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Doppler confirmation of TESS planet candidate TOI1408.01: grazing transit and likely eccentric orbit. / Galazutdinov, G.A.; Baluev, R.V.; Valyavin, G.; Aitov, V.; Gadelshin, D.; Valeev, A.; Sendzikas, E.; Sokov, E.; Mitiani, G.; Burlakova, T.; Yakunin, I.; Antonyuk, K. A.; Vlasyuk, V.; Romanyuk, I.; Rzaev, A.; Yushkin, M.; Ivanova, A.; Tavrov, A.; Korablev, O.

In: Monthly Notices of the Royal Astronomical Society: Letters, Vol. 526, No. 1, 18.09.2023, p. L111-L115.

Research output: Contribution to journal › Article › peer-review

Harvard

Galazutdinov, GA, Baluev, RV, Valyavin, G, Aitov, V, Gadelshin, D, Valeev, A, Sendzikas, E, Sokov, E, Mitiani, G, Burlakova, T, Yakunin, I, Antonyuk, KA, Vlasyuk, V, Romanyuk, I, Rzaev, A, Yushkin, M, Ivanova, A, Tavrov, A & Korablev, O 2023, 'Doppler confirmation of TESS planet candidate TOI1408.01: grazing transit and likely eccentric orbit', Monthly Notices of the Royal Astronomical Society: Letters, vol. 526, no. 1, pp. L111-L115. https://doi.org/10.1093/mnrasl/slad127

APA

Galazutdinov, G. A., Baluev, R. V., Valyavin, G., Aitov, V., Gadelshin, D., Valeev, A., Sendzikas, E., Sokov, E., Mitiani, G., Burlakova, T., Yakunin, I., Antonyuk, K. A., Vlasyuk, V., Romanyuk, I., Rzaev, A., Yushkin, M., Ivanova, A., Tavrov, A., & Korablev, O. (2023). Doppler confirmation of TESS planet candidate TOI1408.01: grazing transit and likely eccentric orbit. Monthly Notices of the Royal Astronomical Society: Letters, 526(1), L111-L115. https://doi.org/10.1093/mnrasl/slad127

Vancouver

Galazutdinov GA, Baluev RV, Valyavin G, Aitov V, Gadelshin D, Valeev A et al. Doppler confirmation of TESS planet candidate TOI1408.01: grazing transit and likely eccentric orbit. Monthly Notices of the Royal Astronomical Society: Letters. 2023 Sep 18;526(1):L111-L115. https://doi.org/10.1093/mnrasl/slad127

Author

Galazutdinov, G.A. ; Baluev, R.V. ; Valyavin, G. ; Aitov, V. ; Gadelshin, D. ; Valeev, A. ; Sendzikas, E. ; Sokov, E. ; Mitiani, G. ; Burlakova, T. ; Yakunin, I. ; Antonyuk, K. A. ; Vlasyuk, V. ; Romanyuk, I. ; Rzaev, A. ; Yushkin, M. ; Ivanova, A. ; Tavrov, A. ; Korablev, O. / Doppler confirmation of TESS planet candidate TOI1408.01: grazing transit and likely eccentric orbit. In: Monthly Notices of the Royal Astronomical Society: Letters. 2023 ; Vol. 526, No. 1. pp. L111-L115.

BibTeX

@article{c512ded545c84854aa9a3c32b6e5a17c,
title = "Doppler confirmation of TESS planet candidate TOI1408.01: grazing transit and likely eccentric orbit",
abstract = "We report an independent Doppler confirmation of the TESS planet candidate orbiting an F-type main-sequence star TOI−1408 located 140 pc away. We present a set of radial velocities obtained with a high-resolution fibre-optic spectrograph FFOREST mounted at the SAO RAS 6-m telescope (BTA-6). Our self-consistent analysis of these Doppler data and TESS photometry suggests a grazing transit such that the planet obscures its host star by only a portion of the visible disc. Because of this degeneracy, the radius of TOI−1408.01 appears ill-determined with lower limit about ∼1 RJup, significantly larger than in the current TESS solution. We also derive the planet mass of 1.69 ± 0.20 MJup and the orbital period ∼4.425 d, thus making this object a typical hot Jupiter, but with a significant orbital eccentricity of 0.259 ± 0.026. Our 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 possible presence of other unseen companions in the system, yet to be detected.",
author = "G.A. Galazutdinov and R.V. Baluev and G. Valyavin and V. Aitov and D. Gadelshin and A. Valeev and E. Sendzikas and E. Sokov and G. Mitiani and T. Burlakova and I. Yakunin and Antonyuk, {K. A.} and V. Vlasyuk and I. Romanyuk and A. Rzaev and M. Yushkin and A. Ivanova and A. Tavrov and O. Korablev",
year = "2023",
month = sep,
day = "18",
doi = "10.1093/mnrasl/slad127",
language = "English",
volume = "526",
pages = "L111--L115",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Wiley-Blackwell",
number = "1",

}

RIS

TY - JOUR

T1 - Doppler confirmation of TESS planet candidate TOI1408.01: grazing transit and likely eccentric orbit

AU - Galazutdinov, G.A.

AU - Baluev, R.V.

AU - Valyavin, G.

AU - Aitov, V.

AU - Gadelshin, D.

AU - Valeev, A.

AU - Sendzikas, E.

AU - Sokov, E.

AU - Mitiani, G.

AU - Burlakova, T.

AU - Yakunin, I.

AU - Antonyuk, K. A.

AU - Vlasyuk, V.

AU - Romanyuk, I.

AU - Rzaev, A.

AU - Yushkin, M.

AU - Ivanova, A.

AU - Tavrov, A.

AU - Korablev, O.

PY - 2023/9/18

Y1 - 2023/9/18

N2 - We report an independent Doppler confirmation of the TESS planet candidate orbiting an F-type main-sequence star TOI−1408 located 140 pc away. We present a set of radial velocities obtained with a high-resolution fibre-optic spectrograph FFOREST mounted at the SAO RAS 6-m telescope (BTA-6). Our self-consistent analysis of these Doppler data and TESS photometry suggests a grazing transit such that the planet obscures its host star by only a portion of the visible disc. Because of this degeneracy, the radius of TOI−1408.01 appears ill-determined with lower limit about ∼1 RJup, significantly larger than in the current TESS solution. We also derive the planet mass of 1.69 ± 0.20 MJup and the orbital period ∼4.425 d, thus making this object a typical hot Jupiter, but with a significant orbital eccentricity of 0.259 ± 0.026. Our 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 possible presence of other unseen companions in the system, yet to be detected.

AB - We report an independent Doppler confirmation of the TESS planet candidate orbiting an F-type main-sequence star TOI−1408 located 140 pc away. We present a set of radial velocities obtained with a high-resolution fibre-optic spectrograph FFOREST mounted at the SAO RAS 6-m telescope (BTA-6). Our self-consistent analysis of these Doppler data and TESS photometry suggests a grazing transit such that the planet obscures its host star by only a portion of the visible disc. Because of this degeneracy, the radius of TOI−1408.01 appears ill-determined with lower limit about ∼1 RJup, significantly larger than in the current TESS solution. We also derive the planet mass of 1.69 ± 0.20 MJup and the orbital period ∼4.425 d, thus making this object a typical hot Jupiter, but with a significant orbital eccentricity of 0.259 ± 0.026. Our 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 possible presence of other unseen companions in the system, yet to be detected.

UR - https://www.mendeley.com/catalogue/6660ffbd-7a54-3428-abad-c9897349cdb4/

U2 - 10.1093/mnrasl/slad127

DO - 10.1093/mnrasl/slad127

M3 - Article

VL - 526

SP - L111-L115

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 1

ER -

ID: 108805773