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| NAME UKIRT 2017-BLG-001 , the SIMBAD biblio (5 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST15:45:21 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2018ApJ...857L...8S | 227 | A | X C | 5 | 5 | 11 |
UKIRT-2017-BLG-001Lb: a giant planet detected through the dust. |
SHVARTZVALD Y., CALCHI NOVATI S., GAUDI B.S., et al. | |
| 2019MNRAS.488.3308L | 41 | X | 1 | 5 | 2 | OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing. | LI S.-S., ZANG W., UDALSKI A., et al. | ||
| 2020AJ....159...58R | 41 | X | 1 | 15 | ~ | KMT-2018-BLG-1292: a super-Jovian microlens planet in the Galactic plane. | RYU Y.-H., NAVARRO M.G., GOULD A., et al. | ||
2020ApJ...890...23L 
|
16 | D | 1 | 4936 | 35 | Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. | LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al. | ||
| 2022NatAs...6..121C | 17 | D | 1 | 115 | 8 | Microlensing mass measurement from images of rotating gravitational arcs. | CASSAN A., RANC C., ABSIL O., et al. |
