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20042009
most citedOGLE 2004-BLG-254: a K3 III Galactic Bulge Giant spatially resolved by a single microlens

29 citations · 88 across the 5 of their papers we have counts for

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astro-ph20089 cited

Towards A Census of Earth-mass Exo-planets with Gravitational Microlensing

J. P. Beaulieu, E. Kerins, S. Mao +26

Thirteen exo-planets have been discovered using the gravitational microlensing technique (out of which 7 have been published). These planets already demonstrate that super-Earths (…

astro-ph200727 cited

Limits on additional planetary companions to OGLE-2005-BLG-390L

D. Kubas, A. Cassan, M. Dominik +1

We investigate constraints on additional planets orbiting the distant M-dwarf star OGLE-2005-BLG-390L, around which photometric microlensing data has revealed the existence of the…

astro-ph200629 cited

OGLE 2004-BLG-254: a K3 III Galactic Bulge Giant spatially resolved by a single microlens

A. Cassan, J. -P. Beaulieu, P. Fouque +37

We present an analysis of OGLE 2004-BLG-254, a high-magnification and relatively short duration microlensing event in which the source star, a Bulge K3-giant, has been spatially re…

astro-ph20058 cited

The red optical afterglow of GRB 030725

G. Pugliese, P. Møller, J. Gorosabel +6

We present a photometric study of the optical counterpart of the long-duration Gamma Ray Burst (GRB) 030725, which triggered the HETE FREGATE and WXM instruments on July 25th, 2003…

astro-ph2005

Full characterization of binary-lens event OGLE-2002-BLG-069 from PLANET observations

D. Kubas, A. Cassan, J. P. Beaulieu +25

We analyze the photometric data obtained by PLANET and OGLE on the caustic-crossing binary-lens microlensing event OGLE-2002-BLG-069. Thanks to the excellent photometric and spectr…

astro-ph2004

On the Afterglow of the X-Ray Flash of July 23 2003: Photometric evidence for an off-axis Gamma-Ray Burst with an associated Supernova?

J. P. U. Fynbo, J. Sollerman, J. Hjorth +31

We present optical and near-infrared follow-up observations of the X-Ray Flash (XRF) of July 23 2003. Our observations in the R-band cover the temporal range from 4.2 h to 64 days…