| 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 | |
Letter to the Editor
MINDS: JWST/NIRCam imaging of the protoplanetary disk PDS 70
A spiral accretion stream and a potential third protoplanet (Corrigendum)
1
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, Leuven, Belgium
2
STAR Institute, Université de Liège, Allée du Six Août 19c, 4000 Liège, Belgium
3
MPIA, Königstuhl 17, 69117 Heidelberg, Germany
4
Kapteyn Astronomical Institute, Rijksuniversiteit Groningen, Postbus 800, 9700 AV Groningen, The Netherlands
5
LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, 92195 Meudon, France
6
Université Paris-Saclay, CNRS, Institut d’Astrophysique Spatiale, 91405 Orsay, France
7
Fakultät für Physik, Universität Duisburg-Essen, Lotharstraße 1, 47057 Duisburg, Germany
8
Institut für Astronomie und Astrophysik, Universität Tübingen, Auf der Morgenstelle 10, 72076 Tübingen, Germany
9
Physikalisches Institut, Universität Bern, Gesellschaftsstr. 6, 3012 Bern, Switzerland
10
Leiden Sterrewacht, Leiden University, 2300 RA Leiden, The Netherlands
11
MPE, Giessenbachstr. 1, 85748 Garching, Germany
12
Institut für Astrophysik, Universität Wien, Türkenschanzstr. 17, A-1180 Vienna, Austria
13
ETH Zürich, Institute for Particle Physics and Astrophysics, Wolfgang-Pauli-Str. 27, 8093 Zürich, Switzerland
14
Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, F-91191 Gif-sur-Yvette, France
15
Centro de Astrobiología, CSIC-INTA, ESAC Campus, Camino Bajo del Castillo s/n, 28692 Villanueva de la Cañada, Madrid, Spain
16
INAF – Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, 80131 Napoli, Italy
17
Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, D02 XF86 Dublin, Ireland
18
Institutionen för Astronomi, Stockholms Universitet, AlbaNova Universitetscentrum, 10691 Stockholm, Sweden
19
Department of Astrophysics/IMAPP, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands
20
SRON Netherlands Institute for Space Research, Niels Bohrweg 4, NL-2333 CA, Leiden, The Netherlands
21
Institut für Weltraumforschung, Austrian Academy of Sciences, Schmiedlstr. 6, A-8042 Graz, Austria
22
TU Graz, Fakultät für Mathematik, Physik und Geodäsie, Petersgasse 16, 8010 Graz, Austria
⋆ Corresponding author; valentin.christiaens@kuleuven.be
Key words: planets and satellites: detection / planets and satellites: formation / planets and satellites: gaseous planets / protoplanetary disks / planet-disk interactions / errata, addenda
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.
Properties of the star(+disk), protoplanets b and c, and candidate d inferred from the NIRCam F187N and F480M observations.
References
- Mesa, D., Keppler, M., Cantalloube, F., et al. 2019, A&A, 632, A25 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Wang, J. J., Vigan, A., Lacour, S., et al. 2021, AJ, 161, 148 [Google Scholar]
Appendix C: NEGFC retrieval of planet parameters
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
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
Properties of the star(+disk), protoplanets b and c, and candidate d inferred from the NIRCam F187N and F480M observations.
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.
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.