Thierry Fusco Gérard Rousset NAOS-CONICA (a.k.a NACO) for the VLT.
POLARIMETRIC OBSERVATIONS OF TNOs AND CENTAURS AT THE ESO-VLT Institute of Astronomy, Kharkiv National University, Ukraine Irina Belskaya In collaboration.
Masters Course: Experimental Techniques Wavelength – Frequency Measurements Frequency: - unit to be measured most accurately in physics - frequency counters.
ESO-ESA Existing Activities Archives, Virtual Observatories and the Grid.
SPIE 2002 Aug. 22-28, 2002 ACS CORBA-based Common Software for the ALMA project - 4848-05 G. Chiozzi, B. Gustafsson, B. Jeram – ESO M. Plesko, M. Sekoranja,
March 26, 2014 In your journal, title it “Name that Galaxy” # 1-8. Get with your partner (s) from yesterday and decide if the picture represents: Spiral.
11/30/06Astrophysics enabled by the Return to the Moon Astrophysics Enabled by a Permanent Lunar Facility Massimo Stiavelli Space Telescope Science Institute.
High Precision Spectroscopy 2006 - LP CODEX …Opening a new parameter Space…
CORBA Controls Workshop, Grenoble 9-11 October, 2002 ACS CORBA-based Common Software for ALMA and other projects G.Chiozzi*, B.Gustafsson*, B.Jeram*, P.Sivera*
Tuesday. Parent Function Quiz 4 Graphs No Calculators/No Notes Use entire 10x10 grid Don’t forget to graph asymptotes if needed! About 8-10 minutes to.
Observational techniques meeting #2. Good use for diffraction: exoplanets.
Widening the Scope of Adaptive Optics Matthew Britton.