activity
19941998
most citedEROS and MACHO Combined Limits on Planetary Mass Dark Matter in the Galactic Halo

216 citations · 234 across the 6 of their papers we have counts for

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astro-ph1998★ 216 cited

EROS and MACHO Combined Limits on Planetary Mass Dark Matter in the Galactic Halo

EROS Collaboration, MACHO Collaboration

The EROS and MACHO collaborations have each published upper limits on the amount of planetary mass dark matter in the Galactic Halo obtained from gravitational microlensing searche…

astro-ph1996

Metallicity Effects on the Cepheid Extragalactic Distance Scale from EROS photometry in LMC and SMC

D. D. Sasselov, J. P. Beaulieu, C. Renault +30

This is an investigation of the period-luminosity relation of classical Cepheids in samples of different metallicity. It is based on 481 Cepheids in the Large and Small Magellanic…

astro-ph1996★ 3 cited

The effect of metallicity on the Cepheid distance scale and its implications for the Hubble constant () determination

J. P. Beaulieu, D. D. Sasselov, C. Renault +30

Recent HST determinations of the expansion's rate of the Universe (the Hubble constant, H_0) assumed that the Cepheid Period-Luminosity relation at V and I are independent of metal…

astro-ph1995★ 6 cited

EROS VARIABLE STARS : FUNDAMENTAL-MODE AND FIRST OVERTONE CEPHEIDS IN THE BAR OF THE LARGE MAGELLANIC CLOUD

J. P. Beaulieu, P. Grison, W. Tobin +27

We present CCD phase-binned light curves at 490 nm for 97 Cepheid variable stars in the bar of the LMC. The photometry was obtained as part of the French EROS project and has excel…

astro-ph1995★ 8 cited

SEARCH FOR VERY LOW MASS OBJECTS IN THE GALACTIC HALO

EROS collaboration, E. Aubourg, P. Bareyre +26

We present results from a search for gravitational microlensing of stars in the Large Magellanic Cloud by low mass objects in the Galactic Halo. The search uses the CCD light curve…

astro-ph1994★ 1 cited

Spectroscopic Studies of the Two Eros Candidate Microlensed Stars

J. P. Beaulieu, R. Ferlet, Ph. Grison +26

Low resolution spectroscopy, and UBVRI photometry, have been obtained for the two EROS microlensing candidates. Radial velocities indicate that both stars are members of the Large…