activity
19942004
most citedEROS and MACHO Combined Limits on Planetary Mass Dark Matter in the Galactic Halo

216 citations · 309 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2004★ 76 cited

Type Ia supernova rate at a redshift of ~ 0.1

G. Blanc, C. Afonso, C. Alard +58

We present the type Ia rate measurement based on two EROS supernova search campaigns (in 1999 and 2000). Sixteen supernovae identified as type Ia were discovered. The measurement o…

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★ 2 cited

Observational Limits on Machos in the Galactic Halo

EROS collaboration, C. Renault, C. Afonso +40

We present final results from the first phase of the EROS search for gravitational microlensing of stars in the Magellanic Clouds by unseen deflectors (machos: MAssive Compact Halo…

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…