TOI-4860 , the SIMBAD biblio

TOI-4860 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST14:34:54


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Title First 3 Authors
2021A&A...649A...6G viz 17       D               1 227180 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.
2023MNRAS.521.3663B 366       D     X   F     8 38 8 The occurrence rate of giant planets orbiting low-mass stars with TESS. BRYANT E.M., BAYLISS D. and VAN EYLEN V.
2023MNRAS.525L..98T 696           X         16 18 ~ An M dwarf accompanied by a close-in giant orbiter with SPECULOOS. TRIAUD A.H.M.J., DRANSFIELD G., KAGETANI T., et al.
2024A&A...683A.166A viz 179   K       X C       3 24 ~
TOI-4860 b, a short-period giant planet transiting an M3.5 dwarf.
ALMENARA J.M., BONFILS X., BRYANT E.M., et al.
2024A&A...689A..53B viz 18       D               1 194 ~ The TROY project III. Exploring co-orbitals around low-mass stars. BALSALOBRE-RUZA O., LILLO-BOX J., BARRADO D., et al.
2024A&A...689A.302G viz 18       D               1 1270 ~ Multiplicity of stars with planets in the solar neighbourhood. GONZALEZ-PAYO J., CABALLERO J.A., GORGAS J., et al.
2024AJ....168..202H viz 45           X         1 26 ~ TOI 762 A b and TIC 46432937 b: Two Giant Planets Transiting M-dwarf Stars. HARTMAN J.D., BAYLISS D., BRAHM R., et al.
2024A&A...691A..53S viz 18       D               1 4078 ~ SWEET-Cat: A view on the planetary mass-radius relation. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al.
2025ApJ...988L...4H 19       D               1 301 ~ Hundreds of TESS Exoplanets Might Be Larger than We Thought. HAN T., ROBERTSON P., BRANDT T.D., et al.
2026AJ....171..115S 20       D               1 126 ~ The Orbital Eccentricity-Radius Relation for Planets Orbiting M Dwarfs. SAGEAR S., BALLARD S., GILBERT G.J., et al.
2026AJ....171..146G 20       D               2 49 ~ Searching for GEMS: The Occurrence of Giant Planets Orbiting M Dwarfs within 100 pc. GLUSMAN R.I., CANAS C.I., KANODIA S., et al.
2026AJ....171..157S 20       D               2 480 ~ Most Hot Jupiters Were Cool Giant Planets for More Than 1 Gyr. SCHMIDT S.P. and SCHLAUFMAN K.C.

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