FIES: The high-resolution Fiber-fed Echelle Spectrograph at the Nordic Optical Telescope

被引：192
|
作者：
Telting, J. H. [1 ]
Avila, G. [2 ]
Buchhave, L. [3 ]
Frandsen, S. [4 ]
Gandolfi, D. [5 ]
Lindberg, B. [6 ]
Stempels, H. C. [7 ]
Prins, S. [8 ]
机构：
[1] Nord Opt Telescope, Roque Los Muchachos Observ, La Palma 38711, Canarias, Spain
[2] European So Observ, Photon & Opt Grp, Garching, Germany
[3] Univ Copenhagen, Niels Bohr Inst, DK-1168 Copenhagen, Denmark
[4] Univ Aarhus, Dept Phys & Astron, DK-8000 Aarhus C, Denmark
[5] ESTEC ESA, Res & Sci Support Dept, Noordwijk, Netherlands
[6] LensTech AB, Skelleftea, Sweden
[7] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden
[8] KULeuven, Inst Sterrenkunde, Louvain, Belgium
来源：
ASTRONOMISCHE NACHRICHTEN | 2014年 / 335卷 / 01期
关键词：
instrumentation: spectrographs; techniques: radial velocities; techniques: spectroscopic; EXOPLANETS; STARS;
D O I：
10.1002/asna.201312007
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
FIES is a cross-dispersed high-resolution echelle spectrograph at the 2.56 m Nordic Optical Telescope (NOT), and was optimised for throughput and stability in 2006. The major 2006 upgrade involved the relocation of FIES to a stable environment and development of a fiber bundle that offers 3 different resolution modes, and made FIES an attractive tool for the user community of the NOT. Radial-velocity stability is achieved through double-chamber active temperature control. A dedicated data reduction tool, FIEStool, was developed. As a result of these upgrades, FIES is now one of the work-horse instruments at the NOT. ((c) 2014 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)
引用
收藏
页码：41 / 45
页数：5
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