OGLE-2016-BLG-0613 , the SIMBAD biblio

OGLE-2016-BLG-0613 , the SIMBAD biblio (29 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST11:20:44


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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 viz 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 viz 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 viz 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 viz 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 viz 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.

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