A probability theoretical method is presented which enables the calculation of microlensing autocorrelation functions. Following an idea of Deguchi and Watson the Holtsmark–Markov method is employed to reduce this calculation to the numerical evaluation of twodimensional integrals. Comparing these results with autocorrelation functions calculated from measurements, consistent preliminary information about the individual lens system B1600+43
It has been conjectured that the distribution of magnifications of a point source microlensed by a p...
Cosmological gravitational microlensing is a useful technique for understanding the structure of the...
We discuss the results of the MEGA microlensing campaign towards M 31. Our analysis is based on anal...
A method to calculate the statistical properties of microlensing light curves is developed. The appr...
The passage of stars through the beam of a lensed quasar can induce violent fluctuations in its appa...
Gravitational microlensing is a key probe of the nature of dark matter and its distribution on the s...
International audienceMicrolensing of extragalactic sources, in particular the probability of signif...
A comprehensive new approach is presented for deriving probability densities of physical properties ...
A comprehensive new approach is presented for deriving probability densities of physical properties ...
<p>Stochastic microlensing is a central tool in probing dark matter on galactic scales. From first p...
Theoretical investigations into the deflection angle caused by microlenses offer a direct path to un...
The phenomena of gravitational microlensing are described, and predictions are made about its possib...
The phenomena of gravitational microlensing are described, and predictions are made about its possib...
Received; accepted Aims. Caustic-crossing binary-lens microlensing events are important anomalous ev...
We present a new and very fast method for producing microlensing magnification maps at high optical ...
It has been conjectured that the distribution of magnifications of a point source microlensed by a p...
Cosmological gravitational microlensing is a useful technique for understanding the structure of the...
We discuss the results of the MEGA microlensing campaign towards M 31. Our analysis is based on anal...
A method to calculate the statistical properties of microlensing light curves is developed. The appr...
The passage of stars through the beam of a lensed quasar can induce violent fluctuations in its appa...
Gravitational microlensing is a key probe of the nature of dark matter and its distribution on the s...
International audienceMicrolensing of extragalactic sources, in particular the probability of signif...
A comprehensive new approach is presented for deriving probability densities of physical properties ...
A comprehensive new approach is presented for deriving probability densities of physical properties ...
<p>Stochastic microlensing is a central tool in probing dark matter on galactic scales. From first p...
Theoretical investigations into the deflection angle caused by microlenses offer a direct path to un...
The phenomena of gravitational microlensing are described, and predictions are made about its possib...
The phenomena of gravitational microlensing are described, and predictions are made about its possib...
Received; accepted Aims. Caustic-crossing binary-lens microlensing events are important anomalous ev...
We present a new and very fast method for producing microlensing magnification maps at high optical ...
It has been conjectured that the distribution of magnifications of a point source microlensed by a p...
Cosmological gravitational microlensing is a useful technique for understanding the structure of the...
We discuss the results of the MEGA microlensing campaign towards M 31. Our analysis is based on anal...
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