Correction to: Trio of super-Earth candidates orbiting K-dwarf HD 48948: a new habitable zone candidate
Notes or commentaries
Article Title | Correction to: Trio of super-Earth candidates orbiting K-dwarf HD 48948: a new habitable zone candidate |
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ERA Journal ID | 1074 |
Article Category | Notes or commentaries |
Authors | Dalal, S., Rescigno, F., Cretignier, M., John, A.A., Majidi, F.Z., Malavolta, L., Mortier, A., Pinamonti, M., Buchhave, L. A., Haywood, R., Sozzetti, A., Dumusque, X., Lienhard, F., Rice, K., Vanderburg, A., Lakeland, B., Bonomo, A. S., Collier Cameron, A., Damasso, M., Affer, L., Boschin, W., Cooke, B., Cosentino, R., Di Fabrizio, L., Ghedina, A., Harutyunyan, A., Latham, D., Lopez-Morales, M., Lovis, C., Martinez Fiorenzano, A., Mayor, M., Nicholson, B., Pepe, F., Stalport, M., Udry, S., Watson, C. a. and Wilson, T. G. |
Journal Title | Monthly Notices of the Royal Astronomical Society |
Journal Citation | 534 (3), pp. 2410-2411 |
Number of Pages | 2 |
Year | 2024 |
Publisher | Oxford University Press |
Place of Publication | United Kingdom |
ISSN | 0035-8711 |
1365-2966 | |
Digital Object Identifier (DOI) | https://doi.org/10.1093/mnras/stae2228 |
Web Address (URL) | https://academic.oup.com/mnras/article/534/3/2410/7817797 |
Abstract | This is an erratum to the paper titled ‘Trio of super-Earth candidates orbiting K-Dwarf HD 48948: a new habitable zone candidate’, published in MNRAS 531, 4464–4481 (2024) with 10.1093/mnras/stae1367. We have identified and corrected errors in table 3 of the original publication. The incident flux and temperature values for the three planetary candidates were incorrectly calculated due to a mathematical error. Additionally, we discovered a typographical mistake in the eccentricity values for candidates c and d in the tweaks analysis. The accurate and updated values are provided in the Table 1. While these errors do not alter the overall conclusions of the paper, the corrected values provide a more accurate representation of the data and should be used for reference in future research. |
Keywords | errata, addenda; techniques: radial velocities; planets and satellites: detection; stars: activity; methods: statistical; stars: rotation; instrumentation: spectrographs |
Contains Sensitive Content | Does not contain sensitive content |
Byline Affiliations | University of Exeter, United Kingdom |
University of Oxford, United Kingdom | |
University of St Andrews, United Kingdom | |
University of Padua, Italy | |
INAF - Astrophysical Observatory of Turin, Italy | |
Blue Skies Space, Italy | |
University of Birmingham, United Kingdom | |
Technical University of Denmark, Denmark | |
University of Geneva, Switzerland | |
University of Cambridge, United Kingdom | |
University of Edinburgh, United Kingdom | |
Massachusetts Institute of Technology, United States | |
Galileo Galilei Foundation - INAF, Spain | |
Instituto de Astrof´ısica de Canarias (IAC), Spain | |
University of La Laguna, Spain | |
University of Warwick, United Kingdom | |
Center for Astrophysics Harvard and Smithsonian, United States | |
Centre for Astrophysics | |
University of Liege, Belgium | |
Queen’s University Belfast, United Kingdom |
https://research.usq.edu.au/item/zqz41/correction-to-trio-of-super-earth-candidates-orbiting-k-dwarf-hd-48948-a-new-habitable-zone-candidate
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