Commissioning of the Infrared Imaging Survey (IRIS) System

被引：14

作者：

Hodapp, Klaus W. ^{[1
]}

Chini, Rolf

Reipurth, Bo ^{[1
,2
]}

Murphy, Miguel ^{[3
]}

Lemke, Roland ^{[2
]}

Watermann, Ramon ^{[2
]}

Jacobson, Shane ^{[1
]}

Bischoff, Karsten

Chonis, Taylor ^{[1
]}

Dement, Kaniela ^{[1
]}

Terrien, Ryan ^{[1
]}

Bott, Kimberley ^{[1
]}

Provence, Sydney ^{[1
]}

机构：

[1] Univ Hawaii, Inst Astron IfA, 640 N Aohoku Pl, Hilo, HI 96720 USA

[2] Ruhr Univ Bochum, Inst Astron, D-44801 Bochum, Germany

[3] Univ Catolica Norte, Antofagasta, Chile

来源：

GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY III | 2010年 / 7735卷

基金：

美国国家科学基金会;

关键词：

Survey Telescope; Optical Design; NEBULA;

D O I：

10.1117/12.856288

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Infrared Imaging System (IRIS) is a 0.8m telescope and a 1024x1024 pixels camera (IRISCAM) with a HAWAII-1 detector array. IRIS is located at the Cerro Armazones Observatory in Chile that is operated by the Ruhr University Bochum jointly with the Universidad Catolica del Norte in Antofagasta. It will be used primarily to survey star-forming regions for variability. Our goal is to discover young stellar objects undergoing accretion instabilities or rotational modulation of star spots, eclipsing binaries, and variable reflection nebulae. The telescope and the infrared camera are completed and first light was achieved in May of 2010. IRIS is currently being tested and characterized, before the long-term monitoring project will commence.

引用

页数：10

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