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| KMT-2021-BLG-0171 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST16:37:01 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2022MNRAS.516.1894Y | 1362 | A | D | S X C | 31 | 17 | 8 |
KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: two microlensing planets in the KMTNet high-cadence fields with followup observations. |
YANG H., ZANG W., GOULD A., et al. |
|
2023AJ....165...83R |
87 | X | 2 | 28 | 4 | Mass Production of 2021 KMTNet Microlensing Planets II. | RYU Y.-H., SHIN I.-G., YANG H., et al. | ||
|
2023AJ....165..103Z |
44 | X | 1 | 45 | 8 | Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10–4 Planets from the First 4 yr Survey. | ZANG W., JUNG Y.K., YANG H., et al. | ||
| 2023AJ....166..145G | 44 | X | 1 | 18 | ~ | OGLE-2016-BLG-1195 AO: Lens, Companion to Lens or Source, or None of the Above? | GOULD A., SHVARTZVALD Y., ZHANG J., et al. | ||
| 2024PASP..136e4402B | 45 | X | 1 | 9 | ~ | KMT-2023-BLG-1431Lb: A New q < 10–4 Microlensing Planet from a Subtle Signature. | BELL A., ZHANG J., ZANG W., et al. | ||
| 2024A&A...687A.241H | 18 | D | 1 | 38 | ~ | KMT-2023-BLG-1866Lb: Microlensing super-Earth around an M dwarf host. | HAN C., BOND I.A., UDALSKI A., et al. | ||
| 2024PASP..136i4401H | 627 | S X C F | 11 | 9 | ~ | A New Parameterization for Finding Solutions for Microlensing Exoplanet Light Curves. | HALL K.E., YEE J.C., SHIN I.-G., et al. | ||
| 2025A&A...696A..94D | 19 | D | 1 | 44 | ~ | Earth-like planet predictor: A machine learning approach. | DAVOULT J., ELTSCHINGER R. and ALIBERT Y. | ||
| 2025AJ....170..339S | 19 | D | 1 | 52 | ~ | Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function. | SHANG Y., YANG H., ZHANG J., et al. |