LHS 1815b: The First Thick-disk Planet Detected by TESS
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 ra...
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| Veröffentlicht in: | The Astronomical journal 2020-04, Vol.159 (4), p.160 |
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| creator | Gan, Tianjun Shporer, 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 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 |
| 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 3 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 (Pthick/Pthin = 6482) to be in the thick disk with a much higher expected maximal height (Zmax = 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). |
| doi_str_mv | 10.3847/1538-3881/ab775a |
| format | Article |
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N. ; Anglada-Escudé, Guillem ; Ricker, George R. ; Vanderspek, Roland ; 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</creator><creatorcontrib>Gan, Tianjun ; Shporer, 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 ; 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</creatorcontrib><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 3 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 (Pthick/Pthin = 6482) to be in the thick disk with a much higher expected maximal height (Zmax = 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).</description><identifier>ISSN: 0004-6256</identifier><identifier>ISSN: 1538-3881</identifier><identifier>EISSN: 1538-3881</identifier><identifier>DOI: 10.3847/1538-3881/ab775a</identifier><language>eng</language><publisher>Ames Research Center: The American Astronomical Society</publisher><subject>Astrometric exoplanet detection ; Astrometry ; Astronomy ; Astrophysics ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; COMPARATIVE EVALUATIONS ; DWARF STARS ; Earth and Planetary Astrophysics ; Extrasolar planets ; Galactic evolution ; James Webb Space Telescope ; MASS ; ORBITS ; PHOTOMETRY ; Physics ; Planet detection ; Planet formation ; Planetary evolution ; Planetary interiors ; Planetary systems ; PLANETS ; Polls & surveys ; PROBABILITY ; Radial velocity ; Satellites ; SPACE ; Space telescopes ; SPECTROSCOPY ; Stellar kinematics ; TELESCOPES ; Transit ; Transit photometry ; Transits</subject><ispartof>The Astronomical journal, 2020-04, Vol.159 (4), p.160</ispartof><rights>2020. 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All rights reserved.</rights><rights>Copyright Determination: MAY_INCLUDE_COPYRIGHT_MATERIAL</rights><rights>Copyright IOP Publishing Apr 2020</rights><rights>Attribution</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c528t-adcfde3f7e08d17bee73134799fa36855d30e0b5e4438e04e758fc425f0c993d3</citedby><cites>FETCH-LOGICAL-c528t-adcfde3f7e08d17bee73134799fa36855d30e0b5e4438e04e758fc425f0c993d3</cites><orcidid>0000-0003-3654-1602 ; 0000-0001-8317-2788 ; 0000-0002-2532-2853 ; 0000-0002-4625-7333 ; 0000-0002-4671-2957 ; 0000-0002-8462-515X ; 0000-0001-6588-9574 ; 0000-0002-3439-1439 ; 0000-0002-6892-6948 ; 0000-0002-4503-9705 ; 0000-0002-1836-3120 ; 0000-0002-4265-047X ; 0000-0003-2058-6662 ; 0000-0002-4829-7101 ; 0000-0002-0619-7639 ; 0000-0002-3481-9052 ; 0000-0001-5371-3432 ; 0000-0001-9380-6457 ; 0000-0001-6763-6562 ; 0000-0002-5169-9427 ; 0000-0003-1309-2904 ; 0000-0003-0918-7484 ; 0000-0002-4881-3620 ; 0000-0002-4715-9460 ; 0000-0001-9911-7388 ; 0000-0002-0149-1302 ; 0000-0001-8627-9628 ; 0000-0003-3618-7535 ; 0000-0001-7416-7522 ; 0000-0002-6778-7552 ; 0000-0002-4017-0667 ; 0000-0001-6175-3872 ; 0000-0003-4190-1916 ; 0000-0001-9003-8894</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-3881/ab775a/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>230,314,776,780,796,881,27901,27902,38845,38867,53815,53842</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.3847/1538-3881/ab775a$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttps://hal.science/hal-03104110$$DView record in HAL$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/23013162$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Gan, Tianjun</creatorcontrib><creatorcontrib>Shporer, Avi</creatorcontrib><creatorcontrib>Livingston, John H.</creatorcontrib><creatorcontrib>Collins, Karen A.</creatorcontrib><creatorcontrib>Mao, Shude</creatorcontrib><creatorcontrib>Trani, Alessandro A.</creatorcontrib><creatorcontrib>Gandolfi, Davide</creatorcontrib><creatorcontrib>Hirano, Teruyuki</creatorcontrib><creatorcontrib>Luque, Rafael</creatorcontrib><creatorcontrib>Stassun, Keivan G.</creatorcontrib><creatorcontrib>Ziegler, Carl</creatorcontrib><creatorcontrib>Howell, Steve B.</creatorcontrib><creatorcontrib>Hellier, Coel</creatorcontrib><creatorcontrib>Irwin, Jonathan M.</creatorcontrib><creatorcontrib>Winters, Jennifer G.</creatorcontrib><creatorcontrib>Anderson, David R.</creatorcontrib><creatorcontrib>Briceño, César</creatorcontrib><creatorcontrib>Law, Nicholas</creatorcontrib><creatorcontrib>Mann, Andrew W.</creatorcontrib><creatorcontrib>Bonfils, Xavier</creatorcontrib><creatorcontrib>Astudillo-Defru, Nicola</creatorcontrib><creatorcontrib>Jensen, Eric L. N.</creatorcontrib><creatorcontrib>Anglada-Escudé, Guillem</creatorcontrib><creatorcontrib>Ricker, George R.</creatorcontrib><creatorcontrib>Vanderspek, Roland</creatorcontrib><creatorcontrib>Latham, David W.</creatorcontrib><creatorcontrib>Seager, Sara</creatorcontrib><creatorcontrib>Winn, Joshua N.</creatorcontrib><creatorcontrib>Jenkins, Jon M.</creatorcontrib><creatorcontrib>Furesz, Gabor</creatorcontrib><creatorcontrib>Guerrero, Natalia M.</creatorcontrib><creatorcontrib>Quintana, Elisa</creatorcontrib><creatorcontrib>Twicken, Joseph D.</creatorcontrib><creatorcontrib>Caldwell, Douglas A.</creatorcontrib><creatorcontrib>Tenenbaum, Peter</creatorcontrib><creatorcontrib>Huang, Chelsea X.</creatorcontrib><creatorcontrib>Rowden, Pamela</creatorcontrib><creatorcontrib>Rojas-Ayala, Bárbara</creatorcontrib><title>LHS 1815b: The First Thick-disk Planet Detected by TESS</title><title>The Astronomical journal</title><addtitle>AJ</addtitle><addtitle>Astron. J</addtitle><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 3 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 (Pthick/Pthin = 6482) to be in the thick disk with a much higher expected maximal height (Zmax = 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).</description><subject>Astrometric exoplanet detection</subject><subject>Astrometry</subject><subject>Astronomy</subject><subject>Astrophysics</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>COMPARATIVE EVALUATIONS</subject><subject>DWARF STARS</subject><subject>Earth and Planetary Astrophysics</subject><subject>Extrasolar planets</subject><subject>Galactic evolution</subject><subject>James Webb Space Telescope</subject><subject>MASS</subject><subject>ORBITS</subject><subject>PHOTOMETRY</subject><subject>Physics</subject><subject>Planet detection</subject><subject>Planet formation</subject><subject>Planetary evolution</subject><subject>Planetary interiors</subject><subject>Planetary systems</subject><subject>PLANETS</subject><subject>Polls & surveys</subject><subject>PROBABILITY</subject><subject>Radial velocity</subject><subject>Satellites</subject><subject>SPACE</subject><subject>Space telescopes</subject><subject>SPECTROSCOPY</subject><subject>Stellar kinematics</subject><subject>TELESCOPES</subject><subject>Transit</subject><subject>Transit photometry</subject><subject>Transits</subject><issn>0004-6256</issn><issn>1538-3881</issn><issn>1538-3881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>CYI</sourceid><recordid>eNp1kMFLwzAUh4MoOKd3Dx4KehGse69JmtTbmJsTBgqb55CmKes229l0wv57UyrbRU8Jed_73suPkGuERyqZGCCnMqRS4kCnQnB9QnqHp1PSAwAWxhGPz8mFcysARAmsR8RsOg9QIk-fgsXSBpOido2_FWYdZoVbB-8bXdomeLaNNY3NgnQfLMbz-SU5y_XG2avfs08-JuPFaBrO3l5eR8NZaHgkm1BnJs8szYUFmaFIrRUUKRNJkmsaS84zChZSbhmj0gKzgsvcsIjnYJKEZrRPbjtv5ZpCOVP4NZamKku_jYooIMU48tR9Ry31Rm3r4lPXe1XpQk2HM9W-AUVgiPCNR-O2rr521jVqVe3q0n_C-2QECfAYPAUdZerKudrmBy2CagNXbbqqTVd1gfuWm66l1E6rsqm9ECJso2Zx7Mt3XbmotseReuVFiWIKY1DbLPfYwx_Yv0N_ALTukIA</recordid><startdate>20200401</startdate><enddate>20200401</enddate><creator>Gan, Tianjun</creator><creator>Shporer, Avi</creator><creator>Livingston, John H.</creator><creator>Collins, Karen A.</creator><creator>Mao, Shude</creator><creator>Trani, Alessandro A.</creator><creator>Gandolfi, Davide</creator><creator>Hirano, Teruyuki</creator><creator>Luque, Rafael</creator><creator>Stassun, Keivan G.</creator><creator>Ziegler, Carl</creator><creator>Howell, Steve B.</creator><creator>Hellier, Coel</creator><creator>Irwin, Jonathan M.</creator><creator>Winters, Jennifer G.</creator><creator>Anderson, David R.</creator><creator>Briceño, César</creator><creator>Law, Nicholas</creator><creator>Mann, Andrew W.</creator><creator>Bonfils, Xavier</creator><creator>Astudillo-Defru, Nicola</creator><creator>Jensen, Eric L. 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N. ; Anglada-Escudé, Guillem ; Ricker, George R. ; Vanderspek, Roland ; 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><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c528t-adcfde3f7e08d17bee73134799fa36855d30e0b5e4438e04e758fc425f0c993d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Astrometric exoplanet detection</topic><topic>Astrometry</topic><topic>Astronomy</topic><topic>Astrophysics</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>COMPARATIVE EVALUATIONS</topic><topic>DWARF STARS</topic><topic>Earth and Planetary Astrophysics</topic><topic>Extrasolar planets</topic><topic>Galactic evolution</topic><topic>James Webb Space Telescope</topic><topic>MASS</topic><topic>ORBITS</topic><topic>PHOTOMETRY</topic><topic>Physics</topic><topic>Planet detection</topic><topic>Planet formation</topic><topic>Planetary evolution</topic><topic>Planetary interiors</topic><topic>Planetary systems</topic><topic>PLANETS</topic><topic>Polls & surveys</topic><topic>PROBABILITY</topic><topic>Radial velocity</topic><topic>Satellites</topic><topic>SPACE</topic><topic>Space telescopes</topic><topic>SPECTROSCOPY</topic><topic>Stellar kinematics</topic><topic>TELESCOPES</topic><topic>Transit</topic><topic>Transit photometry</topic><topic>Transits</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gan, Tianjun</creatorcontrib><creatorcontrib>Shporer, Avi</creatorcontrib><creatorcontrib>Livingston, John H.</creatorcontrib><creatorcontrib>Collins, Karen A.</creatorcontrib><creatorcontrib>Mao, Shude</creatorcontrib><creatorcontrib>Trani, Alessandro A.</creatorcontrib><creatorcontrib>Gandolfi, Davide</creatorcontrib><creatorcontrib>Hirano, Teruyuki</creatorcontrib><creatorcontrib>Luque, Rafael</creatorcontrib><creatorcontrib>Stassun, Keivan G.</creatorcontrib><creatorcontrib>Ziegler, Carl</creatorcontrib><creatorcontrib>Howell, Steve B.</creatorcontrib><creatorcontrib>Hellier, Coel</creatorcontrib><creatorcontrib>Irwin, Jonathan M.</creatorcontrib><creatorcontrib>Winters, Jennifer G.</creatorcontrib><creatorcontrib>Anderson, David R.</creatorcontrib><creatorcontrib>Briceño, César</creatorcontrib><creatorcontrib>Law, Nicholas</creatorcontrib><creatorcontrib>Mann, Andrew W.</creatorcontrib><creatorcontrib>Bonfils, Xavier</creatorcontrib><creatorcontrib>Astudillo-Defru, Nicola</creatorcontrib><creatorcontrib>Jensen, Eric L. N.</creatorcontrib><creatorcontrib>Anglada-Escudé, Guillem</creatorcontrib><creatorcontrib>Ricker, George R.</creatorcontrib><creatorcontrib>Vanderspek, Roland</creatorcontrib><creatorcontrib>Latham, David W.</creatorcontrib><creatorcontrib>Seager, Sara</creatorcontrib><creatorcontrib>Winn, Joshua N.</creatorcontrib><creatorcontrib>Jenkins, Jon M.</creatorcontrib><creatorcontrib>Furesz, Gabor</creatorcontrib><creatorcontrib>Guerrero, Natalia M.</creatorcontrib><creatorcontrib>Quintana, Elisa</creatorcontrib><creatorcontrib>Twicken, Joseph D.</creatorcontrib><creatorcontrib>Caldwell, Douglas A.</creatorcontrib><creatorcontrib>Tenenbaum, Peter</creatorcontrib><creatorcontrib>Huang, Chelsea X.</creatorcontrib><creatorcontrib>Rowden, Pamela</creatorcontrib><creatorcontrib>Rojas-Ayala, Bárbara</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><collection>OSTI.GOV</collection><jtitle>The Astronomical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Gan, Tianjun</au><au>Shporer, Avi</au><au>Livingston, John H.</au><au>Collins, Karen A.</au><au>Mao, Shude</au><au>Trani, Alessandro A.</au><au>Gandolfi, Davide</au><au>Hirano, Teruyuki</au><au>Luque, Rafael</au><au>Stassun, Keivan G.</au><au>Ziegler, Carl</au><au>Howell, Steve B.</au><au>Hellier, Coel</au><au>Irwin, Jonathan M.</au><au>Winters, Jennifer G.</au><au>Anderson, David R.</au><au>Briceño, César</au><au>Law, Nicholas</au><au>Mann, Andrew W.</au><au>Bonfils, Xavier</au><au>Astudillo-Defru, Nicola</au><au>Jensen, Eric L. N.</au><au>Anglada-Escudé, Guillem</au><au>Ricker, George R.</au><au>Vanderspek, Roland</au><au>Latham, David W.</au><au>Seager, Sara</au><au>Winn, Joshua N.</au><au>Jenkins, Jon M.</au><au>Furesz, Gabor</au><au>Guerrero, Natalia M.</au><au>Quintana, Elisa</au><au>Twicken, Joseph D.</au><au>Caldwell, Douglas A.</au><au>Tenenbaum, Peter</au><au>Huang, Chelsea X.</au><au>Rowden, Pamela</au><au>Rojas-Ayala, Bárbara</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>LHS 1815b: The First Thick-disk Planet Detected by TESS</atitle><jtitle>The Astronomical journal</jtitle><stitle>AJ</stitle><addtitle>Astron. J</addtitle><date>2020-04-01</date><risdate>2020</risdate><volume>159</volume><issue>4</issue><spage>160</spage><pages>160-</pages><issn>0004-6256</issn><issn>1538-3881</issn><eissn>1538-3881</eissn><abstract>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 3 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 (Pthick/Pthin = 6482) to be in the thick disk with a much higher expected maximal height (Zmax = 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).</abstract><cop>Ames Research Center</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-3881/ab775a</doi><tpages>12</tpages><orcidid>https://orcid.org/0000-0003-3654-1602</orcidid><orcidid>https://orcid.org/0000-0001-8317-2788</orcidid><orcidid>https://orcid.org/0000-0002-2532-2853</orcidid><orcidid>https://orcid.org/0000-0002-4625-7333</orcidid><orcidid>https://orcid.org/0000-0002-4671-2957</orcidid><orcidid>https://orcid.org/0000-0002-8462-515X</orcidid><orcidid>https://orcid.org/0000-0001-6588-9574</orcidid><orcidid>https://orcid.org/0000-0002-3439-1439</orcidid><orcidid>https://orcid.org/0000-0002-6892-6948</orcidid><orcidid>https://orcid.org/0000-0002-4503-9705</orcidid><orcidid>https://orcid.org/0000-0002-1836-3120</orcidid><orcidid>https://orcid.org/0000-0002-4265-047X</orcidid><orcidid>https://orcid.org/0000-0003-2058-6662</orcidid><orcidid>https://orcid.org/0000-0002-4829-7101</orcidid><orcidid>https://orcid.org/0000-0002-0619-7639</orcidid><orcidid>https://orcid.org/0000-0002-3481-9052</orcidid><orcidid>https://orcid.org/0000-0001-5371-3432</orcidid><orcidid>https://orcid.org/0000-0001-9380-6457</orcidid><orcidid>https://orcid.org/0000-0001-6763-6562</orcidid><orcidid>https://orcid.org/0000-0002-5169-9427</orcidid><orcidid>https://orcid.org/0000-0003-1309-2904</orcidid><orcidid>https://orcid.org/0000-0003-0918-7484</orcidid><orcidid>https://orcid.org/0000-0002-4881-3620</orcidid><orcidid>https://orcid.org/0000-0002-4715-9460</orcidid><orcidid>https://orcid.org/0000-0001-9911-7388</orcidid><orcidid>https://orcid.org/0000-0002-0149-1302</orcidid><orcidid>https://orcid.org/0000-0001-8627-9628</orcidid><orcidid>https://orcid.org/0000-0003-3618-7535</orcidid><orcidid>https://orcid.org/0000-0001-7416-7522</orcidid><orcidid>https://orcid.org/0000-0002-6778-7552</orcidid><orcidid>https://orcid.org/0000-0002-4017-0667</orcidid><orcidid>https://orcid.org/0000-0001-6175-3872</orcidid><orcidid>https://orcid.org/0000-0003-4190-1916</orcidid><orcidid>https://orcid.org/0000-0001-9003-8894</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | ISSN: 0004-6256 |
| ispartof | The Astronomical journal, 2020-04, Vol.159 (4), p.160 |
| issn | 0004-6256 1538-3881 1538-3881 |
| language | eng |
| recordid | cdi_nasa_ntrs_20210011466 |
| source | IOP Publishing Free Content |
| subjects | Astrometric exoplanet detection Astrometry Astronomy Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY COMPARATIVE EVALUATIONS DWARF STARS Earth and Planetary Astrophysics Extrasolar planets Galactic evolution James Webb Space Telescope MASS ORBITS PHOTOMETRY Physics Planet detection Planet formation Planetary evolution Planetary interiors Planetary systems PLANETS Polls & surveys PROBABILITY Radial velocity Satellites SPACE Space telescopes SPECTROSCOPY Stellar kinematics TELESCOPES Transit Transit photometry Transits |
| title | LHS 1815b: The First Thick-disk Planet Detected by TESS |
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