Erratum: "TOI-2076 and TOI-1807: Two young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up"
Notes or commentaries
Article Title | Erratum: "TOI-2076 and TOI-1807: Two young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up" |
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Article Category | Notes or commentaries |
Authors | Hedges, Christina, Hughes, Alex, Zhou, George, David, Trevor J., Becker, Juliette C., Giacalone, Steven, Vanderburg, Andrew, Rodriguez, Joseph E., Bieryla, Allyson, Wirth, Christopher P., Atherton, Shaun, Fetherolf, Tara, Collins, Karen A., Price-Whelan, Karen A., Bedell, Megan E., Quinn, Samuel N., Gan, Tianjun, Ricker, George, Latham, David W., Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Tronsgaard, Rene, Buchhave, Buchhave, Kielkopf, John F., Schwarz, Richard P., Dressing, Courtney D., Gonzales, Erica J., Crossfield, Ian J. M., Matthews, Elisabeth C., Jensen, Eric L.N., Furlan, Elise, Gnilka, Crystal L., Howell, Steve B., Lester, Kathryn V., Scott, Nicholas J., Feliz, Dax, Lund, Michael B., Siverd, Robert J., Stevens, Daniel J., Narita, N., Fukui, A., Murgas, F., Palle, Enric, Sutton, Phil J., Stassun, Keivan G., Bouma, Luke G., Vezie, Michael, Villasenor, Jesus Noel, Quintana, Elisa V. and Smith, Jeffrey C. |
Journal Title | Astronomical Journal |
Journal Citation | 163 (3), pp. 1-3 |
Article Number | 143 |
Number of Pages | 3 |
Year | 2022 |
Place of Publication | United States |
Digital Object Identifier (DOI) | https://doi.org/10.3847/1538-3881/ac4477 |
Web Address (URL) | https://iopscience.iop.org/article/10.3847/1538-3881/ac4477 |
Abstract | In the original paper the reported planet radii are incorrect: the planet radii (Rp) were too large by a factor of the stellar radius in solar units (R*/Re). The quoted values in the abstract, Tables 4 and 5, and Paragraph 2 of Section 7 should be for TOI-2076, Rb=2.5+0.06-0.06 R Rc=3.38+0.08-0.08 R and Rd= 3.16-0.09+0.08 R and for TOI-1807, Rb=1.258-0.039+0.04 R. In Tables 4 and 5, the Planet Radius/Star Radius, (Rp/R*) should be 0.03009 ± +0.00039-0.00039, 0.04069 ±+0.00042-0.00042, and 0.038 ±+0.0006-0.0006 for TOI-2076b, c and d, respectively, and 0.01695 ± 0.00039-0.00039 for TOI-1807 b. We update Figure 12 to the following, and in Section 7, Paragraph 4, we update the text to: "We found that the average planet radius and the sum of planetary radii in the TOI-2076 system are larger than 83% and 86% of the equivalent values in confirmed multiplanet systems, respectively."In Section 7, Paragraph 9, the text should read; "We found that TOI-1807b is the seventh most favorable USP for the detection of mid-IR thermal emission (Table 6 and Figure 13)."Since the original publication date, further TESS discoveries now mean TOI-1807b is the tenth most favorable small USP for phase-curve observations. {figure presented}. {figure presented}. |
Related Output | |
Obsoletes | TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up |
Public Notes | File reproduced in accordance with the copyright policy of the publisher/author. |
https://research.usq.edu.au/item/xv8q3/erratum-toi-2076-and-toi-1807-two-young-comoving-planetary-systems-within-50-pc-identified-by-tess-that-are-ideal-candidates-for-further-follow-up
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