MIRC-X/CHARA: sensitivity improvements with an ultra-low noise SAPHIRA detector

被引：8

作者：

Anugu, Narsireddy ^{[1
]}

Le Bouquin, Jean-Baptiste ^{[2
,3
]}

Monnier, John D. ^{[2
]}

Kraus, Stefan ^{[1
]}

Ennis, Jacob ^{[2
]}

Lanthermann, Cyprien ^{[3
]}

Setterholm, Bebjamin R. ^{[2
]}

Davies, Claire L. ^{[1
]}

ten Brummelaar, Theo ^{[4
]}

Haidar, Mariam ^{[2
]}

Dubravec, Veronika ^{[2
]}

Peters, Scott ^{[2
]}

机构：

[1] Univ Exeter, Sch Phys & Astron, Exeter EX4 4QL, Devon, England

[2] Univ Michigan, Ann Arbor, MI 48109 USA

[3] Inst Planetol & Astrophys Grenoble, F-38058 Grenoble, France

[4] Georgia State Univ, CHARA Array, Atlanta, GA 30302 USA

来源：

OPTICAL AND INFRARED INTERFEROMETRY AND IMAGING VI | 2018年 / 10701卷

基金：

欧洲研究理事会;

关键词：

infrared; interferometry; imaging; SAPHIRA; C-RED ONE;

D O I：

10.1117/12.2313036

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

MIRC-X is an upgrade of the six-telescope infrared beam combiner at the CHARA telescope array, the world's largest baseline interferometer in the optical/infrared, located at the Mount Wilson Observatory in Los Angeles. The upgraded instrument features an ultra-low noise and fast frame rate infrared camera (SAPHIRA detector) based on e-APD technology. We report the MIRC-X sensitivity upgrade work and first light results in detail focusing on the detector characteristics and software architecture.

引用

页数：16

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