TY - JOUR
T1 - Erratum
T2 - TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up (Astronomical Journal (2021) 162 (54) DOI: 10.3847/1538-3881/ac06cd)
AU - Hedges, Christina
AU - Hughes, Alex
AU - Zhou, George
AU - David, Trevor J.
AU - Becker, Juliette
AU - Giacalone, Steven
AU - Vanderburg, Andrew
AU - Rodriguez, Joseph E.
AU - Bieryla, Allyson
AU - Wirth, Christopher
AU - Atherton, Shaun
AU - Fetherolf, Tara
AU - Collins, Karen A.
AU - Price-Whelan, Adrian M.
AU - Bedell, Megan
AU - Quinn, Samuel N.
AU - Gan, Tianjun
AU - Ricker, George R.
AU - Latham, David W.
AU - Vanderspek, Roland K.
AU - Seager, Sara
AU - Winn, Joshua N.
AU - Jenkins, Jon M.
AU - Tronsgaard, René
AU - Buchhave, Lars A.
AU - Kielkopf, John F.
AU - Schwarz, Richard P.
AU - Dressing, Courtney D.
AU - Gonzales, Erica J.
AU - Crossfield, Ian J.M.
AU - Matthews, Elisabeth C.
AU - Jensen, Eric L.N.
AU - Furlan, Elise
AU - Gnilka, Crystal L.
AU - Howell, Steve B.
AU - Lester, Kathryn V.
AU - Scott, Nicholas J.
AU - Feliz, Dax L.
AU - Lund, Michael B.
AU - Siverd, Robert J.
AU - Stevens, Daniel J.
AU - Narita, N.
AU - Fukui, A.
AU - Murgas, F.
AU - Palle, Enric
AU - Sutton, Phil J.
AU - Stassun, Keivan G.
AU - Bouma, Luke G.
AU - Vezie, Michael
AU - Villaseñor, Jesus Noel
AU - Quintana, Elisa V.
AU - Smith, Jeffrey C.
N1 - Publisher Copyright:
© 2022. The Author(s).
PY - 2022/3/1
Y1 - 2022/3/1
N2 - 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}.
AB - 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}.
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U2 - 10.3847/1538-3881/ac4477
DO - 10.3847/1538-3881/ac4477
M3 - Comment/debate
AN - SCOPUS:85125744420
SN - 0004-6256
VL - 163
JO - Astronomical Journal
JF - Astronomical Journal
IS - 3
M1 - 143
ER -