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| OGLE-2016-BLG-0613 , the SIMBAD biblio (29 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST11:20:44 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2017AJ....154..223H | 492 | D | X | 13 | 11 | 13 | OGLE-2016-BLG-0613LABb: a microlensing planet in a binary system. | HAN C., UDALSKI A., GOULD A., et al. | |
|
2018ApJS..239...14J |
16 | D | 1 | 1561 | 6 | Revised exoplanet radii and habitability using Gaia data release 2. | JOHNS D., MARTI C., HUFF M., et al. | ||
| 2019ApJ...880...72D | 41 | X | 1 | 8 | ~ | Triple-lens gravitational microlensing: critical curves for arbitrary spatial configuration. | DANEK K. and HEYROVSKY D. | ||
| 2019AJ....158..114H | 41 | X | 1 | 29 | ~ | OGLE-2018-BLG-1011Lb,c: microlensing planetary system with two giant planets orbiting a low-mass star. | HAN C., BENNETT D.P., UDALSKI A., et al. | ||
| 2020AJ....159...48H | 41 | X | 1 | 15 | ~ | OGLE-2018-BLG-1700L: microlensing planet in binary stellar system. | HAN C., LEE C.-U., UDALSKI 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. | ||
| 2020AJ....160...72B | 41 | X | 1 | 15 | ~ | A gas giant planet in the OGLE-2006-BLG-284L stellar binary system. | BENNETT D.P., UDALSKI A., BOND I.A., et al. | ||
| 2020AJ....160..183R | 41 | X | 1 | 23 | ~ | OGLE-2018-BLG-0532Lb: cold Neptune with possible jovian sibling. | RYU Y.-H., UDALSKI A., YEE J.C., et al. | ||
| 2021MNRAS.503.6143K | 84 | X | 2 | 13 | ~ | Light-curve calculations for triple microlensing systems. | KUANG R., MAO S., WANG T., et al. | ||
|
2021AJ....161..270H |
43 | X | 1 | 8 | 11 | KMT-2019-BLG-1715: planetary microlensing event with three lens masses and two source stars. | HAN C., UDALSKI A., KIM D., et al. | ||
| 2021A&A...649A..91H | 100 | D | X | 3 | 26 | ~ | KMT-2019-BLG-0797: Binary-lensing event occurring on a binary stellar system. | HAN C., LEE C.-U., RYU Y.-H., 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. | ||
|
2021AJ....162..203H |
125 | X C | 2 | 12 | 3 | OGLE-2019-BLG-0304: competing interpretations between a planet-binary model and a binary-source + binary-lens model. | HAN C., UDALSKI A., LEE C.-U., et al. | ||
| 2021RAA....21..239Z | 126 | X C | 2 | 17 | 27 | An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb. | ZANG W., HAN C., KONDO I., et al. | ||
| 2021A&A...655A..24H | 84 | X | 2 | 11 | 4 | KMT-2021-BLG-0322: Severe degeneracy between triple-lens and higher-order binary-lens interpretations. | HAN C., GOULD A., HIRAO Y., 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...663A.145H | 43 | X | 1 | 16 | 7 | KMT-2021-BLG-1898: Planetary microlensing event involved with binary source stars. | HAN C., GOULD A., KIM D., et al. | ||
| 2022A&A...664A.114H | 43 | X | 1 | 19 | 7 | KMT-2021-BLG-0240: Microlensing event with a deformed planetary signal. | HAN C., KIM D., YANG H., et al. | ||
| 2022MNRAS.516.1704K | 213 | X C | 4 | 20 | 5 | OGLE-2019-BLG-1470LABc: Another microlensing giant planet in a binary system? | KUANG R., ZANG W., JUNG Y.K., et al. | ||
| 2023A&A...670A.172H | 17 | D | 1 | 23 | 1 | OGLE-2018-BLG-0584 and KMT-2018-BLG-2119: Two microlensing events with two lens masses and two source stars. | HAN C., UDALSKI A., JUNG Y.K., et al. | ||
| 2023MNRAS.520.4540K | 17 | D | 1 | 23 | ~ | Simulations of triple microlensing events I: detectability of a scaled Sun-Jupiter-Saturn system. | KUANG R., ZANG W., MAO S., et al. | ||
| 2023AJ....166..104S | 104 | D | C | 3 | 34 | ~ | Systematic KMTNet Planetary Anomaly Search. IX. Complete Sample of 2016 Prime-field Planets. | SHIN I.-G., YEE J.C., ZANG W., et al. | |
| 2023A&A...678A.101H | 44 | X | 1 | 21 | ~ | KMT-2021-BLG-1547Lb: Giant microlensing planet detected through a signal deformed due to source binarity. | HAN C., ZANG W., JUNG Y.K., et al. | ||
| 2024AJ....167..269S | 18 | D | 2 | 55 | ~ | Systematic KMTNet Planetary Anomaly Search. XI. Complete Sample of 2016 Subprime Field Planets. | SHIN I.-G., YEE J.C., ZANG W., et al. | ||
| 2024A&A...692A.221H | 18 | D | 1 | 31 | ~ | KMT-2021-BLG-0284, KMT-2022-BLG-2480, and KMT-2024-BLG-0412: Three microlensing events involving two lens masses and two source stars. | HAN C., UDALSKI A., BOND I.A., et al. | ||
| 2025AJ....170...75C | 47 | X | 1 | 19 | ~ | KMT-2022-BLG-0086: Another Binary-lens Binary-source Microlensing Event. | CHUNG S.-J., HWANG K.-H., YEE J.C., et al. | ||
| 2025A&A...700A.181H | 47 | X | 1 | 23 | ~ | KMT-2024-BLG-0404L: A triple microlensing system consisting of a star, a brown dwarf, and a planet. | HAN C., UDALSKI A., LEE C.-U., et al. | ||
| 2025PASP..137j4501H | 93 | X | 2 | 34 | ~ | Three Binary-source Binary-lens Microlensing Events from the 2024 Microlensing Campaign. | HAN C., LEE C.-U., UDALSKI A., et al. | ||
| 2025ApJ...995L..55Z | 205 | D | X | 5 | 18 | ~ | The Brown-dwarf Desert Persists as a Mass-ratio Desert around Low-mass Stars. | ZHANG K. |