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| Kepler-90c , the SIMBAD biblio (33 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST23:23:26 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2014ApJS..210...19B |
15 | D | 1 | 5860 | 211 | Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). | BURKE C.J., BRYSON S.T., MULLALLY F., et al. | ||
| 2014ApJS..211....6T | 41 | X | 1 | 6 | 31 | Detection of potential transit signals in 16 quarters of Kepler mission data. | TENENBAUM P., JENKINS J.M., SEADER S., et al. | ||
| 2014ApJ...784...44L | 16 | D | 2 | 47 | 179 | Validation of Kepler's multiple planet candidates. II. Refined statistical framework and descriptions of systems of special interest. | LISSAUER J.J., MARCY G.W., BRYSON S.T., et al. | ||
|
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. | ||
|
2014A&A...566A.103L |
15 | D | 1 | 359 | 102 | High-resolution imaging of Kepler planet host candidates. A comprehensive comparison of different techniques. | LILLO-BOX J., BARRADO D. and BOUY H. | ||
| 2014AJ....148...28S | 15 | D | 3 | 34 | 36 | Planet Hunters. VI. An independent characterization of KOI-351 and several long period planet candidates from the Kepler archival data. | SCHMITT J.R., WANG J., FISCHER D.A., 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...18S |
39 | X | 1 | 16 | 16 | Detection of potential transit signals in 17 quarters of Kepler mission data. | SEADER S., JENKINS J.M., TENENBAUM P., 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. | ||
|
2016A&A...587A..64S |
55 | D | X | 2 | 179 | 172 | SOPHIE velocimetry of Kepler transit candidates. XVII. The physical properties of giant exoplanets within 400 days of period. | SANTERNE A., MOUTOU C., TSANTAKI M., 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. | ||
|
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. | ||
| 2018AJ....155...94S | 43 | X | 1 | 51 | 191 | Identifying exoplanets with deep learning: a five-planet resonant chain around Kepler-80 and an eighth planet around Kepler-90. | SHALLUE C.J. and VANDERBURG A. | ||
| 2018AJ....155..139G | 763 | A | D | X C | 19 | 23 | 4 | The dynamics of tightly-packed planetary systems in the presence of an outer planet: case studies using Kepler-11 and Kepler-90. | GRANADOS CONTRERAS A.P. and BOLEY A.C. |
|
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 |
16 | 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 |
16 | 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. | ||
|
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..224R | 140 | D | X | 4 | 9 | ~ | Kepler data analysis: non-Gaussian noise and Fourier Gaussian process analysis of stellar variability. | ROBNIK J. and SELJAK U. | |
|
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. | ||
| 2021MNRAS.504.5829R | 184 | D | C F | 3 | 13 | ~ | Matched filtering with non-Gaussian noise for planet transit detections. | ROBNIK J. and SELJAK U. | |
|
2022AJ....163..179P |
17 | D | 1 | 2962 | 39 | The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age. | PETIGURA E.A., ROGERS J.G., ISAACSON H., et al. | ||
|
2022A&A...662A..15M |
17 | D | 1 | 733 | 3 | Tidally driven tectonic activity as a parameter in exoplanet habitability. | McINTYRE S.R.N. | ||
|
2023MNRAS.519.6210M |
17 | D | 1 | 688 | 1 | A rocky exoplanet classification method and its application to calculating surface pressure and surface temperature. | McINTYRE S.R.N., KING P.L. and MILLS F.P. | ||
|
2023AJ....165..125A |
17 | D | 1 | 578 | ~ | Planetary Orbit Eccentricity Trends (POET). I. The Eccentricity-Metallicity Trend for Small Planets Revealed by the LAMOST-Gaia-Kepler Sample. | AN D.-S., XIE J.-W., DAI Y.-Z., et al. | ||
|
2024ApJS..270....8W |
18 | D | 2 | 250 | ~ | The Kepler Giant Planet Search. I. A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory. | WEISS L.M., ISAACSON H., HOWARD A.W., 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. | ||
| 2024MNRAS.535.3198G | 2643 | A | D | S X C F | 57 | 10 | ~ | Analysing the dynamics of the Kepler-90 planetary system. | GASLAC GALLARDO D.M., GIULIATTI WINTER S.M., WINTER O., et al. |
| 2025MNRAS.538.2730K | 19 | D | 1 | 47 | ~ | Exponential distance relation (aka Titius-Bode rule) in extra solar planetary systems. | KROMMYDAS D. and SCARDIGLI F. | ||
| 2025AJ....170..146S | 47 | X | 1 | 6 | ~ | Updated Masses for the Gas Giants in the Eight-planet Kepler-90 System Via Transit-timing Variation and Radial Velocity Observations. | SHAW D.E., WEISS L.M., AGOL E., et al. |