Open Access
Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202349089]


Issue
A&A
Volume 694, February 2025
Article Number C2
Number of page(s) 2
Section Letters to the Editor
DOI https://doi.org/10.1051/0004-6361/202451943e
Published online 10 February 2025

The measurements for planet candidate PDS 70 d reported in Tables 1 and C.1 of the original paper did not reflect the results obtained with our best data reduction. The correct values can now be found in Tables 1 and C.1, respectively.

Table 1.

Properties of the star(+disk), protoplanets b and c, and candidate d inferred from the NIRCam F187N and F480M observations.

References

  1. Mesa, D., Keppler, M., Cantalloube, F., et al. 2019, A&A, 632, A25 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
  2. Wang, J. J., Vigan, A., Lacour, S., et al. 2021, AJ, 161, 148 [Google Scholar]

Appendix C: NEGFC retrieval of planet parameters

Table C.1.

Comparison of the properties of the protoplanets inferred from the NIRCam F187N and F480M observations using NEGFC combined with either roll subtraction or IPCA, and the predictions made in either Wang et al. (2021) for b and c and M19 for candidate d.


© The Authors 2025

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All Tables

Table 1.

Properties of the star(+disk), protoplanets b and c, and candidate d inferred from the NIRCam F187N and F480M observations.

Table C.1.

Comparison of the properties of the protoplanets inferred from the NIRCam F187N and F480M observations using NEGFC combined with either roll subtraction or IPCA, and the predictions made in either Wang et al. (2021) for b and c and M19 for candidate d.

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