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| MOA 2014-BLG-175 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:42:20 |
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More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2016MNRAS.457.4089S 
|
94 | D | F | 3 | 31 | 60 | The frequency of snowline-region planets from four years of OGLE-MOA-Wise second-generation microlensing. | SHVARTZVALD Y., MAOZ D., UDALSKI A., et al. | |
| 2016ApJ...833..145S | 80 | X | 2 | 64 | 176 | The exoplanet mass-ratio function from the MOA-II survey: discovery of a break and likely peak at a Neptune mass. | SUZUKI D., BENNETT D.P., SUMI T., et al. | ||
| 2017MNRAS.466.2710R | 1191 | X C | 29 | 8 | 3 | Faint-source-star planetary microlensing: the discovery of the cold gas-giant planet OGLE-2014-BLG-0676Lb. | RATTENBURY N.J., BENNETT D.P., SUMI T., 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. | ||
|
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. | ||
| 2021RAA....21..303X | 334 | X C | 7 | 3 | ~ | Characterizing microlensing planetary system OGLE-2014-BLG-0676Lb with adaptive optics imaging. | XIE X.-J., DONG S., SHVARTZVALD 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. | ||
| 2022NatAs...6..782Z | 85 | C | 1 | 31 | 15 | A ubiquitous unifying degeneracy in two-body microlensing systems. | ZHANG K., GAUDI B.S. and BLOOM J.S. | ||
|
2023A&A...674A..15L
|
17 | D | 1 | 1720610 | 15 | Gaia Data Release 3 The second Gaia catalogue of long-period variable candidates. | LEBZELTER T., MOWLAVI N., LECOEUR-TAIBI I., et al. |
