|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| OGLE BLG249.2 60315 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:27:03 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2004ApJ...614..404G | 3 | 3 | 34 | The mass of the MACHO-LMC-5 lens star. | GOULD A., BENNETT D.P. and ALVES D.R. | ||||
| 2004ApJ...615..450G | 1 | 4 | 20 | Potential direct single-star mass measurement. | GHOSH H., DEPOY D.L., GAL-YAM A., et al. | ||||
| 2004ApJ...617.1307J | 1 | 7 | 30 | OGLE-2003-BLG-238: microlensing mass estimate of an isolated star. | JIANG G., DEPOY D.L., GAL-YAM A., et al. | ||||
| 2005ApJ...633..914P | 1 | 27 | 110 | Systematic analysis of 22 microlensing parallax candidates. | POINDEXTER S., AFONSO C., BENNETT D.P., et al. | ||||
| 2005MNRAS.361..128S | 29 | 6 | The nature of parallax microlensing events towards the Galactic bulge. | SMITH M.C., BELOKUROV V., EVANS N.W., et al. | |||||
| 2006ApJ...642..842D | 3 | 11 | 110 | Planetary detection efficiency of the magnification 3000 microlensing event OGLE-2004-BLG-343. | DONG S., DEPOY D.L., GAUDI B.S., et al. | ||||
| 2010ApJ...717..435H | 75 | X | 2 | 13 | 4 | Determining the physical lens parameters of the binary gravitational microlensing event MOA-2009-BLG-016. | HWANG K.-H., HAN C., BOND I.A., et al. | ||
2016MNRAS.458.3012W 
|
16 | D | 1 | 62 | 122 | Black hole, neutron star and white dwarf candidates from microlensing with OGLE-III. | WYRZYKOWSKI L., KOSTRZEWA-RUTKOWSKA Z., SKOWRON J., et al. | ||
|
2020A&A...636A..20W
|
17 | D | 1 | 51 | 98 | Constraining the masses of microlensing black holes and the mass gap with Gaia DR2. | WYRZYKOWSKI L. and MANDEL I. |
