Operation of the Adaptive Optics System at the Large Binocular Telescope Observatory

被引：2

作者：

Miller, Douglas L. ^{[1
]}

Guerra, Juan Carlos ^{[1
]}

Boutsia, Konstantina ^{[1
,2
]}

Fini, Luca ^{[3
]}

Argomedo, Javier ^{[3
]}

Biddick, Chris ^{[1
]}

Agapito, Guido ^{[3
]}

Arcidiacon, Carmelo ^{[3
]}

Briguglio, Runa ^{[3
]}

Brusa, Guido ^{[1
]}

Busoni, Lorenzo ^{[3
]}

Esposito, Simone ^{[3
]}

Hill, John ^{[1
]}

Kulesa, Craig ^{[4
]}

McCarthy, Don ^{[4
]}

Pinna, Enrico ^{[3
]}

Puglisi, Alfio Timothy ^{[3
]}

Quiros-Pacheco, Fernando ^{[3
]}

Riccardi, Armando ^{[3
]}

Xompero, Marco ^{[3
]}

机构：

[1] Large Binocular Telescope Observ, Tucson, AZ 85719 USA

[2] INAF, Rome, Italy

[3] INAF Arcetri, Rome, Italy

[4] Steward Observ, Tucson, AZ 85719 USA

来源：

ADAPTIVE OPTICS SYSTEMS III | 2012年 / 8447卷

关键词：

D O I：

10.1117/12.930803

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

The Adaptive Optics System at the Large Binocular Telescope Observatory consists of two Adaptive Secondary (ASM) mirrors and two Pyramid Wavefront sensors. The first ASM/Pyramid pair has been commissioned and is being used for science operation using the NIR camera PISCES on the right side of the binocular telescope. The left side ASM/Pyramid system is currently being commissioned, with completion scheduled for the Fall of 2012. We will discuss the operation of the first Adaptive Optics System at the LBT Observatory including interactions of the AO system with the telescope and its TCS, observational modes, user interfaces, observational scripting language, time requirement for closed loop and offsets and observing efficiency.

引用

页数：5

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