SUBARU prime focus spectrograph integration and performance at LAM

被引:2
|
作者
Madec, F. [1 ]
Pascal, S. [1 ]
Le Fur, A. [1 ]
Le Mignant, D. [1 ]
Dohlen, K. [1 ]
Barrette, R. [1 ]
Belhadi, M. [1 ]
Smee, S. [2 ]
Gunn, J. [4 ]
Le Merrer, J. [1 ]
Llored, M. [1 ]
Jaquet, M. [1 ]
Balard, P. [1 ]
Blanchard, P. [1 ]
Roman, F. [1 ]
Lapere, V. [6 ]
Gabriel, J. F. [6 ]
Loomis, C. [4 ]
Golebiowski, M. [2 ]
Hart, M. [2 ]
Oliveira, L. [5 ]
Oliveira, A. [5 ]
Ferreira, D. [5 ]
Tamura, N. [3 ]
Shimono, A. [3 ]
机构
[1] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France
[2] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[3] Univ Tokyo, Kalvi Inst Phys & Math Universe WPI, Tokyo, Japan
[4] Princeton Univ, Princeton, NJ 08544 USA
[5] MCT, LNA, Itajuba, MG, Brazil
[6] Winlight Syst, Pertuis, France
关键词
SUBARU; PFS; SuMIRe; integration; test; fibers spectrograph;
D O I
10.1117/12.2313610
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Prime Focus Spectrograph (PFS) of the Subaru Measurement of Images and Redshifts (SuMIRe) project for Subaru telescope includes four identical spectrograph modules fed by 600 fibers each. This paper presents the integration, alignment and test procedures for the first spectrograph module composed by an optical entrance unit that creates a collimated beam and distributes the light to three channels, two visible and one near infrared. In particular, we present the performance of the single Red channel module. Firstly, we report on the measured optical performance: optical quality and ghost analysis. We also report on the thermal performance of the visible camera cryostat. Finally, we describe the software used to control and monitor the instrument.
引用
收藏
页数:17
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