Add to ORKGOne of the possible astrophysical solutions to the galactic dark matter problem is the presence of a significant amount of ``dark'' compact objects (MACHOs) in galactic dark matter halos. MEGA (Microlensing Exploration of the Galaxy and Andromeda) tries to find proof for or against the presence of compact objects in the halo of the Andromeda galaxy (M31) by looking for the microlensing signature that would be induced by these objects. The lightcurves presented here are preliminary and based on observations of M31 with the Isaac Newton Telescope (INT) on La Palma during the second half of 1999
THERE is now abundant evidence for the presence of large quantities of unseen matter surrounding nor...
We detail how microlensing internal to M31 could be used to test whether a large fraction of the mat...
The POINT-AGAPE CollaborationThe POINT-AGAPE collaboration is carrying out a search for gravitationa...
We present the first M 31 candidate microlensing events from the Microlensing Exploration of the Gal...
We present the first M 31 candidate microlensing events from the Microlensing Exploration of the Gal...
We have completed an intensive monitoring program of two fields on either side of the center of M31 ...
Gravitational Microlensing represents an effective tool in searching for non– luminous astrophysical...
We present results of a microlensing survey toward the Andromeda Galaxy (M31) carried out during fou...
We present the first results of the analysis of data collected during the 1998{99 observational camp...
The POINT-AGAPE CollaborationTo reveal the galactic dark matter in the form of MACHOs ("Massive Astr...
We present results of a microlensing survey toward the Andromeda Galaxy (M 31) carried out during fo...
We present results of a microlensing survey toward the Andromeda Galaxy (M31) carried out during fou...
We report the final analysis of a search for microlensing events in the direction of the Andromeda g...
We present results of a microlensing survey toward the Andromeda Galaxy (M 31) carried out during fo...
THERE is now abundant evidence for the presence of large quantities of unseen matter surrounding nor...
We detail how microlensing internal to M31 could be used to test whether a large fraction of the mat...
The POINT-AGAPE CollaborationThe POINT-AGAPE collaboration is carrying out a search for gravitationa...
We present the first M 31 candidate microlensing events from the Microlensing Exploration of the Gal...
We present the first M 31 candidate microlensing events from the Microlensing Exploration of the Gal...
We have completed an intensive monitoring program of two fields on either side of the center of M31 ...
Gravitational Microlensing represents an effective tool in searching for non– luminous astrophysical...
We present results of a microlensing survey toward the Andromeda Galaxy (M31) carried out during fou...
We present the first results of the analysis of data collected during the 1998{99 observational camp...
The POINT-AGAPE CollaborationTo reveal the galactic dark matter in the form of MACHOs ("Massive Astr...
We present results of a microlensing survey toward the Andromeda Galaxy (M 31) carried out during fo...
We present results of a microlensing survey toward the Andromeda Galaxy (M31) carried out during fou...
We report the final analysis of a search for microlensing events in the direction of the Andromeda g...
We present results of a microlensing survey toward the Andromeda Galaxy (M 31) carried out during fo...
THERE is now abundant evidence for the presence of large quantities of unseen matter surrounding nor...
We detail how microlensing internal to M31 could be used to test whether a large fraction of the mat...
The POINT-AGAPE CollaborationThe POINT-AGAPE collaboration is carrying out a search for gravitationa...