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| OGLE-2017-BLG-1522 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST20:56:03 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2018AJ....155..219J | 391 | T A | X C | 8 | 4 | 24 |
OGLE-2017-BLG-1522: a giant planet around a brown dwarf located in the Galactic bulge. |
JUNG Y.K., UDALSKI A., GOULD A., et al. | |
| 2019PASP..131k4401T | 41 | X | 1 | 8 | ~ | Design considerations for a ground-based search for transiting planets around L and T dwarfs. | TAMBURO P. and MUIRHEAD P.S. | ||
|
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. | ||
| 2020A&A...641A.105H | 41 | X | 1 | 20 | ~ | KMT-2018-BLG-0748Lb: sub-Saturn microlensing planet orbiting an ultracool host. | HAN C., SHIN I.-G., JUNG Y.K., et al. | ||
|
2021AJ....162...17K |
17 | D | 1 | 54 | ~ | KMT-2019-BLG-0371 and the limits of Bayesian analysis. | KIM Y.H., CHUNG S.-J., YEE J.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. | ||
| 2022A&A...664A..33H | 85 | C | 1 | 36 | 6 | Four sub-Jovian-mass planets detected by high-cadence microlensing surveys. | HAN C., KIM D., GOULD A., et al. | ||
| 2024AJ....167...88R | 18 | D | 2 | 32 | ~ | Systematic KMTNet Planetary Anomaly Search. X. Complete Sample of 2017 Prime-field Planets. | RYU Y.-H., UDALSKI A., YEE J.C., et al. | ||
| 2024A&A...691A.237H | 63 | D | X | 2 | 45 | ~ | Microlensing brown-dwarf companions in binaries detected during the 2022 and 2023 seasons. | HAN C., BOND I.A., UDALSKI A., et al. | |
| 2024A&A...692A.106H | 63 | D | X | 2 | 16 | ~ | KMT-2024-BLG-1044L: A sub-Uranus microlensing planet around a host at the star-brown dwarf mass boundary. | HAN C., RYU Y.-H., LEE C.-U., et al. |