If they are located at cosmological distances, a small fraction of gamma-ray bursts should be multiply imaged by intervening galaxies or clusters, resulting in the appearance of two very similar bursts from the same location with a relative time delay of hours to a year. We show that microlensing by individual stars in the lensing galaxy can smear out the light curves of the multiply imaged bursts on millisecond time-scales. Therefore, in deciding whether two bursts are similar enough to qualify as multiple images, one must look at time-scales longer than a few tens of milliseconds, since shorter time-scales are possibly rendered dissimilar by microlensing
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...
If the objects responsible for gravitational microlensing (ML) of Galactic-bulge stars are faint dwa...
If at cosmological distances, a small fraction of gamma-ray bursts should be multiply imaged by inte...
The microlensing effect has developed into a powerful technique for a diverse range of applications ...
The advent of large area photometric surveys has raised a great deal of interest in the possibility ...
Time-delay cosmography in strongly lensed quasars offers an independent way of measuring the Hubble ...
The afterglow of a cosmological Gamma-Ray Burst (GRB) should appear on the sky as a narrow emission ...
Owing to the advent of large area photometric surveys, the possibility to use broad band photometric...
In microlensing of a Galactic star by a brown dwarf or other compact object, the amplified image rea...
We have searched for microlensing variability in the light curves of five gravitationally lensed qua...
The microlensing interpretation of the optical afterglow of GRB 000301C seems naively surprising, si...
In the next future, astrometric microlensing will offer a new channel for investigating the nature o...
Changes of the magnification ratio of images in a lensed blazar, caused by microlensing on individua...
Photometric monitoring of lensed quasars is now performed by several teams around the world in order...
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...
If the objects responsible for gravitational microlensing (ML) of Galactic-bulge stars are faint dwa...
If at cosmological distances, a small fraction of gamma-ray bursts should be multiply imaged by inte...
The microlensing effect has developed into a powerful technique for a diverse range of applications ...
The advent of large area photometric surveys has raised a great deal of interest in the possibility ...
Time-delay cosmography in strongly lensed quasars offers an independent way of measuring the Hubble ...
The afterglow of a cosmological Gamma-Ray Burst (GRB) should appear on the sky as a narrow emission ...
Owing to the advent of large area photometric surveys, the possibility to use broad band photometric...
In microlensing of a Galactic star by a brown dwarf or other compact object, the amplified image rea...
We have searched for microlensing variability in the light curves of five gravitationally lensed qua...
The microlensing interpretation of the optical afterglow of GRB 000301C seems naively surprising, si...
In the next future, astrometric microlensing will offer a new channel for investigating the nature o...
Changes of the magnification ratio of images in a lensed blazar, caused by microlensing on individua...
Photometric monitoring of lensed quasars is now performed by several teams around the world in order...
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...
If the objects responsible for gravitational microlensing (ML) of Galactic-bulge stars are faint dwa...