期刊
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
卷 241, 期 1, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.3847/1538-4365/ab04f5
关键词
catalogs; space vehicles: instruments; stars: fundamental parameters; stars: oscillations; surveys
资金
- University of Birmingham
- UK Science and Technology Facilities Council (STFC)
- European Union [792848]
- NASA [NNX16AB97G]
- Spanish Ministry of Economy [ESP2017-82674-R]
- Generalitat de Catalunya [SGR2017-1131]
- Danish National Research Foundation [DNRF106]
- [CIAAUP-12/2018-BPD]
- NASA [NNX16AB97G, 907754] Funding Source: Federal RePORTER
- Marie Curie Actions (MSCA) [792848] Funding Source: Marie Curie Actions (MSCA)
We present the target list of solar-type stars to be observed in short-cadence (2 minute) for asteroseismology by the NASA Transiting Exoplanet Survey Satellite (TESS) during its 2 year nominal survey mission. The solar-like Asteroseismic Target List (ATL) is comprised of bright, cool main-sequence and subgiant stars and forms part of the larger target list of the TESS Asteroseismic Science Consortium. The ATL uses the Gaia Data Release 2 and the Extended Hipparcos Compilation (XHIP) to derive fundamental stellar properties, to calculate detection probabilities, and to produce a rank-ordered target list. We provide a detailed description of how the ATL was produced and calculate expected yields for solar-like oscillators based on the nominal photometric performance by TESS. We also provide a publicly available source code that can be used to reproduce the ATL, thereby enabling comparisons of asteroseismic results from TESS with predictions from synthetic stellar populations.
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