Erratum: TESS Hunt for Young and Maturing Exoplanets (THYME). VII. Membership, Rotation, and Lithium in the Young Cluster Group-X and a New Young Exoplanet (The Astronomical Journal (2022) 164 (119) DOI: 10.3847/1538-3881/ac8154)

Elisabeth R. Newton, Rayna Rampalli, Adam L. Kraus, Andrew W. Mann, Jason L. Curtis, Andrew Vanderburg, Daniel M. Krolikowski, Daniel Huber, Grayson C. Petter, Allyson Bieryla, Benjamin M. Tofflemire, Pa Chia Thao, Mackenna L. Wood, Ronan Kerr, Boris S. Safanov, Ivan A. Strakhov, David R. Ciardi, Steven Giacalone, Courtney D. Dressing, Holden GillArjun B. Savel, Karen A. Collins, Peyton Brown, Felipe Murgas, Keisuke Isogai, Norio Narita, Enric Palle, Samuel N. Quinn, Jason D. Eastman, Gábor Fűrész, Bernie Shiao, Tansu Daylan, Douglas A. Caldwell, George R. Ricker, Roland Vanderspek, Sara Seager, Joshua N. Winn, Jon M. Jenkins, David W. Latham

Research output: Contribution to journalComment/debatepeer-review

Abstract

In the original paper (Newton et al. 2022), the reported planetary radii are incorrect and are too small by a factor of R (where R∗ = 0.79 ± 0.04R⊙). In Table 8 of Newton et al. (2022), the values reported as RP/R⊙ are in units of RP/R⊙. The planetary radius in Earth radii quoted in the abstract and the final paragraph of the paper (2.1 ± 0.2R⊕) is correctly RP = 2.6 ± 0.2R⊕. In Table 8, the value for the column "ω fixed"is RP R⊕ 2.59-0.16+0.17 and for the column "ω free"is RP R⊕ 2.61-0.16+0.17 . The planet still falls within the range of radii typical for both field and young mini-Neptunes.

Original languageEnglish (US)
Article number136
JournalAstronomical Journal
Volume165
Issue number3
DOIs
StatePublished - Mar 1 2023

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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