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19942009
most citedLimits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds

940 citations · 1k across the 7 of their papers we have counts for

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astro-ph20081 cited

Discovery of a peculiar Cepheid-like star towards the northern edge of the Small Magellanic Cloud

J. B. Marquette, P. Tisserand, P. Francois +37

For seven years, the EROS-2 project obtained a mass of photometric data on variable stars. We present a peculiar Cepheid-like star, in the direction of the Small Magellanic Cloud,…

astro-ph200837 cited

R Coronae Borealis stars in the Galactic Bulge discovered by EROS-2

P. Tisserand, J. B. Marquette, P. R. Wood +33

Rare types of variable star may give unique insight into short-lived stages of stellar evolution. The systematic monitoring of millions of stars and advanced light curve analysis t…

astro-ph2006940 cited

Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds

P. Tisserand, L. Le Guillou, C. Afonso +35

The EROS-2 project was designed to test the hypothesis that massive compact halo objects (the so-called ``machos'') could be a major component of the dark matter halo of the Milky…

astro-ph200610 cited

Removing the Microlensing Blending-Parallax Degeneracy Using Source Variability

R. J. Assef, A. Gould, the EROS-2 +2

Microlensing event MACHO 97-SMC-1 is one of the rare microlensing events for which the source is a variable star, simply because most variable stars are systematically eliminated f…

astro-ph20062 cited

The OGLE-II event sc5_2859 : a Classical Nova outburst?

C. Afonso, J. F. Glicenstein, A. Gould +3

The OGLE-II event sc5_2859 was previously identified as the third longest microlensing event ever observed. Additional photometric observations from the EROS (Experience de Recherc…

astro-ph2006

Galactic Bulge Microlensing Optical Depth from EROS-2

C. Hamadache, L. Le Guillou, P. Tisserand +34

We present a new EROS-2 measurement of the microlensing optical depth toward the Galactic Bulge. Light curves of clump-giant stars distributed over of t…