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| Kepler-328b , the SIMBAD biblio (17 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:22:18 |
| 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...784...45R |
15 | D | 1 | 1691 | 388 | Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems. | ROWE J.F., BRYSON S.T., MARCY G.W., 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. | ||
|
2015ApJS..217...31M |
16 | D | 1 | 2033 | 213 | Planetary candidates observed by Kepler. VI. Planet sample from Q1–Q16 (47 months). | MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al. | ||
|
2015ApJ...809....8B |
16 | D | 1 | 112329 | 282 | Terrestrial planet occurrence rates for the Kepler GK dwarf sample. | BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al. | ||
| 2015MNRAS.453.4089S | 16 | D | 1 | 103 | 3 | Tides alone cannot explain Kepler planets close to 2:1 MMR. | SILBURT A. and REIN H. | ||
|
2016AJ....152..158T |
16 | D | 1 | 4388 | 37 | Detection of potential transit signals in 17 quarters of Kepler data: results of the final Kepler mission transiting planet search (DR25). | TWICKEN J.D., JENKINS J.M., SEADER S.E., et al. | ||
|
2017MNRAS.466.1868C |
16 | D | 1 | 176 | 21 | An overabundance of low-density Neptune-like planets. | CUBILLOS P., ERKAEV N.V., JUVAN I., et al. | ||
|
2017A&A...603A..30S |
16 | D | 4 | 2500 | 58 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., 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. | ||
|
2019ApJ...874L..31T |
16 | D | 1 | 403 | 62 | Connecting giant planet atmosphere and interior modeling: constraints on atmospheric metal enrichment. | THORNGREN D. and FORTNEY J.J. | ||
|
2019AJ....157..171K |
16 | D | 1 | 4069 | 2 | Visual analysis and demographics of Kepler transit timing variations. | KANE M., RAGOZZINE D., FLOWERS X., et al. | ||
|
2020AJ....159...41T |
16 | D | 1 | 564 | ~ | Estimating planetary mass with deep learning. | TASKER E.J., LANEUVILLE M. and GUTTENBERG N. | ||
|
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. | ||
|
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. | ||
|
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. | ||
|
2025AJ....169...90O |
19 | D | 1 | 194 | ~ | Planetary Mass Determinations from a Simplified Photodynamical Model-Application to the Complete Kepler Dataset. | OFIR A., YOFFE G. and AHARONSON O. |