⁶ Department of Astronomy, Sofia University “St Kliment Ohridski”, 5 James Bourchier Blvd, 1164 Sofia, Bulgaria

^★ Corresponding author: a.kaminski@lsw.uni-heidelberg.de

Key words: planets and satellites: detection / stars: late-type / stars: low-mass / errata, addenda

Erratum for: A&A, 696, A101 (2025), https://doi.org/10.1051/0004-6361/202453381

Regarding Table 5 on page 8 of the original paper, the entry in the last line in the column “Planet ID” needs to be changed from “LP 756-18 b” to “Wolf 1069 b.” The correct table is provided below.

References

Astudillo-Defru, N., Díaz, R. F., Bonfils, X., et al. 2017, A&A, 605, L11 [EDP Sciences] [Google Scholar]
Bauer, F. F., Zechmeister, M., Kaminski, A., et al. 2020, A&A, 640, A50 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
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© 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

Table 5

Known planets around stars in our sample.

In the text

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[1] Astudillo-Defru, N., Díaz, R. F., Bonfils, X., et al. 2017, A&A, 605, L11 [EDP Sciences] [Google Scholar]

[2] Bauer, F. F., Zechmeister, M., Kaminski, A., et al. 2020, A&A, 640, A50 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

[3] Dreizler, S., Luque, R., Ribas, I., et al. 2024, A&A, 684, A117 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

[4] Kossakowski, D., Kürster, M., Trifonov, T., et al. 2023, A&A, 670, A84 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

[5] Morales, J. C., Mustill, A. J., Ribas, I., et al. 2019, Science, 365, 1441 [Google Scholar]

[6] Ribas, I., Reiners, A., Zechmeister, M., et al. 2023, A&A, 670, A139 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

[7] Stock, S., Kemmer, J., Reffert, S., et al. 2020, A&A, 636, A119 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

[8] Suárez Mascareño, A., González-Álvarez, E., Zapatero Osorio, M. R., et al. 2023, A&A, 670, A5 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

[9] Zechmeister, M., Dreizler, S., Ribas, I., et al. 2019, A&A, 627, A49 [NASA ADS] [EDP Sciences] [Google Scholar]