In the same section :
Is AMBER observing the formation of a planet ?
Welcome to the new AMBER web site
First sky fringes (21 March 2004)
Outcome of the 3rd commissioning run
Fringes alignment complete (16 March 2004)
AMBER observes a quasar in medium resolution
Fuel for the black hole
A new Nova eruption followed by AMBER on the VLTI
Letter of the PI to the AMBER team (21 March 2004)
AMBER scrutinizes the environment of stars
AMBER second commissioning (15-26 Oct 2004)
23 October 2004, by
- AMBER team at Paranal for the 2nd commissioning on AT1 mirror.
- B. Koehler (ESO) is taking the picture through the first auxialiary telescope (AT1). From left to right: G. Zins, E. Le Coarer, F. Malbet, M. Vannier, L. Glück, G. Weigelt, G. Duvert.
The second commissioning run of the the AMBER instrument is currently taking place. It will last from 15 to 26 October 2004, with 4 days in lab, 5 nights on siderostats and finally 3 nights with UT2, UT3 and UT4. If everything goes well, it will be followed by three nights of Science Demonstration Time (27-28 Oct 2004).
The main goal of this run is to assess the performances of AMBER with the VLTI and to commission all spectral resolutions in H and K so that AMBER is rapidly offered to the astronomical community.
The AMBER team is composed of: G. Duvert (LAOG), L. Glück (LAOG), E. Le Coarer (LAOG), F. Malbet (LAOG), G. Weigelt (MPIfR) and G. Zins (LAOG). In Europe, R. Petrov (LUAN), F. Millour (LAOG/LUAN), D. Mourard (OCA), S. Lagarde (OCA) in Nice and D. Schertl (MPIfR), S. Kraus (MPIfR) in Bonn are in support especially for rapida data reduction.
On ESO side, the team is assisted by N. Housen, M. Kiekebush, F. Rantakyro, A. Richichi, M. Schoeller, M. Vannier, and, of course the VLT engineers and operators.