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| MOA 2007-BLG-197 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST18:45:18 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 2008A&A...491..587C | 16 | 23 | An alternative parameterisation for binary-lens caustic-crossing events. | CASSAN A. | |||||
| 2009MNRAS.397.2099A | 51 | X | 1 | 6 | 178 | Difference imaging photometry of blended gravitational microlensing events with a numerical kernel. | ALBROW M.D., HORNE K., BRAMICH D.M., et al. | ||
| 2010ApJ...716.1408B | 76 | X | 2 | 19 | 52 | An efficient method for modeling high-magnification planetary microlensing events. | BENNETT D.P. | ||
| 2015A&A...580A.125R | 803 | T A | X C | 19 | 20 | 10 |
MOA-2007-BLG-197: Exploring the brown dwarf desert. |
RANC C., CASSAN A., ALBROW M.D., et al. | |
| 2015MNRAS.454..946R | 39 | X | 1 | 7 | 12 | MOA-2010-BLG-353Lb: a possible Saturn revealed. | RATTENBURY N.J., BENNETT D.P., SUMI T., et al. | ||
| 2016ApJ...822...75H | 16 | D | 1 | 17 | 9 | OGLE-2014-BLG-0257L: a microlensing brown dwarf orbiting a low-mass M dwarf. | HAN C., JUNG Y.K., UDALSKI A., et al. | ||
| 2017A&A...604A.103P | 40 | O X | 1 | 14 | 10 | A companion on the planet/brown dwarf mass boundary on a wide orbit discovered by gravitational microlensing. | POLESKI R., UDALSKI A., BOND I.A., et al. | ||
| 2019ApJ...871..179C | 16 | D | 1 | 21 | 3 | Spitzer microlensing of MOA-2016-BLG-231L: a counter-rotating brown dwarf binary in the Galactic disk. | CHUNG S.-J., GOULD A., SKOWRON J., et al. | ||
2022A&A...663A.100H 
|
17 | D | 1 | 9 | 1 | Precision measurement of a brown dwarf mass in a binary system in the microlensing event. OGLE-2019-BLG-0033/MOA-2019-BLG-035. | HERALD A., UDALSKI A., BOZZA V., et al. | ||
| 2025ApJ...995L..55Z | 65 | D | X | 2 | 18 | ~ | The Brown-dwarf Desert Persists as a Mass-ratio Desert around Low-mass Stars. | ZHANG K. |
