The Astrophysical Journal. 48, pp. 19.We measure the astrometric shifts of the light centroids for the microlensing events in the OGLE-1 database. Of the 15 consistently detected events, 7 had significant shifts which we were able to measure with a fair degree of confidence. Those events with large shifts are also expected to be unresolved with a background “blend”, and thus, we suggest that we have identified events in the OGLE-1 catalog which are strongly blended. Though we concentrate on the OGLE-1 database, and use the DoPHOT package in order to perform our analysis, we suggest that this shift is a generic effect, and should be observable in any crowded field
© 2018. The American Astronomical Society. All rights reserved. We present an analysis of the binary...
We present an analysis of OGLE 2004-BLG-254, a high-magnification and relatively short duration micr...
The light curves of the OGLE microlensing candidates have been reconstructed using the image subtrac...
The Astrophysical Journal. 498, pp. 156.We discuss the prospect of deblending microlensing events by...
We present the first systematic search for microlensing events with variability in their baselines u...
If the objects responsible for gravitational microlensing (ML) of Galactic-bulge stars are faint dwa...
We investigate the effect of blending in future gravitational microlensing surveys by carrying out s...
We present a sample of microlensing events discovered in the Difference Image Analysis (DIA) of the ...
We present a systematic search for parallax microlensing events among a total of 512 microlensing ca...
Gravitational microlensing surveys target very dense stellar fields in the local group. As a consequ...
In the next future, astrometric microlensing will offer a new channel for investigating the nature o...
In this work, we present the analysis of the binary microlensing event OGLE-2018-BLG-0022 that is de...
Gravitational microlensing is a rare event in which the light from a foreground star (source star) i...
In this paper, we study the astrometric properties of gravitational microlensing events caused by bi...
Because of dramatic improvements in the precision of astrometric measurements, the observation of li...
© 2018. The American Astronomical Society. All rights reserved. We present an analysis of the binary...
We present an analysis of OGLE 2004-BLG-254, a high-magnification and relatively short duration micr...
The light curves of the OGLE microlensing candidates have been reconstructed using the image subtrac...
The Astrophysical Journal. 498, pp. 156.We discuss the prospect of deblending microlensing events by...
We present the first systematic search for microlensing events with variability in their baselines u...
If the objects responsible for gravitational microlensing (ML) of Galactic-bulge stars are faint dwa...
We investigate the effect of blending in future gravitational microlensing surveys by carrying out s...
We present a sample of microlensing events discovered in the Difference Image Analysis (DIA) of the ...
We present a systematic search for parallax microlensing events among a total of 512 microlensing ca...
Gravitational microlensing surveys target very dense stellar fields in the local group. As a consequ...
In the next future, astrometric microlensing will offer a new channel for investigating the nature o...
In this work, we present the analysis of the binary microlensing event OGLE-2018-BLG-0022 that is de...
Gravitational microlensing is a rare event in which the light from a foreground star (source star) i...
In this paper, we study the astrometric properties of gravitational microlensing events caused by bi...
Because of dramatic improvements in the precision of astrometric measurements, the observation of li...
© 2018. The American Astronomical Society. All rights reserved. We present an analysis of the binary...
We present an analysis of OGLE 2004-BLG-254, a high-magnification and relatively short duration micr...
The light curves of the OGLE microlensing candidates have been reconstructed using the image subtrac...