Using the near infrared VLTI instrument AMBER

被引：39

作者：

Petrov, RG ^{[1
]}

Malbet, F ^{[1
]}

Weigelt, G ^{[1
]}

Lisi, F ^{[1
]}

Puget, P ^{[1
]}

Antonelli, P ^{[1
]}

Beckmann, U ^{[1
]}

Lagarde, S ^{[1
]}

Lecoarer, E ^{[1
]}

Robbe-Dubois, S ^{[1
]}

Duvert, G ^{[1
]}

Gennari, S ^{[1
]}

Chelli, A ^{[1
]}

Dugué, M ^{[1
]}

Rousselet-Perraut, K ^{[1
]}

Vannier, M ^{[1
]}

Mourard, D ^{[1
]}

机构：

[1] Univ Nice Sophia Antipolis, F-06108 Nice, France

来源：

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

关键词：

astronomy; optical interferometry; instrumentation; high angular resolution; Very Large Telescope; differential interferometry; extra solar planets;

D O I：

10.1117/12.459113

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

AMBER is the General User near infrared focal instrument of the Very Large Telescope Interferometer. Its a single mode, dispersed fringes, three telescopes instrument. A limiting magnitude of the order of H=13 will allow to tackle a fair sample of extra galactic targets. A very high accuracy, in particular in color differential phase and closure phase modes gives good hope for very high dynamic range observation, possibly including hot extra solar planets. The relatively high maximum spectral resolution, up to 10000, will allow some stellar activity observations. Between this extreme goals, AMBER should have a wide range of applications including Young Stellar Objects, Evolved Stars, circumstellar material and many others. This papers tries to introduce AMBER to its future users with information on what it measures, how it is calibrated and hopes to give the readers ideas for applications.

引用

页码：924 / 933

页数：10

共 50 条

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