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CONFIRMATION OF THE OGLE-2005-BLG-169 PLANET SIGNATURE AND ITS CHARACTERISTICS WITH
LENS–SOURCE PROPER MOTION DETECTION
V....
Hband. This is the first time that a proper motion determined
from the planetary signal of a microlensing light curve is
c...
3. GOING FROM STAR/PLANET MASS RATIOS TO
PHYSICAL MASSES
As explained in Batista et al. (2014), for most microlensing
even...
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