We discuss pixel lensing observations towards M31 carried out at the Loiano telescope. We have established a fully automatic pipeline for the detection and the characterization of microlensing events. We have evaluated the efficiency of the pipeline. We have estimated the expected signal by means of a Monte Carlo simulation. As a result we select 2 microlensing candidates. This is compatible with the expected M31 self-lensing signal. The small statistics of events at disposal does not still allow us, however, to draw definite conclusions on the content of compact halo objects
Pixel lensing is gravitational microlensing of unresolved stars. The main target explored up to now ...
A.G. was supported by NSF grant AST-1103471. M.D. is thankful to Qatar National Research Fund (QNRF)...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...
Microlensing observations towards M31 are a powerful tool for the study of the dark matter populatio...
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...
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...
Microlensing observations toward M31 are a powerful tool for the study of the dark matter population...
We analyse a series of pilot observations in order to study microlensing of (unresolved) stars in M3...
none17siWe present the final analysis of the observational campaign carried out by the PLAN (Pixel L...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...
We discuss the results of the MEGA microlensing campaign towards M31. Our analysis is based on an an...
Pixel lensing is gravitational microlensing of unresolved stars. The main target explored up to now ...
A.G. was supported by NSF grant AST-1103471. M.D. is thankful to Qatar National Research Fund (QNRF)...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...
Microlensing observations towards M31 are a powerful tool for the study of the dark matter populatio...
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...
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...
Microlensing observations toward M31 are a powerful tool for the study of the dark matter population...
We analyse a series of pilot observations in order to study microlensing of (unresolved) stars in M3...
none17siWe present the final analysis of the observational campaign carried out by the PLAN (Pixel L...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...
We discuss the results of the MEGA microlensing campaign towards M31. Our analysis is based on an an...
Pixel lensing is gravitational microlensing of unresolved stars. The main target explored up to now ...
A.G. was supported by NSF grant AST-1103471. M.D. is thankful to Qatar National Research Fund (QNRF)...
We present the final analysis of the observational campaign carried out by the PLAN (Pixel Lensing A...