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| NAME L 788-37b , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST11:33:34 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2018A&A...620A.171L |
345 | A | S X C | 7 | 24 | 15 | The CARMENES search for exoplanets around M dwarfs. The warm super-Earths in twin orbits around the mid-type M dwarfs Ross 1020 (GJ 3779) and LP 819-052 (GJ 1265). | LUQUE R., NOWAK G., PALLE E., et al. | |
|
2019ApJ...880L...1A |
16 | D | 1 | 146 | ~ | A gap in the mass distribution for warm Neptune and terrestrial planets. | ARMSTRONG D.J., MERU F., BAYLISS D., et al. | ||
| 2019MNRAS.488..633V | 16 | D | 1 | 148 | ~ | Can we detect aurora in exoplanets orbiting M dwarfs? | VIDOTTO A.A., FEENEY N. and GROH J.H. | ||
|
2019ApJ...887..261M |
16 | D | 1 | 329 | 29 | Exomoons in the habitable zones of M dwarfs. | MARTINEZ-RODRIGUEZ H., CABALLERO J.A., CIFUENTES C., et al. | ||
|
2020A&A...644A..68M |
16 | D | 1 | 312 | 28 | HADES RV programme with HARPS-N at TNG. XII. The abundance signature of M dwarf stars with planets. | MALDONADO J., MICELA G., BARATELLA M., et al. | ||
| 2022A&A...664A.180S | 17 | D | 1 | 188 | 15 | RV-detected planets around M dwarfs: Challenges for core accretion models. | SCHLECKER M., BURN R., SABOTTA S., et al. | ||
| 2022AJ....164..176M | 17 | D | 2 | 44 | 3 | MIRECLE: Science Yield for a Mid-infrared Explorer-class Mission to Study Nontransiting Rocky Planets Orbiting the Nearest M Stars Using Planetary Infrared Excess. | MANDELL A.M., LUSTIG-YAEGER J., STEVENSON K.B., et al. | ||
|
2023A&A...678A..96C |
17 | D | 1 | 305 | ~ | Large Interferometer For Exoplanets (LIFE) X. Detectability of currently known exoplanets and synergies with future IR/O/UV reflected-starlight imaging missions. | CARRION-GONZALEZ O., KAMMERER J., ANGERHAUSEN D., et al. | ||
|
2023Sci...382.1031S |
87 | F | 1 | 12 | ~ | A Neptune-mass exoplanet in close orbit around a very low-mass star challenges formation models. | STEFANSSON G., MAHADEVAN S., MIGUEL Y., et al. |