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| Kepler-445d , the SIMBAD biblio (22 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST12:58:06 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2015ApJ...801...18M | 601 | D | X C | 15 | 31 | 39 | Kepler-445, Kepler-446 and the occurrence of compact multiples orbiting mid-M dwarf stars. | MUIRHEAD P.S., MANN A.W., VANDERBURG A., et al. | |
|
2015ApJS..218...26S |
55 | D | X | 2 | 275 | 13 | Characterizing the cool KOIs. VIII. Parameters of the planets orbiting Kepler's coolest dwarfs. | SWIFT J.J., MONTET B.T., VANDERBURG A., et al. | |
| 2016ApJ...820...41H | 80 | F | 1 | 18 | 37 | The K2-ESPRINT project III: a close-in super-earth around a metal-rich mid-M dwarf. | HIRANO T., FUKUI A., MANN A.W., et al. | ||
| 2017AJ....153...59D | 238 | X C | 5 | 26 | 3 | Kepler transit depths contaminated by a phantom star. | DALBA P.A., MUIRHEAD P.S., CROLL B., et al. | ||
| 2017AJ....153..267M | 16 | D | 2 | 42 | 16 | The gold standard: accurate stellar and planetary parameters for eight Kepler M dwarf systems enabled by parallaxes. | MANN A.W., DUPUY T., MUIRHEAD P.S., et al. | ||
| 2017MNRAS.471.4628R | 56 | D | X | 2 | 28 | 10 | Statistical-likelihood Exo-Planetary Habitability Index (SEPHI). | RODRIGUEZ-MOZOS J.M. and MOYA A. | |
|
2018ApJ...866...99B |
16 | D | 1 | 7129 | 233 | Revised radii of Kepler stars and planet's using Gaia Data Release 2. | BERGER T.A., HUBER D., GAIDOS E., et al. | ||
|
2019AJ....157..143B |
179 | D | X | 5 | 423 | 5 | Re-evaluating small long-period confirmed planets from Kepler. | BURKE C.J., MULLALLY F., THOMPSON S.E., et al. | |
|
2019AJ....157..235C |
16 | D | 2 | 415 | 7 | Observations of the Kepler field with TESS: predictions for planet yield and observable features. | CHRIST C.N., MONTET B.T. and FABRYCKY D.C. | ||
|
2019AJ....158...75H |
16 | D | 2 | 581 | 108 | Kepler planet occurrence rates for mid-type M dwarfs as a function of spectral type. | HARDEGREE-ULLMAN K.K., CUSHING M.C., MUIRHEAD P.S., 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. | ||
| 2020AJ....159..207B | 16 | D | 1 | 150 | ~ | Transit duration variations in multiplanet systems. | BOLEY A.C., VAN LAERHOVEN C. and GRANADOS CONTRERAS A.P. | ||
|
2020AJ....159..239G |
16 | D | 1 | 1408 | ~ | Updated parameters and a new transmission spectrum of HD 97658b. | GUO X., CROSSFIELD I.J.M., DRAGOMIR D., et al. | ||
|
2020AJ....160..108B |
16 | D | 1 | 6855 | 109 | The Gaia-Kepler stellar properties catalog. II. Planet radius demographics as a function of stellar mass and age. | BERGER T.A., HUBER D., GAIDOS E., et al. | ||
| 2020RNAAS...4...32B | 41 | X | 1 | 3 | ~ | Exoplanet Occurrence Rates of Mid M-dwarfs Based on Kepler DR25. | BRYSON S. | ||
| 2020AJ....160..172N | 82 | F | 1 | 32 | ~ | π Earth: a 3.14 day Earth-sized planet from K2's kitchen served warm by the SPECULOOS team. | NIRAULA P., DE WIT J., RACKHAM B.V., et al. | ||
|
2022AJ....163...91J |
17 | D | 1 | 504 | ~ | Physical properties and impact parameter variations of Kepler planets from analytic light-curve modeling. | JUDKOVSKY Y., OFIR A. and AHARONSON O. | ||
|
2022A&A...667A..59D |
85 | F | 1 | 34 | 18 | Two temperate super-Earths transiting a nearby late-type M dwarf. | DELREZ L., MURRAY C.A., POZUELOS F.J., et al. | ||
| 2023ApJ...957...15A | 17 | D | 2 | 17 | ~ | Detecting Technosignatures from Earth-scale Civilizations. | ASHTARI R. | ||
| 2023A&A...679A.126T | 131 | X F | 2 | 41 | ~ | Water condensation zones around main sequence stars. | TURBET M., FAUCHEZ T.J., LECONTE J., 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. |