http://arxiv.org/abs/2202.00970
We report the discovery of GJ 3929 b, a hot Earth-sized planet orbiting the nearby M3.5 V dwarf star, GJ 3929 (G 180–18, TOI-2013). Joint modelling of photometric observations from TESS sectors 24 and 25 together with 73 spectroscopic observations from CARMENES and follow-up transit observations from SAINT-EX, LCOGT, and OSN yields a planet radius of $R_b = 1.150 +/- 0.040$ R${earth}$, a mass of $M_b = 1.21 +/- 0.42$ M${earth}$, and an orbital period of $P_b = 2.6162745 +/- 0.0000030$ d. The resulting density of $\rho_b= 4.4 +/- 1.6$ g/cm$^{-3}$ is compatible with the Earth’s mean density of about 5.5 g/cm$^{-3}$. Due to the apparent brightness of the host star (J=8.7 mag) and its small size, GJ 3929 b is a promising target for atmospheric characterisation with the JWST. Additionally, the radial velocity data show evidence for another planet candidate with $P_{[c]} = 14.303 +/- 0.035$ d, which is likely unrelated to the stellar rotation period, $P_{rot} = 122+/-13$ d, which we determined from archival HATNet and ASAS-SN photometry combined with newly obtained TJO data.
J. Kemmer, S. Dreizler, D. Kossakowski, et. al.
Thu, 3 Feb 22
34/56
Comments: 24 pages; accepted for publication in A&A