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Cited article:

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The Period Distribution of Hot Jupiters Is Not Dependent on Host Star Metallicity

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Doppler confirmation of TESS planet candidate TOI−1408.01: grazing transit and likely eccentric orbit

G A Galazutdinov, R V Baluev, G Valyavin, V Aitov, D Gadelshin, A Valeev, E Sendzikas, E Sokov, G Mitiani, T Burlakova, I Yakunin, K A Antonyuk, V Vlasyuk, I Romanyuk, A Rzaev, M Yushkin, A Ivanova, A Tavrov and O Korablev
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Production of hot Jupiter candidates from high-eccentricity mechanisms for different initial planetary mass configurations

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Evidence for the Late Arrival of Hot Jupiters in Systems with High Host-star Obliquities

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Tidal migration of hot Jupiters: introducing the impact of gravity wave dissipation

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