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author Gan, Tianjun
Shporer, Abraham-Avi
Livingston, John H.
Collins, Karen A.
Mao, Shude
Trani, Alessandro A.
Gandolfi, Davide
Hirano, Teruyuki
Luque, Rafael
Stassun, Keivan G.
Ziegler, Carl
Howell, Steve B.
Hellier, Coel
Irwin, Jonathan M.
Winters, Jennifer G.
Anderson, David R.
Briceño, César
Law, Nicholas
Mann, Andrew W.
Bonfils, Xavier
Astudillo-Defru, Nicola
Jensen, Eric L. N.
Anglada-Escudé, Guillem
Ricker, George R
Vanderspek, Roland K
Latham, David W.
Seager, Sara
Winn, Joshua N.
Jenkins, Jon M.
Furesz, Gabor
Guerrero, Natalia M.
Quintana, Elisa
Twicken, Joseph D.
Caldwell, Douglas A.
Tenenbaum, Peter
Huang, Chelsea X.
Rowden, Pamela
Rojas-Ayala, Bárbara
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Gan, Tianjun
Shporer, Abraham-Avi
Livingston, John H.
Collins, Karen A.
Mao, Shude
Trani, Alessandro A.
Gandolfi, Davide
Hirano, Teruyuki
Luque, Rafael
Stassun, Keivan G.
Ziegler, Carl
Howell, Steve B.
Hellier, Coel
Irwin, Jonathan M.
Winters, Jennifer G.
Anderson, David R.
Briceño, César
Law, Nicholas
Mann, Andrew W.
Bonfils, Xavier
Astudillo-Defru, Nicola
Jensen, Eric L. N.
Anglada-Escudé, Guillem
Ricker, George R
Vanderspek, Roland K
Latham, David W.
Seager, Sara
Winn, Joshua N.
Jenkins, Jon M.
Furesz, Gabor
Guerrero, Natalia M.
Quintana, Elisa
Twicken, Joseph D.
Caldwell, Douglas A.
Tenenbaum, Peter
Huang, Chelsea X.
Rowden, Pamela
Rojas-Ayala, Bárbara
author_sort Gan, Tianjun
collection MIT
description We report the first discovery of a thick-disk planet, LHS 1815b (TOI-704b, TIC 260004324), detected in the Transiting Exoplanet Survey Satellite (TESS) survey. LHS 1815b transits a bright (V = 12.19 mag, K = 7.99 mag) and quiet M dwarf located 29.87 ± 0.02 pc away with a mass of 0.502 ± 0.015 M ⊙ and a radius of 0.501 ± 0.030 R ⊙. We validate the planet by combining space- and ground-based photometry, spectroscopy, and imaging. The planet has a radius of 1.088 ± 0.064 R ⊕ with a 3σ mass upper limit of 8.7 M ⊕. We analyze the galactic kinematics and orbit of the host star LHS 1815 and find that it has a large probability (P thick/P thin = 6482) to be in the thick disk with a much higher expected maximal height (Z max = 1.8 kpc) above the Galactic plane compared with other TESS planet host stars. Future studies of the interior structure and atmospheric properties of planets in such systems using, for example, the upcoming James Webb Space Telescope, can investigate the differences in formation efficiency and evolution for planetary systems between different Galactic components (thick disks, thin disks, and halo). Keywords: Astrometric exoplanet detection ; Astrometry; Stellar kinematics; Transit photometry; Radio velocity
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spelling mit-1721.1/1252602022-09-29T20:26:19Z LHS 1815b: The First Thick-disk Planet Detected by TESS Gan, Tianjun Shporer, Abraham-Avi Livingston, John H. Collins, Karen A. Mao, Shude Trani, Alessandro A. Gandolfi, Davide Hirano, Teruyuki Luque, Rafael Stassun, Keivan G. Ziegler, Carl Howell, Steve B. Hellier, Coel Irwin, Jonathan M. Winters, Jennifer G. Anderson, David R. Briceño, César Law, Nicholas Mann, Andrew W. Bonfils, Xavier Astudillo-Defru, Nicola Jensen, Eric L. N. Anglada-Escudé, Guillem Ricker, George R Vanderspek, Roland K Latham, David W. Seager, Sara Winn, Joshua N. Jenkins, Jon M. Furesz, Gabor Guerrero, Natalia M. Quintana, Elisa Twicken, Joseph D. Caldwell, Douglas A. Tenenbaum, Peter Huang, Chelsea X. Rowden, Pamela Rojas-Ayala, Bárbara Massachusetts Institute of Technology. Department of Physics Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Massachusetts Institute of Technology. Department of Aeronautics and Astronautics MIT Kavli Institute for Astrophysics and Space Research We report the first discovery of a thick-disk planet, LHS 1815b (TOI-704b, TIC 260004324), detected in the Transiting Exoplanet Survey Satellite (TESS) survey. LHS 1815b transits a bright (V = 12.19 mag, K = 7.99 mag) and quiet M dwarf located 29.87 ± 0.02 pc away with a mass of 0.502 ± 0.015 M ⊙ and a radius of 0.501 ± 0.030 R ⊙. We validate the planet by combining space- and ground-based photometry, spectroscopy, and imaging. The planet has a radius of 1.088 ± 0.064 R ⊕ with a 3σ mass upper limit of 8.7 M ⊕. We analyze the galactic kinematics and orbit of the host star LHS 1815 and find that it has a large probability (P thick/P thin = 6482) to be in the thick disk with a much higher expected maximal height (Z max = 1.8 kpc) above the Galactic plane compared with other TESS planet host stars. Future studies of the interior structure and atmospheric properties of planets in such systems using, for example, the upcoming James Webb Space Telescope, can investigate the differences in formation efficiency and evolution for planetary systems between different Galactic components (thick disks, thin disks, and halo). Keywords: Astrometric exoplanet detection ; Astrometry; Stellar kinematics; Transit photometry; Radio velocity 2020-05-15T14:04:29Z 2020-05-15T14:04:29Z 2020-03 2019-12 2020-05-06T14:21:58Z Article http://purl.org/eprint/type/JournalArticle 1538-3881 https://hdl.handle.net/1721.1/125260 Gan, Tianjun, et al. "LHS 1815b: The First Thick-disk Planet Detected by TESS." The Astronomical Journal, 159 (April 2020). © 2020. The American Astronomical Society. All rights reserved. en http://dx.doi.org/10.3847/1538-3881/ab775a The Astronomical Journal Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf American Astronomical Society The American Astronomical Society
spellingShingle Gan, Tianjun
Shporer, Abraham-Avi
Livingston, John H.
Collins, Karen A.
Mao, Shude
Trani, Alessandro A.
Gandolfi, Davide
Hirano, Teruyuki
Luque, Rafael
Stassun, Keivan G.
Ziegler, Carl
Howell, Steve B.
Hellier, Coel
Irwin, Jonathan M.
Winters, Jennifer G.
Anderson, David R.
Briceño, César
Law, Nicholas
Mann, Andrew W.
Bonfils, Xavier
Astudillo-Defru, Nicola
Jensen, Eric L. N.
Anglada-Escudé, Guillem
Ricker, George R
Vanderspek, Roland K
Latham, David W.
Seager, Sara
Winn, Joshua N.
Jenkins, Jon M.
Furesz, Gabor
Guerrero, Natalia M.
Quintana, Elisa
Twicken, Joseph D.
Caldwell, Douglas A.
Tenenbaum, Peter
Huang, Chelsea X.
Rowden, Pamela
Rojas-Ayala, Bárbara
LHS 1815b: The First Thick-disk Planet Detected by TESS
title LHS 1815b: The First Thick-disk Planet Detected by TESS
title_full LHS 1815b: The First Thick-disk Planet Detected by TESS
title_fullStr LHS 1815b: The First Thick-disk Planet Detected by TESS
title_full_unstemmed LHS 1815b: The First Thick-disk Planet Detected by TESS
title_short LHS 1815b: The First Thick-disk Planet Detected by TESS
title_sort lhs 1815b the first thick disk planet detected by tess
url https://hdl.handle.net/1721.1/125260
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