Blended light is an important source of degeneracy in the characterization of microlensing events, particularly in binary-lens and high-magnification events. We show how the techniques of image subtraction can be applied to form an image of the blend with the source removed. In many cases, it should be possible to construct images with a very high signal-to-noise ratio. Analysis of these images can help distinguish between competing models that have different blend fractions, and in some cases should allow direct detection of the lens
Microlensing event MACHO 97-SMC-1 is one of the rare microlensing events for which the source is a v...
The light curves of the OGLE microlensing candidates have been reconstructed using the image subtrac...
Detecting color changes of a gravitational microlensing event induced by the limb-darkened extended ...
Blended light is an important source of degeneracy in the characterization of microlensing events, p...
Blended light is an important source of degeneracy in the characterization of microlensing events, p...
The Astrophysical Journal. 498, pp. 156.We discuss the prospect of deblending microlensing events by...
We investigate the effect of blending in future gravitational microlensing surveys by carrying out s...
The biggest uncertainty in determining microlensing parameters comes from the blending of source sta...
The microlensing monitoring programs have studied large numbers of standard light curves which seem ...
We investigate whether the "close/wide" class of degeneracies in caustic-crossing binary microlensin...
Gravitational microlensing surveys target very dense stellar fields in the local group. As a consequ...
Gravitational microlensing surveys target very dense stellar fields in the local group. As a consequ...
Despite the detection of a large number of gravitational microlensing events, the nature of Galactic...
If the objects responsible for gravitational microlensing (ML) of Galactic-bulge stars are faint dwa...
15 text pages + 2 tables + 7 figures. Accepted for publication in ApJ - By EROS-2 Collaboration and ...
Microlensing event MACHO 97-SMC-1 is one of the rare microlensing events for which the source is a v...
The light curves of the OGLE microlensing candidates have been reconstructed using the image subtrac...
Detecting color changes of a gravitational microlensing event induced by the limb-darkened extended ...
Blended light is an important source of degeneracy in the characterization of microlensing events, p...
Blended light is an important source of degeneracy in the characterization of microlensing events, p...
The Astrophysical Journal. 498, pp. 156.We discuss the prospect of deblending microlensing events by...
We investigate the effect of blending in future gravitational microlensing surveys by carrying out s...
The biggest uncertainty in determining microlensing parameters comes from the blending of source sta...
The microlensing monitoring programs have studied large numbers of standard light curves which seem ...
We investigate whether the "close/wide" class of degeneracies in caustic-crossing binary microlensin...
Gravitational microlensing surveys target very dense stellar fields in the local group. As a consequ...
Gravitational microlensing surveys target very dense stellar fields in the local group. As a consequ...
Despite the detection of a large number of gravitational microlensing events, the nature of Galactic...
If the objects responsible for gravitational microlensing (ML) of Galactic-bulge stars are faint dwa...
15 text pages + 2 tables + 7 figures. Accepted for publication in ApJ - By EROS-2 Collaboration and ...
Microlensing event MACHO 97-SMC-1 is one of the rare microlensing events for which the source is a v...
The light curves of the OGLE microlensing candidates have been reconstructed using the image subtrac...
Detecting color changes of a gravitational microlensing event induced by the limb-darkened extended ...