papers

Publications (7)

astro-ph2000

Type Ia supernova rate at

D. Hardin, C. Afonso, C. Alard +44

We present the EROS nearby supernova () search and the analysis of the first year of data (1997). A total of 80 square degrees were surveyed. Eight supernovæ we…

astro-ph2008

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-ph2004

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-ph.SR2009

The beat Cepheids in the Magellanic Clouds: an analysis from the EROS-2 database

J. B. Marquette, J. P. Beaulieu, J. R. Buchler +36

A number of microlensing dark-matter surveys have produced tens of millions of light curves of individual background stars. These data provide an unprecedented opportunity for syst…

astro-ph2007

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-ph.GA2009

The EROS2 search for microlensing events towards the spiral arms: the complete seven season results

Y. R. Rahal, C. Afonso, J. -N. Albert +36

The EROS-2 project has been designed to search for microlensing events towards any dense stellar field. The densest parts of the Galactic spiral arms have been monitored to maximiz…

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…