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Kepler-450d , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.03.29CET15:53:54 |
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 |
---|---|---|---|---|---|---|---|---|---|
2014ApJ...783....4W | 16 | D | 1 | 487 | 103 | Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates. | WANG J., XIE J.-W., BARCLAY T., et al. | ||
2015ApJS..217...16R | 16 | D | 1 | 8625 | 149 | Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). | ROWE J.F., COUGHLIN J.L., ANTOCI V., et al. | ||
2015ApJ...808..126V | 95 | D | X | 3 | 105 | 201 | Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities. | VAN EYLEN V. and ALBRECHT S. | |
2016AJ....152..143V | 41 | X | 1 | 20 | 32 | The K2-ESPRINT project V: a short-period giant planet orbiting a subgiant star. | VAN EYLEN V., ALBRECHT S., GANDOLFI D., et al. | ||
2017AJ....154..108J | 16 | D | 1 | 3237 | 137 | The California-Kepler Survey. II. Precise physical properties of 2025 Kepler planets and their host stars. | JOHNSON J.A., PETIGURA E.A., FULTON B.J., et al. | ||
2017AJ....154..109F | 16 | D | 1 | 900 | 847 | The California-Kepler Survey. III. A gap in the radius distribution of small planets. | FULTON B.J., PETIGURA E.A., HOWARD A.W., et al. | ||
2017AJ....154..236W | 16 | D | 1 | 34 | 7 | Near mean-motion resonances in the system observed by Kepler: affected by mass accretion and Type I migration. | WANG S. and JI J. | ||
2018AJ....155...48W | 16 | D | 1 | 911 | 204 | The California-Kepler survey. V. Peas in a pod: planets in a Kepler multi-planet system are similar in size and regularly spaced. | WEISS L.M., MARCY G.W., PETIGURA E.A., et al. | ||
2018ApJ...864L..38D | 16 | D | 2 | 109 | 49 | Larger mutual inclinations for the shortest-period planets. | DAI F., MASUDA K. and WINN J.N. | ||
2018MNRAS.479.4786V | 18 | D | 1 | 117 | 318 | An asteroseismic view of the radius valley: stripped cores, not born rocky. | VAN EYLEN V., AGENTOFT C., LUNDKVIST M.S., et al. | ||
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. | ||
2018AJ....156..254W | 16 | D | 2 | 1269 | 42 | The California-Kepler Survey. VI. Kepler multis and singles have similar planet and stellar properties indicating a common origin. | WEISS L.M., ISAACSON H.T., MARCY G.W., et al. | ||
2018AJ....156..264F | 16 | D | 1 | 1909 | 365 | The California-Kepler Survey. VII. Precise planet radii leveraging Gaia DR2 reveal the stellar mass dependence of the Planet radius gap. | FULTON B.J. and PETIGURA E.A. | ||
2019RAA....19...41G | 17 | D | 1 | 1982 | 17 | Transit timing variations and linear ephemerides of confirmed Kepler transiting exoplanets. | GAJDOS P., VANKO M. and PARIMUCHA S. | ||
2019ApJ...875...29M | 17 | D | 1 | 2918 | 72 | A spectroscopic analysis of the California-Kepler Survey sample. I. Stellar parameters, planetary radii, and a slope in the radius gap. | MARTINEZ C.F., CUNHA K., GHEZZI L., 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. | ||
2020MNRAS.491.5287O | 17 | D | 1 | 127 | 43 | Testing exoplanet evaporation with multitransiting systems. | OWEN J.E. and CAMPOS ESTRADA B. | ||
2021ApJ...908..114Y | 192 | D | X C | 4 | 16 | 9 | A simplified photodynamical model for planetary mass determination in low-eccentricity multitransiting systems. | YOFFE G., OFIR A. and AHARONSON O. | |
2022AJ....163...91J | 90 | X | 2 | 248 | ~ | Physical properties and impact parameter variations of Kepler planets from analytic light-curve modeling. | JUDKOVSKY Y., OFIR A. and AHARONSON O. | ||
2022A&A...662A..15M | 18 | D | 1 | 733 | 3 | Tidally driven tectonic activity as a parameter in exoplanet habitability. | McINTYRE S.R.N. | ||
2022ApJS..261...26S | 18 | D | 4 | 1893 | 2 | Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys. | SU T., ZHANG L.-Y., LONG L., et al. |