AGAPE is an observational search of massive compact halo objects (MACHOs) in the direction of M31 by means of a novel method: the gravitational microlensing of unresolved stars. The search consists in examining CCD pixel light curves for microlensing features. The high level of temporal stability necessary to detect microlensing events has been achieved, with quiet pixels stable within a factor of two of the photon noise (the brightest ones down to a level of 0.001 mag). The data analysis is still in progress, but hundreds of variable objects (cepheids, novae, ...) have already been found. Among them there are several lightcurves that resemble microlensing events
We present the first results of the analysis of data collected during the 1998{99 observational camp...
An automated search is carried out for microlensing events using a catalogue of 44 554 variable supe...
One of the most important problems in astrophysics concerns the nature of the dark matter in galacti...
We report the discovery of a short-duration microlensing candidate in the Northern field of the POIN...
A status report of the microlensing search by the pixel method in the direction of M31, on the 2 met...
An automated search is carried out for microlensing events using a catalogue of 44 554 variable supe...
The aim of the AGAPE (Andromeda Gravitational Amplification Pixel Experiment), experiment which has ...
We describe a new method to search for gravitational microlensing toward the Galactic bulge that emp...
ManuscriptThe M31 galaxy in Andromeda is the nearest large galaxy after the Small and Large Magellan...
Pixel lensing is gravitational microlensing of unresolved stars. The main target explored up to now ...
membres du jury : Pierre Encrenaz (directeur du jury) - Alain Falvard - Andrew Gould - Jean Kaplan (...
The POINT-AGAPE collaboration, an international project looking for gravitational microlensing towar...
We present WeCAPP, a long term monitoring project searching for microlensing events towards M31. Sin...
Gravitational microlensing has generated a great deal of scientific interest over recent years. Thi...
Microlensing has established itself as a powerful new method for the detection of baryonic dark matt...
We present the first results of the analysis of data collected during the 1998{99 observational camp...
An automated search is carried out for microlensing events using a catalogue of 44 554 variable supe...
One of the most important problems in astrophysics concerns the nature of the dark matter in galacti...
We report the discovery of a short-duration microlensing candidate in the Northern field of the POIN...
A status report of the microlensing search by the pixel method in the direction of M31, on the 2 met...
An automated search is carried out for microlensing events using a catalogue of 44 554 variable supe...
The aim of the AGAPE (Andromeda Gravitational Amplification Pixel Experiment), experiment which has ...
We describe a new method to search for gravitational microlensing toward the Galactic bulge that emp...
ManuscriptThe M31 galaxy in Andromeda is the nearest large galaxy after the Small and Large Magellan...
Pixel lensing is gravitational microlensing of unresolved stars. The main target explored up to now ...
membres du jury : Pierre Encrenaz (directeur du jury) - Alain Falvard - Andrew Gould - Jean Kaplan (...
The POINT-AGAPE collaboration, an international project looking for gravitational microlensing towar...
We present WeCAPP, a long term monitoring project searching for microlensing events towards M31. Sin...
Gravitational microlensing has generated a great deal of scientific interest over recent years. Thi...
Microlensing has established itself as a powerful new method for the detection of baryonic dark matt...
We present the first results of the analysis of data collected during the 1998{99 observational camp...
An automated search is carried out for microlensing events using a catalogue of 44 554 variable supe...
One of the most important problems in astrophysics concerns the nature of the dark matter in galacti...