NAME PM J13119+6550b , the SIMBAD biblio

NAME PM J13119+6550b , the SIMBAD biblio (16 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST09:10:51


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Title First 3 Authors
2020A&A...642A..49D 2017     A D S   X C F     47 56 48 A super-Earth and a sub-Neptune orbiting the bright, quiet M3 dwarf TOI-1266. DEMORY B.-O., POZUELOS F.J., GOMEZ MAQUEO CHEW Y., et al.
2020AJ....160..259S viz 329           X C       7 23 11 A mini-Neptune and a radius valley planet orbiting the nearby M2 dwarf TOI-1266 in its Venus zone: validation with the Habitable-zone Planet Finder. STEFANSSON G., KOPPARAPU R., LIN A., et al.
2021ApJS..254...39G viz 17       D               1 2206 165 The TESS Objects of Interest Catalog from the TESS Prime Mission. GUERRERO N.M., SEAGER S., HUANG C.X., et al.
2022A&A...661A.101R viz 17       D               1 66 1 Internal structures and magnetic moments of rocky planets. Application to the first exoplanets discovered by TESS. RODRIGUEZ-MOZOS J.M. and MOYA A.
2022Sci...377.1211L viz 44           X         1 35 50 Density, not radius, separates rocky and water-rich small planets orbiting M dwarf stars. LUQUE R. and PALLE E.
2023AJ....165...84M 44           X         1 19 1 Hubble Space Telescope Transmission Spectroscopy for the Temperate Sub-Neptune TOI-270 d: A Possible Hydrogen-rich Atmosphere Containing Water Vapor. MIKAL-EVANS T., MADHUSUDHAN N., DITTMANN J., et al.
2023AJ....166..137R 17       D               1 81 ~ A Comparison of the Composition of Planets in Single-planet and Multiplanet Systems Orbiting M dwarfs. RODRIGUEZ MARTINEZ R., MARTIN D.V., GAUDI B.S., et al.
2024AJ....167....1W viz 18       D               1 336 ~ A Blind Search for Transit Depth Variability with TESS. WANG G. and ESPINOZA N.
2024MNRAS.527.5464C 2195     A D     X C F     48 17 ~ Masses, revised radii, and a third planet candidate in the 'Inverted' planetary system around TOI-1266. CLOUTIER R., GREKLEK-MCKEON M., WURMSER S., et al.
2024A&A...685A.143M viz 18       D               1 535 ~ Planets similar in size are often dissimilar in interior. MAMONOVA E., SHAN Y., HATALOVA P., et al.
2024A&A...687L...1L viz 18       D               1 140 ~ Resonant sub-Neptunes are puffier. LELEU A., DELISLE J.-B., BURN R., et al.
2025AJ....169..109T viz 886     A D S   X C F     17 3 ~ Revised Masses for Low-density Planets Orbiting the Disordered M-dwarf System TOI-1266. TYLER D., PETIGURA E.A., ROGERS J., et al.
2025A&A...695A.253D 19       D               1 60 ~ No robust statistical evidence for a population of water worlds in a 2025 sample of planets orbiting M stars. DAINESE S. and ALBRECHT S.H.
2025AJ....169..292G 7931     A D     X C F     169 16 ~ Tidally Heated Sub-Neptunes, Refined Planetary Compositions, and Confirmation of a Third Planet in the TOI-1266 System. GREKLEK-MCKEON M., VISSAPRAGADA S., KNUTSON H.A., et al.
2025ApJ...993..233W viz 19       D               1 391 ~ An Analysis of the Radius Gap in a Sample of Kepler, K2, and TESS Exoplanets Orbiting M-dwarf Stars. WANDERLEY F., CUNHA K., SMITH V.V., 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.

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