Share Email Print
cover

Proceedings Paper

Interferometric fringes with MACAO-VLTI corrected starlight and VINCI
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

We report on observations with MACAO-VLTI to feed the VLT Interferometer in November 2003. The purpose of this observing run was to optimize the feed to the VLTI by varying certain parameters of the curvature AO system and of the interferometer instrument VINCI. All along the main concern about this instrument combination was the differential piston introduced by 2 independent AO systems. A special so-called “piston removal algorithm” has been developed especially for this purpose. Each DM Influence Function is carefully characterized and a pure piston mode is defined to compensate piston over the pupil produced by a given voltage set. Piston is reduced by ~20 using this algorithm. It was found that decreasing the system main gain, while reducing strehl ratio, also reduces high frequency vibrations on the DM and therefore OPD variations. A control frequency of 420 Hz instead of the nominal 350 Hz was found to improve substantially the coupling by reducing the excitation of the DM resonance (~700Hz). On bright stars, an improvement of a factor of 30 in the flux injection into the VINCI fibers was measured. Following these tests a successful observation of the active nucleus of NGC 1068 was performed leading to a visibility of 40.4±5.4% on an average baseline of 45.84 m. The K magnitude in the 60 mas central source is 9.2±0.4. The results already put some interesting constraints on the inner torus and central engine of the nucleus of NGC 1068 but mostly show that the combination MACAO-VLTI and VINCI opens the realm of extragalactic astronomy to interferometry.

Paper Details

Date Published: 25 October 2004
PDF: 10 pages
Proc. SPIE 5490, Advancements in Adaptive Optics, (25 October 2004); doi: 10.1117/12.552574
Show Author Affiliations
Robin Arsenault, European Southern Observatory (Germany)
Pierre Kervella, LESIA, CNRS, and Observatoire de Paris (France)
Rob Donaldson, European Southern Observatory (Germany)
Markus Erdmann Kasper, European Southern Observatory (Germany)
Enrico Fedrigo, European Southern Observatory (Germany)
Anders Wallander, European Southern Observatory (Germany)
Markus Schoeller, European Southern Observatory (Germany)
Nico Housen, European Southern Observatory (Germany)
Francoise Delplancke, European Southern Observatory (Germany)
Fernando Salgado, European Southern Observatory (Germany)
Christophe Dupuy, European Southern Observatory (Germany)
Norbert N. Hubin, European Southern Observatory (Germany)
Liviu Ivanescu, European Southern Observatory (Germany)
Sylvain Oberti, European Southern Observatory (Germany)
Jerome Paufique, European Southern Observatory (Germany)
Silvio Rossi, European Southern Observatory (Germany)
Markus Wittkowski, European Southern Observatory (Germany)


Published in SPIE Proceedings Vol. 5490:
Advancements in Adaptive Optics
Domenico Bonaccini Calia; Brent L. Ellerbroek; Roberto Ragazzoni, Editor(s)

© SPIE. Terms of Use
Back to Top