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| NAME PM J13119+6550b , the SIMBAD biblio (16 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST09:10:51 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
18 | D | 1 | 140 | ~ | Resonant sub-Neptunes are puffier. | LELEU A., DELISLE J.-B., BURN R., et al. | ||
|
2025AJ....169..109T |
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 |
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. |