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19962009
most citedDiscovery of a Jupiter/Saturn Analog with Gravitational Microlensing

366 citations · 552 across the 9 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-ph2008366 cited

Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing

B. S. Gaudi, D. P. Bennett, A. Udalski +66

Searches for extrasolar planets have uncovered an astonishing diversity of planetary systems, yet the frequency of solar system analogs remains unknown. The gravitational microlens…

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-ph200675 cited

The spectral energy distribution of PKS 2004-447: a compact steep-spectrum source and possible radio-loud narrow-line Seyfert 1 galaxy

L. C. Gallo, P. G. Edwards, E. Ferrero +10

(abridged) The spectral energy distribution (SED) of the compact steep spectrum (CSS) source and possible radio-loud narrow-line Seyfert 1 galaxy (NLS1), PKS2004-447, is presented.…

astro-ph200616 cited

A transient I band excess in the optical spectrum of the accreting millisecond pulsar SAX J1808.4-3658

J. G. Greenhill, A. B. Giles, C. Coutures

The optical counterpart of the transient, millisecond X-ray pulsar SAX J1808.4-3658 was observed in four colours (BVRI) for five weeks during the 2005 June-July outburst. The optic…