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Proceedings Paper

Status of the VLTI complementary characterization
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Paper Abstract

The first phase of the VLTI is now almost completed with 8 available telescopes, 2 science instruments and complementary facilities (in particular a fringe tracker and angle tracker). The next step will be the integration of PRIMA and the development of the second generation instruments for which a thorough understanding of the performance that can provided by the VLTI facility is required. This is the basic purpose of this ongoing complementary characterization. The rationale of this activity is recalled and the methods used as well as the results obtained so far presented.

Paper Details

Date Published: 28 July 2008
PDF: 11 pages
Proc. SPIE 7013, Optical and Infrared Interferometry, 70130J (28 July 2008); doi: 10.1117/12.790695
Show Author Affiliations
Philippe Gitton, European Southern Observatory (Chile)
Pierre Haguenauer, European Southern Observatory (Chile)


Published in SPIE Proceedings Vol. 7013:
Optical and Infrared Interferometry
Markus Schöller; William C. Danchi; Françoise Delplancke, Editor(s)

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