Author:
Blanc G.,Afonso C.,Alard C.,Albert J. N.,Aldering G.,Amadon A.,Andersen J.,Ansari R.,Aubourg É.,Balland C.,Bareyre P.,Beaulieu J. P.,Charlot X.,Conley A.,Coutures C.,Dahlén T.,Derue F.,Fan X.,Ferlet R.,Folatelli G.,Fouqué P.,Garavini G.,Glicenstein J. F.,Goldman B.,Goobar A.,Gould A.,Graff D.,Gros M.,Haissinski J.,Hamadache C.,Hardin D.,Hook I. M.,de Kat J.,Kent S.,Kim A.,Lasserre T.,Le Guillou L.,Lesquoy É.,Loup C.,Magneville C.,Marquette J. B.,Maurice É.,Maury A.,Milsztajn A.,Moniez M.,Mouchet M.,Newberg H.,Nobili S.,Palanque-Delabrouille N.,Perdereau O.,Prévot L.,Rahal Y. R.,Regnault N.,Rich J.,Ruiz-Lapuente P.,Spiro M.,Tisserand P.,Vidal-Madjar A.,Vigroux L.,Walton N. A.,Zylberajch S.
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference46 articles.
1. Bulge microlensing optical depth from EROS 2
observations $^{\bullet}$
2. Limits on Galactic dark matter with 5 years of EROS SMC data
3. Overview of the Nearby Supernova Factory
4. Bauer, F., & de Kat, J. 1997, in Optical Detectors for Astronomy, held at ESO, Garching, October 8-10, 1996, ed. J. W. Beletic, & P. Amico (The EROS collaboration)
5. SExtractor: Software for source extraction