S. Lagarde

The Mira variable S Orionis: relationships between the photosphere, molecular layer, dust shell, and SiO maser shellat 4 epochs

Accurate spectroscopic parameters of WASP planet host stars★

The Galactic Center: An Improved Astrometric Reference Frame for Stellar Orbits around the Supermassive Black Hole

First step to detect an extrasolar planet using simultaneous observations with the VLTI instruments AMBER and MIDI

Using the near infrared VLTI instrument AMBER