Galactic Bulge microlensing optical depth from EROS-2
Aims. We present a new EROS-2 measurement of the microlensing optical depth toward the Galactic Bulge. Methods. Light curves of 5.6 × 106 clump-giant stars distributed over 66 deg2 of the Bulge were monitored during seven Bulge seasons. 120 events were f
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
|01_Hamadache_Galactic_Bulge_microlensing_2006.pdf||1.7 MB||Adobe PDF||Request a copy|
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