The GALAH Survey: Using galactic archaeology to refine our knowledge of TESS target stars
dc.contributor.author | Clark, Jake T. | |
dc.contributor.author | Clerté, Mathieu | |
dc.contributor.author | Hinkel, Natalie R. | |
dc.contributor.author | Unterborn, Cayman T. | |
dc.contributor.author | Wittenmyer, Robert | |
dc.contributor.author | Horner, Jonathan | |
dc.contributor.author | Wright, Duncan | |
dc.contributor.author | Carter, Bradley | |
dc.contributor.author | Morton, Timothy D | |
dc.contributor.author | Spina, Lorenzo | |
dc.contributor.author | Asplund, Martin | |
dc.contributor.author | Buder, Sven | |
dc.contributor.author | Duong, Ly | |
dc.contributor.author | Freeman, Kenneth | |
dc.contributor.author | Ting, Yuan-Sen | |
dc.contributor.author | Lin, Jane | |
dc.contributor.author | Nordlander, Thomas | |
dc.date.accessioned | 2022-11-03T01:18:01Z | |
dc.date.available | 2022-11-03T01:18:01Z | |
dc.date.issued | 2021 | |
dc.date.updated | 2021-11-28T07:26:22Z | |
dc.description.abstract | An unprecedented number of exoplanets are being discovered by the Transiting Exoplanet Survey Satellite (TESS). Determining the orbital parameters of these exoplanets, and especially their mass and radius, will depend heavily upon the measured physical characteristics of their host stars. We have cross-matched spectroscopic, photometric, and astrometric data from GALAH Data Release 2, the TESS Input Catalog and Gaia Data Release 2, to create a curated, self-consistent catalogue of physical and chemical properties for 47 285 stars. Using these data, we have derived isochrone masses and radii that are precise to within 5 per cent. We have revised the parameters of three confirmed, and twelve candidate, TESS planetary systems. These results cast doubt on whether CTOI-20125677 is indeed a planetary system, since the revised planetary radii are now comparable to stellar sizes. Our GALAH-TESS catalogue contains abundances for up to 23 elements. We have specifically analysed the molar ratios for C/O, Mg/Si, Fe/Si, and Fe/Mg, to assist in determining the composition and structure of planets with Rp < 4R⊕. From these ratios, 36 per cent fall within 2$\sigma$ sigma of the Sun/Earth values, suggesting that these stars may host rocky exoplanets with geological compositions similar to planets found within our own Solar system. | en_AU |
dc.description.sponsorship | JTC would like to thank SW, BC, and DN, and is supported by the Australian Government Research Training Program (RTP) Scholarship. JTC would also like to thank Vardan Adibekyan for their valuable comments which have significantly improved the science of this manuscript. JDS and SM acknowledges the support of the Australian Research Council through Discovery Project grant DP180101791. SB acknowledges funds from the Australian Research Council (grants DP150100250 and DP160103747). Parts of this research were supported by the Australian Research Council (ARC) Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. YST is grateful to be supported by the NASA Hubble Fellowship grant HSTHF2-51425.001 awarded by the Space Telescope Science Institute. | en_AU |
dc.format.mimetype | application/pdf | en_AU |
dc.identifier.issn | 0035-8711 | en_AU |
dc.identifier.uri | http://hdl.handle.net/1885/277980 | |
dc.language.iso | en_AU | en_AU |
dc.provenance | https://v2.sherpa.ac.uk/id/publication/24618..."The Published Version can be archived in an Institutional Repository" from SHERPA/RoMEO site (as at 3/11/2022). This article has been accepted for publication in [Monthly Notices of the Royal Astronomical Society] ©: 2021 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved | en_AU |
dc.publisher | Oxford University Press | en_AU |
dc.relation | http://purl.org/au-research/grants/arc/DP180101791 | en_AU |
dc.relation | http://purl.org/au-research/grants/arc/DP150100250 | en_AU |
dc.relation | http://purl.org/au-research/grants/arc/DP160103747 | en_AU |
dc.relation | http://purl.org/au-research/grants/arc/CE170100013 | en_AU |
dc.rights | © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society | en_AU |
dc.source | Monthly Notices of the Royal Astronomical Society | en_AU |
dc.subject | methods: observational | en_AU |
dc.subject | catalogues | en_AU |
dc.subject | planets and satellites: interiors | en_AU |
dc.subject | stars: fundamental parameters | en_AU |
dc.subject | stars: abundances | en_AU |
dc.title | The GALAH Survey: Using galactic archaeology to refine our knowledge of TESS target stars | en_AU |
dc.type | Journal article | en_AU |
dcterms.accessRights | Open Access | en_AU |
local.bibliographicCitation.issue | 4 | en_AU |
local.bibliographicCitation.lastpage | 4989 | en_AU |
local.bibliographicCitation.startpage | 4968 | en_AU |
local.contributor.affiliation | Clark, Jake T., University of Southern Queensland | en_AU |
local.contributor.affiliation | Clerté, Mathieu, Centre for Astrophysics | en_AU |
local.contributor.affiliation | Hinkel, Natalie R., Arizona State University | en_AU |
local.contributor.affiliation | Unterborn, Cayman T., School of Earth and Space Exploration | en_AU |
local.contributor.affiliation | Wittenmyer, Robert, University of Southern Queensland | en_AU |
local.contributor.affiliation | Horner, Jonathan, University of Southern Queensland | en_AU |
local.contributor.affiliation | Wright, Duncan , University of Southern Queensland | en_AU |
local.contributor.affiliation | Carter, Bradley, University of Southern Queensland | en_AU |
local.contributor.affiliation | Morton, Timothy D, Department of Physics and Astronomy | en_AU |
local.contributor.affiliation | Spina, Lorenzo, Monash University | en_AU |
local.contributor.affiliation | Asplund, Martin, College of Science, ANU | en_AU |
local.contributor.affiliation | Buder, Sven, College of Science, ANU | en_AU |
local.contributor.affiliation | Duong, Ly, College of Science, ANU | en_AU |
local.contributor.affiliation | Freeman, Kenneth, College of Science, ANU | en_AU |
local.contributor.affiliation | Ting, Yuan-Sen, College of Science, ANU | en_AU |
local.contributor.affiliation | Lin, Jane, College of Science, ANU | en_AU |
local.contributor.affiliation | Nordlander, Thomas, College of Science, ANU | en_AU |
local.contributor.authoremail | u4042723@anu.edu.au | en_AU |
local.contributor.authoruid | Asplund, Martin, u4042723 | en_AU |
local.contributor.authoruid | Buder, Sven, u1054434 | en_AU |
local.contributor.authoruid | Duong, Ly, u4677579 | en_AU |
local.contributor.authoruid | Freeman, Kenneth, u7000399 | en_AU |
local.contributor.authoruid | Ting, Yuan-Sen, u5043815 | en_AU |
local.contributor.authoruid | Lin, Jane, u5027368 | en_AU |
local.contributor.authoruid | Nordlander, Thomas, u1019177 | en_AU |
local.description.notes | Imported from ARIES | en_AU |
local.identifier.absfor | 510109 - Stellar astronomy and planetary systems | en_AU |
local.identifier.absfor | 510104 - Galactic astronomy | en_AU |
local.identifier.absseo | 280120 - Expanding knowledge in the physical sciences | en_AU |
local.identifier.ariespublication | a383154xPUB19995 | en_AU |
local.identifier.citationvolume | 504 | en_AU |
local.identifier.doi | 10.1093/mnras/stab1052 | en_AU |
local.identifier.scopusID | 2-s2.0-85108603353 | |
local.identifier.uidSubmittedBy | a383154 | en_AU |
local.publisher.url | https://academic.oup.com/mnras | en_AU |
local.type.status | Published Version | en_AU |
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