activity
19982003
most citedFirst microlens mass measurement: PLANET photometry of EROS BLG-2000-5

180 citations · 1.1k across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph2003★ 87 cited

High-Precicison Limb-Darkening Measurement of a K3 Giant Using Microlensing

Dale L. Fields, M. D. Albrow, J. An +21

We obtain high-precision limb-darkening measurements in five bands (V, V_E, I_E, I, and H) for the K3 III (Teff=4200 K, [Fe/H]=+0.3, log(g)=2.3) source of the Galactic bulge microl…

astro-ph2002★ 32 cited

A Short, Non-Planetary, Microlensing Anomaly: Observations and Lightcurve Analysis of MACHO 99-BLG-47

M. D. Albrow, J. An, J. -P. Beaulieu +17

We analyze PLANET and MACHO observations of MACHO 99-BLG-47, the first nearly-normal microlensing event for which high signal-to-noise-ratio data reveal a well-covered, short-durat…

astro-ph2001★ 180 cited

First microlens mass measurement: PLANET photometry of EROS BLG-2000-5

Jin H. An, M. D. Albrow, J. -P. Beaulieu +17

We analyze PLANET photometric observations of the caustic-crossing binary-lens microlensing event, EROS BLG-2000-5, and find that modeling the observed light curve requires incorpo…

astro-ph2001★ 131 cited

Microlensing Constraints on the Frequency of Jupiter-Mass Companions: Analysis of Five Years of PLANET Photometry

B. S. Gaudi, M. D. Albrow, J. An +21

We analyze five years of PLANET photometry of microlensing events toward the Galactic bulge to search for the short-duration deviations from single lens light curves that are indic…

astro-ph2000★ 31 cited

H-alpha Equivalent Width Variations across the Face of a Microlensed K Giant in the Galactic Bulge

M. Albrow, J. An, J. -P. Beaulieu +14

We present VLT FORS1 spectroscopy that temporally resolves the second caustic crossing of the Bulge K giant source of microlensing event EROS 2000-BLG-5, the first time this has be…

astro-ph2000★ 65 cited

Limits on the Abundance of Galactic Planets From Five Years of Planet Observations

M. D. Albrow, J. An, J. -P. Beaulieu +21

We search for signatures of planets in 43 intensively monitored microlensing events that were observed between 1995 and 1999. Planets would be expected to cause a short duration (~…