A status report of the microlensing search by the pixel method in the direction of M31, on the 2 meter telescope at Pic du Midi is given. Pixels are stable to a level better than 0.5%. Pixel variations as small as 0.02 magnitude can clearly be detected
We describe the results and outline the methods used in a search for microlensing events affecting s...
We describe a new method to search for gravitational microlensing toward the Galactic bulge that emp...
An automated search is carried out for microlensing events using a catalogue of 44 554 variable supe...
ManuscriptThe M31 galaxy in Andromeda is the nearest large galaxy after the Small and Large Magellan...
We report the discovery of a short-duration microlensing candidate in the Northern field of the POIN...
January 2000 completes the first season of intensive, wide-field observations of microlensing and st...
We detail how microlensing internal to M31 could be used to test whether a large fraction of the mat...
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 Cousin R and I band photometric observations of ~ 13' × 13' field in the direction of M31 galaxy...
We describe the results of a search for microlensing events affecting stars in the outer bulge and i...
AGAPE is an observational search of massive compact halo objects (MACHOs) in the direction of M31 by...
We present WeCAPP, a long term monitoring project searching for microlensing events towards M31. Sin...
The POINT-AGAPE collaboration, an international project looking for gravitational microlensing towar...
We present the rst results of the analysis of data collected during the 1998{99 observational campai...
We describe the results and outline the methods used in a search for microlensing events affecting s...
We describe a new method to search for gravitational microlensing toward the Galactic bulge that emp...
An automated search is carried out for microlensing events using a catalogue of 44 554 variable supe...
ManuscriptThe M31 galaxy in Andromeda is the nearest large galaxy after the Small and Large Magellan...
We report the discovery of a short-duration microlensing candidate in the Northern field of the POIN...
January 2000 completes the first season of intensive, wide-field observations of microlensing and st...
We detail how microlensing internal to M31 could be used to test whether a large fraction of the mat...
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 Cousin R and I band photometric observations of ~ 13' × 13' field in the direction of M31 galaxy...
We describe the results of a search for microlensing events affecting stars in the outer bulge and i...
AGAPE is an observational search of massive compact halo objects (MACHOs) in the direction of M31 by...
We present WeCAPP, a long term monitoring project searching for microlensing events towards M31. Sin...
The POINT-AGAPE collaboration, an international project looking for gravitational microlensing towar...
We present the rst results of the analysis of data collected during the 1998{99 observational campai...
We describe the results and outline the methods used in a search for microlensing events affecting s...
We describe a new method to search for gravitational microlensing toward the Galactic bulge that emp...
An automated search is carried out for microlensing events using a catalogue of 44 554 variable supe...