Optical design concept for the Giant Magellan Telescope Multi-object Astronomical and Cosmological Spectrograph (GMACS)

被引：0

作者：

Schmidt, Luke M. ^{[1
]}

Ribeiro, Rafael ^{[2
]}

Taylor, Keith ^{[3
]}

Jones, Damien ^{[4
]}

Prochaska, Travis ^{[1
]}

DePoy, Darren L. ^{[1
,6
]}

Marshall, Jennifer L. ^{[1
]}

Cook, Erika ^{[1
]}

Froning, Cynthia ^{[5
]}

Ji, Tae-Geun ^{[6
]}

Lee, Hye-In ^{[6
]}

de Oliveira, Claudia Mendes ^{[2
]}

Pak, Soojong ^{[6
]}

Papovich, Casey ^{[1
]}

机构：

[1] Texas A&M Univ, Dept Phys & Astron, 4242 TAMU, College Stn, TX 77843 USA

[2] Univ Sao Paulo, Dept Astron, IAG, BR-05508900 Sao Paulo, Brazil

[3] Instruments4, Woodland Hills, CA 91011 USA

[4] Prime Opt, Eumundi, Qld, Australia

[5] Univ Texas Austin, Dept Astron, C1400, Austin, TX 78712 USA

[6] Kyung Hee Univ, Sch Space Res, Yongin 17104, Gyeonggi Do, South Korea

来源：

GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY VI | 2016年 / 9908卷

关键词：

GMT; Extremely Large Telescopes; spectrograph; multi-object spectrograph; optical instruments; MOTION COMPENSATION SYSTEM;

D O I：

10.1117/12.2233543

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a preliminary conceptual optical design for GMACS, a wide field, multi-object, optical spectrograph currently being developed for the Giant Magellan Telescope (GMT). We include details of the optical design requirements derived from the instrument scientific and technical objectives and demonstrate how these requirements are met by the current design. Detector specifications, field acquisition/alignment optics, and optical considerations for the active flexure control system are also discussed.

引用

页数：19

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