J/AJ/161/65       THYME. IV. 3 Exoplanets around TOI-451 B       (Newton+, 2021)

TESS hunt for young and maturing exoplanets (THYME). IV. Three small planets orbiting a 120Myr old Star in the Pisces-Eridanus stream. Newton E.R., Mann A.W., Kraus A.L., Livingston J.H., Vanderburg A., Curtis J.L., Thao Pa C., Hawkins K., Wood M.L., Rizzuto A.C., Soubkiou A., Tofflemire B.M., Zhou G., Crossfield I.J.M., Pearce L.A., Collins K.A., Conti D.M., Tan T.-G., Villeneuva S., Spencer A., Dragomir D., Quinn S.N., Jensen E.L.N., Collins K.I., Stockdale C., Cloutier R., Hellier C., Benkhaldoun Z., Ziegler C., Briceno C., Law N., Benneke B., Christiansen J.L., Gorjian V., Kane S.R., Kreidberg L., Morales F.Y., Werner M.W., Twicken J.D., Levine A.M., Ciardi D.R., Guerrero N.M., Hesse K., Quintana E.V., Shiao B., Smith J.C., Torres G., Ricker G.R., Vanderspek R., Seager S., Winn J.N., Jenkins J.M., Latham D.W. <Astron. J., 161, 65 (2021)> =2021AJ....161...65N 2021AJ....161...65N
ADC_Keywords: Exoplanets; Stars, dwarfs; Stars, M-type; Optical; Photometry; Stars, double and multiple Keywords: Exoplanet astronomy ; Exoplanet evolution ; Exoplanet systems ; Young star clusters ; Stellar activity Abstract: Young exoplanets can offer insight into the evolution of planetary atmospheres, compositions, and architectures. We present the discovery of the young planetary system TOI-451 (TIC257605131, GaiaDR24844691297067063424). TOI-451 is a member of the 120Myr old Pisces-Eridanus stream (Psc-Eri). We confirm membership in the stream with its kinematics, its lithium abundance, and the rotation and UV excesses of both TOI451 and its wide-binary companion, TOI-451B (itself likely an M-dwarf binary). We identified three candidate planets transiting in the Transiting Exoplanet Survey Satellite data and followed up the signals with photometry from Spitzer and ground-based telescopes. The system comprises three validated planets at periods of 1.9, 9.2, and 16days, with radii of 1.9, 3.1, and 4.1 R, respectively. The host star is near-solar mass with V=11.0 and H=9.3 and displays an infrared excess indicative of a debris disk. The planets offer excellent prospects for transmission spectroscopy with the Hubble Space Telescope and the James Webb Space Telescope, providing the opportunity to study planetary atmospheres that may still be in the process of evolving. Description: Transiting Exoplanet Survey Stallite (TESS) observed TIC257605131 in Sectors 4 and 5, from 2018 October 19 to 2018 December 11. Objects: ------------------------------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------------------------------- 04 11 49.18 -37 56 42.2 TOI 451 B = Gaia DR2 4844691297067064576 ------------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file fig8.dat 20 2107 TESS light curve of TOI 451 B -------------------------------------------------------------------------------- See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) I/337 : Gaia DR1 (Gaia Collaboration, 2016) II/335 : Revised catalog of GALEX UV sources (GUVcat_AIS GR6+7)(Bianchi+ 2017) I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018) I/345 : Gaia DR2 (Gaia Collaboration, 2018) II/358 : SkyMapper Southern Sky Survey. 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(Ziegler+, 2020) Byte-by-byte Description of file: fig8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.4 d BJD [1410/1464] Barycentric Julian Date; BJD-2457000 11- 20 F10.8 --- Flux [0.98/1.14] Relative flux -------------------------------------------------------------------------------- History: From electronic version of the journal References: Newton et al. Paper I. 2019ApJ...880L..17N 2019ApJ...880L..17N Rizzuto et al. Paper II. 2020AJ....160...33R 2020AJ....160...33R Mann et al. Paper III. 2020AJ....160..179M 2020AJ....160..179M Newton et al. Paper IV. 2021AJ....161...65N 2021AJ....161...65N This catalog Tofflemire et al. Paper V. 2021AJ....161..171T 2021AJ....161..171T Cat. J/AJ/161/171 Mann et al. Paper VI. 2022AJ....163..156M 2022AJ....163..156M Cat. J/AJ/163/156 Newton et al. Paper VII. 2022AJ....164..115N 2022AJ....164..115N Cat. J/AJ/164/115 Barber et al. Paper VIII. 2022AJ....164...88B 2022AJ....164...88B Cat. J/AJ/164/88 Wood et al. Paper IX. 2023AJ....165...85W 2023AJ....165...85W Cat. J/AJ/165/85 Thao et al. Paper X. 2024AJ....168...41T 2024AJ....168...41T Cat. J/AJ/168/41 Capistrant et al. Paper XI. 2024AJ....167...54C 2024AJ....167...54C
(End) Prepared by [AAS], Coralie Fix [CDS], 30-Mar-2021
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