Adaptive optics on a 3.6-meter telescope - The ADONIS system

被引：31

作者：

Beuzit, JL

Demailly, L

Gendron, E

Gigan, P

Lacombe, F

Rouan, D

Hubin, N

Bonaccini, D

Prieto, E

Chazallet, F

Rabaud, D

Madec, PY

Rousset, G

Hofmann, R

Eisenhuer, F

机构：

[1] Observ Paris, DESPA, F-92195 Meudon, France

[2] ESO, D-85748 Garching, Germany

[3] SHAKTI SA, F-13001 Marseille, France

[4] Off Natl Etud & Rech Aerosp, F-92322 Chatillon, France

[5] MPIE, D-85748 Garching, Germany

来源：

EXPERIMENTAL ASTRONOMY | 1997年 / 7卷 / 04期

关键词：

D O I：

10.1023/A:1007924901154

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

ADONIS is an adaptive optics (AO) user friendly instrument offered to the European astronomical community on the ESO 3.6-m telescope at La Silla. It is an ugraded version of COME-ON-PLUS, the VLT AO prototype, which already produced significative astrophysical results in a wide range of fields, from planetology to extragalactic astrophysics. ADONIS is now allowing the astronomer to use adaptive optics as a common user instrument thanks to the implementation of an open artificial intelligence software that handles the large number of parameters needed to optimise the AO correction. We will describe the ADONIS system, including the two dedicated infrared cameras, summarize its performances and discuss the observing procedures.

引用

页码：285 / 292

页数：8

共 13 条

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