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FIES: The high‐resolution Fiber‐fed Echelle Spectrograph at the Nordic Optical Telescope
233
Citations
11
References
2014
Year
PhotometryEngineeringAbstract FiesNatural SciencesSpectroscopyActive OpticsNordic Optical TelescopeCross‐dispersed High‐resolutionSpace OpticAstronomical Image AnalysisFiber OpticsOptical SystemsInstrumentationFiber BundleRadio TelescopeAstrophysics
FIES is a cross‑dispersed high‑resolution echelle spectrograph at the 2.56 m Nordic Optical Telescope, optimised for throughput and stability since 2006. The 2006 upgrade moved FIES to a stable environment, introduced a fiber bundle providing three resolution modes, implemented double‑chamber active temperature control for radial‑velocity stability, and added the FIEStool data‑reduction package. These upgrades have made FIES a work‑horse instrument for the NOT user community. © 2014 WILEY‑VCH Verlag GmbH & Co.
Abstract 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. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
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