OGLE-2017-BLG-0173 , the SIMBAD biblio

OGLE-2017-BLG-0173 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST01:39:51

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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
2018AJ....155...20H 500       D     X C       12 8 22 OGLE-2017-BLG-0173Lb: low-mass-ratio planet in a "hollywood" microlensing event. HWANG K.-H., UDALSKI A., SHVARTZVALD Y., et al.
2018AJ....156..113B 40           X         1 21 9 A planetary microlensing event with an unusually red source star: MOA-2011-BLG-291. BENNETT D.P., UDALSKI A., BOND I.A., et al.
2018AJ....156..226H 40           X         1 17 4 MOA-2016-BLG-319Lb: microlensing planet subject to rare minor-image perturbation degeneracy in determining planet parameters. HAN C., BOND I.A., GOULD A., et al.
2018AcA....68...43S 1 7 10 OGLE-2017-BLG-0373Lb: a Jovian mass-ratio planet exposes a new accidental microlensing degeneracy. SKOWRON J., RYU Y.-H., HWANG K.-H., et al.
2019AJ....157...72J 41           X         1 32 7 KMT-2017-BLG-0165Lb: a super-Neptune-mass planet orbiting a Sun-like host star. JUNG Y.K., GOULD A., ZANG W., et al.
2018AcA....68....1U 646           X         16 13 53 OGLE-2017-BLG-1434Lb: eighth q<1×10–4 mass-ratio microlens planet confirms turnover in planet mass-ratio function. UDALSKI A., RYU Y.-H., SAJADIAN S., 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...64H 41           X         1 10 ~ KMT-2019-BLG-1339L: an M dwarf with a giant planet or a companion near the Planet/Brown dwarf boundary. HAN C., KIM D., UDALSKI A., et al.
2020AJ....160..255J viz 82             C       1 7 ~ KMT-2019-BLG-0842Lb: a cold planet below the Uranus/Sun mass ratio. JUNG Y.K., UDALSKI A., ZANG W., et al.
2021AJ....161..293J viz 85             C       1 27 27 OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: two microlensing planets through the planetary-caustic channel. JUNG Y.K., HAN C., UDALSKI A., 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..163Z viz 85             C       1 20 32 Systematic KMTNet planetary anomaly search. I. OGLE-2019-BLG-1053Lb, a buried terrestrial planet. ZANG W., HWANG K.-H., UDALSKI A., et al.
2021RAA....21..239Z 85             C       1 17 27 An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb. ZANG W., HAN C., KONDO I., 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.
2022MNRAS.514.5952Z 298           X C       6 20 11 OGLE-2018-BLG-0799Lb: a q ∼ 2.7 x 10–3 planet with Spitzer parallax. ZANG W., SHVARTZVALD Y., UDALSKI A., et al.
2023AJ....165..103Z viz 235       D     X         6 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.
2023A&A...675A..36H 44           X         1 20 ~ KMT-2021-BLG-1150Lb: Microlensing planet detected through a densely covered planetary-caustic signal. HAN C., JUNG Y.K., BOND I.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...687A.241H 90             C       1 38 ~ KMT-2023-BLG-1866Lb: Microlensing super-Earth around an M dwarf host. HAN C., BOND I.A., UDALSKI A., et al.
2024A&A...689A.209H 90           X         2 31 ~ KMT-2021-BLG-2609Lb and KMT-2022-BLG-0303Lb: Microlensing planets identified through signals produced by major-image perturbations. HAN C., ALBROW M.D., LEE C.-U., et al.
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.

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