Doppler confirmation of TESS planet candidate TOI-1408.01: updated analysis and fitting

Based on the Doppler observations from the FFOREST spectrograph of the 6-meter telescope (BTA) and on the photometric observations from the TESS spacecraft, we provide an updated analysis for TOI-1408, an F-type main sequence star, located 140 pc away, that hosts exoplanet TOI-1408.01. We confirm the qualitative conclusions from our initial paper: (1) a grazing transit geometry such that the planet obscures its host star by only a portion of the visible disc,(2) unreliably fitted planet radius, (3) which nonetheless has a lower bound constraint of $\sim\!1~R_{\rm Jup}$, (4) unexpectedly large planet mass of $\simeq\!1.7~M_{\rm Jup}$, and (5) significant evidence in favor of a moderately eccentric orbit with $e\simeq0.27$. This solution may suggest that the planet is likely to experience a high tidal eccentricity migration at the stage of intense orbital rounding or may indicate the possible presence of other unseen companions in the system, yet to be detected.

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Published
2024-12-27
DOI
https://doi.org/10.26119/vak2024.127
Primary Topic
Stellar, planetary, and galactic studies
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article
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article

Doppler confirmation of TESS planet candidate TOI-1408.01: updated analysis and fitting

A. F. Valeev, G. Sh. Mitiani, A. V. Tavrov, K. A. Antonyuk et al.
Stellar, planetary, and galactic studies
article

Doppler confirmation of TESS planet candidate TOI-1408.01: updated analysis and fitting

A. F. Valeev, G. Sh. Mitiani, A. V. Tavrov, K. A. Antonyuk, V. N. Aitov, Roman V. Baluev, Г. А. Галазутдинов, I. I. Romanyuk, Oleg Korablev, I. A. Yakunin, Anastasiia Ivanova, D. R. Gadelshin, E. Sokov, Е. Г. Сендзикас, А. Х. Рзаев, G. G. Valyavin, T. E. Burlakova, M. V. Yushkin, V. V. Vlasyuk
article en

Abstract

Based on the Doppler observations from the FFOREST spectrograph of the 6-meter telescope (BTA) and on the photometric observations from the TESS spacecraft, we provide an updated analysis for TOI-1408, an F-type main sequence star, located 140 pc away, that hosts exoplanet TOI-1408.01. We confirm the qualitative conclusions from our initial paper: (1) a grazing transit geometry such that the planet obscures its host star by only a portion of the visible disc,(2) unreliably fitted planet radius, (3) which nonetheless has a lower bound constraint of $\sim\!1~R_{\rm Jup}$, (4) unexpectedly large planet mass of $\simeq\!1.7~M_{\rm Jup}$, and (5) significant evidence in favor of a moderately eccentric orbit with $e\simeq0.27$. This solution may suggest that the planet is likely to experience a high tidal eccentricity migration at the stage of intense orbital rounding or may indicate the possible presence of other unseen companions in the system, yet to be detected.

Russian Academy of Sciences (RU), St Petersburg University (RU), Special Astrophysical Observatory (RU), Space Research Institute (RU), Pulkovo Observatory (RU), Development Agency of Serbia (RS), Crimean Astrophysical Observatory (UA)
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