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| NAME NGC 2682 YBP 1194b , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST23:25:46 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 2014A&A...561L...9B | 17 | D | 1 | 13 | 54 | Three planetary companions around M 67 stars. | BRUCALASSI A., PASQUINI L., SAGLIA R., et al. | ||
| 2017AstL...43..186C | 1 | 1 | 3 | Change in the orbital period of a binary system due to dynamical tides for main-sequence stars. | CHERNOV S.V. | ||||
| 2017MNRAS.470.4337C | 17 | D | 1 | 27 | 59 | Stability of multiplanetary systems in star clusters. | CAI M.X., KOUWENHOVEN M.B.N., PORTEGIES ZWART S.F., et al. | ||
2018MNRAS.475.3090Y 
|
16 | D | 1 | 483 | ~ | Forecasting the detectability of known radial velocity planets with the upcoming CHEOPS mission. | YI J.S., CHEN J. and KIPPING D. | ||
| 2018MNRAS.477..175O | 56 | D | X | 2 | 42 | 2 | Constraining planetary migration and tidal dissipation with coeval hot Jupiters. | O'CONNOR C.E. and HANSEN B.M.S. | |
|
2019PASP..131c4401D
|
16 | D | 1 | 688 | 5 | Predicted yield of transits of known radial velocity exoplanets from the TESS primary and extended missions. | DALBA P.A., KANE S.R., BARCLAY T., et al. | ||
| 2019MNRAS.489.4311C | 17 | D | 1 | 43 | 49 | On the survivability of planets in young massive clusters and its implication of planet orbital architectures in globular clusters. | CAI M.X., PORTEGIES ZWART S., KOUWENHOVEN M.B.N., et al. | ||
| 2020AJ....160..126G | 16 | D | 1 | 45 | ~ | TYCHO: realistically simulating exoplanets within stellar clusters. I. Improving the Monte Carlo approach. | GLASER J.P., McMILLAN S.L.W., GELLER A.M., et al. | ||
| 2023AJ....165...82J | 87 | X | 2 | 167 | 3 | Statistical Analysis of the Dearth of Super-eccentric Jupiters in the Kepler Sample. | JACKSON J.M., DAWSON R.I., QUARLES B., et al. | ||
|
2024AJ....168..115B
|
18 | D | 1 | 224 | ~ | Different Planetary Eccentricity-period (PEP) Distributions of Small and Giant Planets. | BASHI D., MAZEH T. and FAIGLER S. |
