| Issue |
A&A
Volume 671, March 2023
|
|
|---|---|---|
| Article Number | C3 | |
| Number of page(s) | 4 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361/202243830e | |
| Published online | 13 March 2023 | |
Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy (Corrigendum)
1
Anton Pannekoek Institute for Astronomy, University of Amsterdam,
Science Park 904,
1098 XH
Amsterdam, The Netherlands
e-mail: d.c.linssen@uva.nl
2
Center for Astrophysics | Harvard & Smithsonian,
60 Garden Street, MS-16,
Cambridge, MA
02138, USA
Key words: planets and satellites: atmospheres / planets and satellites: dynamical evolution and stability / methods: numerical / errata, addenda
In Sect. 4.3, we assumed a normally distributed prior and likelihood but erroneously used p-values derived from the survival function instead of from the probability density function of the normal distribution. We gave the example of a temperature difference of THe – T0 = 2σT, which we considered a 2σ discrepancy and thus translated to a prior p-value of ~0.05 (rounded from 0.0455, equal to two times the survival function evaluated at 2σ). Instead, we should have used a p-value of 0.0540, equal to the probability density function evaluated at 2σ. This error has only a minimal effect on the posteriors we derived. Figures 1, 2, and 3 show corrected versions of Figs. 4, 5, and A.1 from the original paper, respectively. Table 1 gives the corrected values for the constrained temperatures and mass-loss rates of Table 1 from the original paper. All main findings and conclusions remain unaffected.
Corrected values for the constrained temperatures and mass-loss rates for the investigated exoplanets.
 |
Fig. 1 Corrected Fig. 4. Only the posteriors in the bottom-right panel have changed, and only slightly. |
 |
Fig. 2 Corrected Fig. 5. The only difference is a slight change in the posteriors. |
 |
Fig. 3 Corrected Fig. A.1. The only difference is a slight change in the posteriors. |
© The Authors 2023
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.
This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.
All Tables
Corrected values for the constrained temperatures and mass-loss rates for the investigated exoplanets.
All Figures
|
Fig. 1 Corrected Fig. 4. Only the posteriors in the bottom-right panel have changed, and only slightly. |
| In the text | |
|
Fig. 2 Corrected Fig. 5. The only difference is a slight change in the posteriors. |
| In the text | |
|
Fig. 3 Corrected Fig. A.1. The only difference is a slight change in the posteriors. |
| In the text | |
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.