15 text pages + 2 tables + 7 figures. Accepted for publication in ApJ - By EROS-2 Collaboration and MACHO Collaboration and OGLE CollaborationMicrolensing event MACHO 97-SMC-1 is one of the rare microlensing events for which the source is a variable star, simply because most variable stars are systematically eliminated from microlensing studies. Using observational data for this event, we show that the intrinsic variability of a microlensed star is a powerful tool to constrain the nature of the lens by breaking the degeneracy between the microlens parallax and the blended light. We also present a statistical test for discriminating the location of the lens based on the \chi^2 contours of the vector \Lambda, the inverse of the projected velo...
We present photometric and spectroscopic data for the second microlensing event seen toward the Smal...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...
Various models for the Galactic distribution of massive compact halo objects (MACHOs) have been prop...
Microlensing event MACHO 97-SMC-1 is one of the rare microlensing events for which the source is a v...
Microlensing event MACHO 97-SMC-1 is one of the rare microlensing events for which the source is a v...
We present photometric observations of the MACHO-SMC-1 microlensing candidate collected by the OGLE-...
We present photometric observations and analysis of the second microlensing event detected toward th...
Blended light is an important source of degeneracy in the characterization of microlensing events, p...
We present a new analysis of the results of the Expérience pour la Recherche d'Objets Sombres (EROS)...
We analyse a series of pilot observations in order to study microlensing of (unresolved) stars in M3...
Microlensing observations toward M31 are a powerful tool for the study of the dark matter population...
I present a new analysis of the MACHO Project 5.7 year Large Magellanic Cloud (LMC) microlensing dat...
Microlensing observations toward M31 are a powerful tool for the study of the dark matter population...
Microlensing observations toward M31 are a powerful tool for the study of the dark matter population...
We present observations of the binary lensing event MACHO 98-SMC-1 conducted at the Mount Stromlo 1....
We present photometric and spectroscopic data for the second microlensing event seen toward the Smal...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...
Various models for the Galactic distribution of massive compact halo objects (MACHOs) have been prop...
Microlensing event MACHO 97-SMC-1 is one of the rare microlensing events for which the source is a v...
Microlensing event MACHO 97-SMC-1 is one of the rare microlensing events for which the source is a v...
We present photometric observations of the MACHO-SMC-1 microlensing candidate collected by the OGLE-...
We present photometric observations and analysis of the second microlensing event detected toward th...
Blended light is an important source of degeneracy in the characterization of microlensing events, p...
We present a new analysis of the results of the Expérience pour la Recherche d'Objets Sombres (EROS)...
We analyse a series of pilot observations in order to study microlensing of (unresolved) stars in M3...
Microlensing observations toward M31 are a powerful tool for the study of the dark matter population...
I present a new analysis of the MACHO Project 5.7 year Large Magellanic Cloud (LMC) microlensing dat...
Microlensing observations toward M31 are a powerful tool for the study of the dark matter population...
Microlensing observations toward M31 are a powerful tool for the study of the dark matter population...
We present observations of the binary lensing event MACHO 98-SMC-1 conducted at the Mount Stromlo 1....
We present photometric and spectroscopic data for the second microlensing event seen toward the Smal...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...
Various models for the Galactic distribution of massive compact halo objects (MACHOs) have been prop...