The VLTI -: A status report

被引：37

作者：

Glindemann, A ^{[1
]}

Algomedo, J ^{[1
]}

Amestica, R ^{[1
]}

Ballester, P ^{[1
]}

Bauvir, B ^{[1
]}

Bugueño, E ^{[1
]}

Correia, S ^{[1
]}

Delgado, F ^{[1
]}

Delplancke, F ^{[1
]}

Derie, F ^{[1
]}

Duhoux, P ^{[1
]}

di Folco, E ^{[1
]}

Gennai, A ^{[1
]}

Gilli, B ^{[1
]}

Giordano, P ^{[1
]}

Gitton, P ^{[1
]}

Guisard, S ^{[1
]}

Housen, N ^{[1
]}

Huxley, A ^{[1
]}

Kervella, P ^{[1
]}

Kiekebusch, M ^{[1
]}

Koehler, B ^{[1
]}

Lévêque, S ^{[1
]}

Longinotti, A ^{[1
]}

Ménardi, S ^{[1
]}

Morel, S ^{[1
]}

Paresce, F ^{[1
]}

Duc, TP ^{[1
]}

Richichi, A ^{[1
]}

Schöller, M ^{[1
]}

Tarenghi, M ^{[1
]}

Wallander, A ^{[1
]}

Wittkowski, M ^{[1
]}

Wilhelm, R ^{[1
]}

机构：

[1] European So Observ, D-85748 Garching, Germany

来源：

INTERFEROMETRY FOR OPTICAL ASTRONOMY II, PTS 1 AND 2 | 2003年 / 4838卷

关键词：

interferometry; Very Large Telescopes; interferometric instrumentation; very high angular resolution; adaptive optics; astrometry; phase referenced imaging; VLTI;

D O I：

10.1117/12.458117

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Very Large Telescope (VLT) Observatory on Cerro Paranal (2635 m) in Northern Chile is approaching completion. After the four 8-m Unit Telescopes (UT) individually saw first light in the last years, two of them were combined for the first time on October 30, 2001 to form a stellar interferometer, the VLT Interferometer. The remaining two UTs will be integrated into the interferometric array later this year. In this article, we will describe the subsystems of the VLTI and the planning for the following years.

引用

页码：89 / 100

页数：12

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