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| NAME LP 759-72c , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST01:07:21 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2016ApJS..226....7C 
|
16 | D | 1 | 400 | 165 | 197 candidates and 104 validated planets in K2's first five fields. | CROSSFIELD I.J.M., CIARDI D.R., PETIGURA E.A., et al. | ||
|
2017AJ....154..207D
|
41 | X | 1 | 118 | 78 | Characterizing K2 candidate planetary systems orbiting low-mass stars. II. Planetary systems observed during campaigns 1-7. | DRESSING C.D., VANDERBURG A., SCHLIEDER J.E., et al. | ||
|
2019MNRAS.485.3999M
|
17 | D | 1 | 474 | ~ | Planetary magnetism as a parameter in exoplanet habitability. | McINTYRE S.R.N., LINEWEAVER C.H. and IRELAND M.J. | ||
| 2019MNRAS.488..633V | 17 | D | 1 | 148 | ~ | Can we detect aurora in exoplanets orbiting M dwarfs? | VIDOTTO A.A., FEENEY N. and GROH J.H. | ||
|
2020AJ....159..211C
|
17 | D | 1 | 351 | 93 | Evolution of the radius valley around low-mass stars from Kepler and K2. | CLOUTIER R. and MENOU K. | ||
| 2020A&A...642A..49D | 85 | F | 1 | 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. | ||
|
2021AJ....162..259Z
|
17 | D | 1 | 1094 | 12 | Scaling K2. IV. A uniform planet sample for Campaigns 1-8 and 10-18. | ZINK J.K., HARDEGREE-ULLMAN K.K., CHRISTIANSEN J.L., et al. | ||
|
2022A&A...662A..15M
|
18 | D | 1 | 733 | 3 | Tidally driven tectonic activity as a parameter in exoplanet habitability. | McINTYRE S.R.N. | ||
| 2023ApJ...957...15A | 19 | D | 2 | 17 | ~ | Detecting Technosignatures from Earth-scale Civilizations. | ASHTARI R. | ||
| 2023A&A...679A.126T | 140 | X F | 2 | 41 | ~ | Water condensation zones around main sequence stars. | TURBET M., FAUCHEZ T.J., LECONTE J., et al. | ||
| 2024ApJ...961...22S | 20 | D | 1 | 42 | ~ | Potential Melting of Extrasolar Planets by Tidal Dissipation. | SELIGMAN D.Z., FEINSTEIN A.D., LAI D., et al. | ||
| 2024ApJ...964L..13S | 50 | X | 1 | 25 | ~ | Predicting the Dominant Formation Mechanism of Multiplanetary Systems. | SHARIAT C., HASEGAWA Y., HANSEN B.M.S., et al. |
