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| OGLE-2015-BLG-1482 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST01:45:02 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2015ApJ...814...92C |
16 | D | 1 | 171 | 31 | Spitzer IRAC photometry for time series in crowded fields. | CALCHI NOVATI S., GOULD A., YEE J.C., et al. | ||
| 2016ApJ...825...60Z | 81 | C | 1 | 7 | 34 | Mass measurements of isolated objects from space-based microlensing. | ZHU W., CALCHI NOVATI S., GOULD A., et al. | ||
| 2017ApJ...838..154C | 977 | T A | X C | 23 | 15 | 22 | OGLE-2015 the first isolated low-mass microlens in the Galactic bulge. | CHUNG S.-J., ZHU W., UDALSKI A., et al. | |
| 2017PASP..129j4501Z | 80 | C | 1 | 5 | 11 | Extracting microlensing signals from K2 Campaign 9. | ZHU W., HUANG C.X., UDALSKI A., et al. | ||
|
2017AJ....154..210Z |
95 | D | X | 3 | 75 | 40 | Toward a Galactic distribution of planets. I. Methodology and planet sensitivities of the 2015 high-cadence Spitzer microlens sample. | ZHU W., UDALSKI A., CALCHI NOVATI S., et al. | |
| 2018AJ....155..261C | 80 | C | 1 | 15 | 8 | Spitzer opens new path to break classic degeneracy for Jupiter-mass microlensing planet OGLE-2017-BLG-1140Lb. | CALCHI NOVATI S., SKOWRON J., JUNG Y.K., et al. | ||
| 2018ApJ...867..136H | 80 | C | 1 | 21 | 4 | OGLE-2017-BLG-0039: microlensing event with light from a lens identified from mass measurement. | HAN C., JUNG Y.K., UDALSKI A., et al. | ||
|
2020ApJ...891....3Z |
123 | X | 3 | 13 | ~ | Spitzer microlensing parallax reveals two isolated stars in the Galactic bulge. | ZANG W., SHVARTZVALD Y., WANG T., et al. | ||
| 2023AJ....166..100G | 44 | X | 1 | 18 | ~ | KMT-2022-BLG-2397: Brown Dwarf at the Upper Shore of the Einstein Desert. | GOULD A., RYU Y.-H., YEE J.C., et al. | ||
| 2023A&A...678A.190H | 44 | X | 1 | 25 | ~ | Brown dwarf companions in binaries detected in the 2021 season high-cadence microlensing surveys. | HAN C., JUNG Y.K., BOND I.A., et al. |