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TESS Science Conference 2
Published July 23, 2021 | Version v1
Poster Open

Precise seismology with TESS CVZ data

Creators

  • 1. Ohio State University, Department of Astronomy
  • 2. School of Physics (UNSW)
  • 3. Max-Planck-Institut für Sönnensustemforschung
  • 4. Sydney Institute for Astronomy (SIfA)
  • 5. Instituto de Astrofisica de Canarias (IAC)

Contributors

  • 1. Planetary Science Institute

Description

The release of TESS light-curves gives us the opportunity to perform all-sky seismology for a lot of stars. Among them, the higher quality data that was obtained from the longer light-curves of the South Continuous Viewing Zone (SCVZ) correspond to the best opportunity to conduct precise seismology. In this work we present the first attempt to measure precisely the evolutionary status of a large number red giants stars with TESS data in order to assess the potentiality of those data to perform precise seimsology.

Files

Poster_TESSconference2021_mvrard.pdf

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Additional details

References

  • Hon et al. (2017). Decouple software associated to arXiv:1705.06405
  • Hon et al. (2018). Decouple software associated to arXiv:1804.07495
  • Kuszlewicz et al. (2020). Decouple software associated to arXiv:2007.10921
  • Mackereth et al. (2021). Decouple software associated to arXiv:2012.00140
  • Vrard et al. (2016). Decouple software associated to arXiv:1602.04940