Standard Candles and Distances

Unraveling the physics of stars and the cosmos using pulsations

My research uses pulsating stars as tools for understanding the physics of stars, the structure of nearby galaxies, and for measuring how fast the Universe is expanding.


Contacts

Head of Laboratory
Dr. Richard Anderson
Office: 447 at SAUV 01
Tel: +41 (0)22 379 2425
E-mail: [email protected]
Secretary
Office: SAUV 01
Tel: +41 (0)22 379 4009
E-mail: [email protected]
Mailing Address
EPFL SB IPHYS GR-ANDERSON
Observatoire de Sauverny
Chemin Pegasi 51
CH-1290 Versoix
Switzerland