AMBER: The VLTI near-infrared instrument optical design and expected performance

被引：0

作者：

Robbe-Dubois, S ^{[1
]}

Antonelli, P ^{[1
]}

Beckmann, U ^{[1
]}

Bresson, Y ^{[1
]}

Gennari, S ^{[1
]}

Lagarde, S ^{[1
]}

Lisi, F ^{[1
]}

Malbet, F ^{[1
]}

Martinot-Lagarde, G ^{[1
]}

Rabbia, Y ^{[1
]}

Rebattu, S ^{[1
]}

Rousselet-Perraut, K ^{[1
]}

Petrov, R ^{[1
]}

机构：

[1] Univ Nice, UMR 6525, F-06108 Nice 2, France

来源：

DARWIN AND ASTRONOMY, PROCEEDINGS: THE INFRARED SPACE INTERFEROMETER | 2000年 / 451卷

关键词：

VLTI; interferometry; spectroscopy; instrument;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

AMBER, Astronomical Multi BEam combineR, is the near-infrared instrument dedicated to the VLTI. It is presently designed to work with three of either the 8 m or the 1.8 m telescopes fi om I to 2.5 mu m. Given the expected scientific performance and requirements for AMBER, we derived the functional analysis leading to the present optical configuration using optical fibers to spatially filler the wavefront perturbations, and dispersed fringes. The expected performance is presented in terms of optical quality and sensitivity to misalignments.

引用

页码：215 / 220

页数：4

共 50 条

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