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This article has an erratum: [https://doi.org/10.1051/0004-6361/201935623e]


Fig. 1

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Ultra-hot Jupiters sample from exoplanets.eu. This sample corresponds to all confirmed planets with equilibrium temperatures larger than 2000 K, which have been detected via radial-velocity or transits methods. In the horizontal axis we show the equilibrium temperatureof the planet, and in the vertical axis the stellar effective temperature. The semi-major axes of the systems are colour-coded in the side bar (in AU). Some names of UHJs’ host stars mentioned in this paper are shown as reference.

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