TOI-2147 b and TOI-6019 b are confirmed eccentric warm Jupiters with masses of 116 and 149 Earth masses and eccentricities of 0.29 and 0.48.
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Long-term spectroscopy of GJ 436 shows activity modulated by the planet's orbit, yielding a 6-110 G estimate for the warm Neptune's magnetic field via a new geometrical model.
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TOI-2147 b and TOI-6019 b: Two eccentric warm Jupiters detected and characterized with TESS and MaHPS
TOI-2147 b and TOI-6019 b are confirmed eccentric warm Jupiters with masses of 116 and 149 Earth masses and eccentricities of 0.29 and 0.48.
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Planet-induced Periodic Modulation of Stellar Activity in GJ~436: Insights into a Warm Neptune's Magnetic Field
Long-term spectroscopy of GJ 436 shows activity modulated by the planet's orbit, yielding a 6-110 G estimate for the warm Neptune's magnetic field via a new geometrical model.