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20032026
most citedLimits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds

940 citations · 1.9k across the 32 of their papers we have counts for

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astro-ph2008★ 1 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-ph2008★ 37 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-ph2007

INTEGRAL Observations of the Vela Region Focusing on Vela X-1

Stephane Schanne, Diego Gotz, Lucie Gerard +5

The Vela region has been observed for 1.7 Ms in November 2005 by the INTEGRAL satellite. We present preliminary spectral and temporal results of Vela X-1, an eclipsing neutron star…

astro-ph2007★ 3 cited

Evidence for 1809 keV Gamma-Ray Emission from 26Al Decays in the Vela Region with INTEGRAL/SPI

Stephane Schanne, Patrick Sizun, David Maurin +3

The Vela region is a promising target for the detection of 1.8 MeV gamma-rays emitted by the decays of radioactive 26Al isotopes produced in hydrostatic or explosive stellar nucleo…

astro-ph2006★ 940 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-ph2006★ 10 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…