LUMINARIES IN THE SKY: THE TESS LEGACY SAMPLE OF BRIGHT STARS. II. In depth seismic characterisation of the 34 luminaries found in the PLATO LOP fields

Bibcode
2025tasc.confE..33P
DOI
10.5281/zenodo.17295204
Panetier, Eva; García, Rafael A.; Gosmain, Justine; Lund, Mikkel Nørup; Chontos, Ashley; Grundahl, Frank; Mathur, Savita; Breton, Sylvain; Palakkatharappil, Dinil Bose
Bibliographical reference

TASC9/KASC16 9th TESS/16th Kepler Asteroseismic Science Consortium Workshop

Advertised on:
7
2025
Number of authors
9
IAC number of authors
1
Citations
0
Refereed citations
0
Description
The Transiting Exoplanet Survey Satellite (TESS; Ricker et al. 2024) is conducting a nearly full-sky survey, enabling the photometric characterisation of millions of stars. Lund et al. (sub) define a catalog of 196 bright stars ─ referred to as the Luminaries ─ that exhibit solar-like oscillations. These stars serve as important calibrators for upcoming missions such as PLATO (PLAnetary Transits and Oscillations of stars; ESA, Rauer et al. 2024), scheduled for launch in late 2026. PLATO will observe two fields of view during its Long-duration Observation Phase (LOP), each spanning 49° × 49° (Rauer et al. 2024). According to the PLATO Input Catalog (PIC; Montalto et al. 2021), 34 Luminaries are expected to fall within the LOP fields (Nascimbeni et al. 2022, 2025). These 34 stars will undergo in-depth asteroseismic characterization (Panetier et al., in prep.), including mode peakbagging using the apollinaire pipeline (Breton et al. 2022). This poster presents our preliminary results from this ongoing analysis.
Type
Non-refereed

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