出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：We present results from the OGLE survey towards the Large Magellanic Cloud, which aimed to
detect the microlensing phenomena caused by compact objects in the Galactic Halo (MACHOs).
The analysed data covers nearly 10 years from 1997 to 2006 and includes the second and third
phase of the OGLE project. In total about 35 million objects were monitored over an area of 38
sq.deg. The small number of plausible microlensing candidates indicates that the Galactic Halo
towards the LMC is not made of dark matter in the form of MACHOs.
