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

页码：41 / 45

页数：5

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