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| Creator | Title | Description | Subject | Date | ||
|---|---|---|---|---|---|---|
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Gondolo, Paolo | AGAPE: a search for dark matter in M31 by microlensing effects on unresolved stars | M 31 is a very tempting target for a microlensing search of compact objects in galactic haloes. It is the nearest large galaxy, it probably has its own dark halo, and its tilted position with respect to the line of sight provides an unmistakable signature of microlensing. However most stars of M 31... | M31; AGAPE; Pixel method; Galaxy; Halo; Cosmology; Gravitational lensing | 1997 |
| 2 |
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Gondolo, Paolo | AGAPEROS: searching for microlensing in the LMC with the pixel method. I. Data treatment and pixel light curves production | Recent surveys monitoring millions of light curves of resolved stars in the LMC have discovered several microlensing events. Unresolved stars could however signi _x000C_cantly contribute to the microlensing rate towards the LMC. Monitoring pixels, as opposed to individual stars, should be able to ... | Data analysis techniques; Halo; Galaxies; Gravitational lensing; Pixel method; Large Magellanic Cloud; LMC | 1999 |
| 3 |
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Gondolo, Paolo | AgapeZ1: a large amplification microlensing event or an odd variable star towards the inner bulge of M31 | AgapeZ1 is the brightest and the shortest duration microlensing candidate event found to date in the Agape experiment. It occurred only 4200 from the centre of M31 at RA = 0h42m41:47s and Dec = 41°16'39.1" (J2000). Our photometry shows that the half intensity duration of the event is 5.3 days and ... | AgapeZ1; Galaxy; Halo; Cosmology; Gravitational lensing; M31; Pixel method | 1999 |
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