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Gregor@night: The future high‐resolution stellar spectrograph for the GREGOR solar telescope

Identifieur interne : 000519 ( Istex/Curation ); précédent : 000518; suivant : 000520

Gregor@night: The future high‐resolution stellar spectrograph for the GREGOR solar telescope

Auteurs : K. G. Strassmeier [Allemagne] ; I. V. Ilyin [Allemagne] ; M. Woche [Allemagne] ; T. Granzer [Allemagne] ; M. Weber [Allemagne] ; J. Weingrill [Allemagne] ; S. Bauer [Allemagne] ; E. Popow [Allemagne] ; C. Denker [Allemagne] ; W. Schmidt [Allemagne] ; O. Von Der Lühe [Allemagne] ; S. Berdyugina [Allemagne] ; M. Collados [Espagne] ; P. Koubsky [République tchèque] ; T. Hackman [Finlande] ; M. J. Mantere [Finlande]

Source :

RBID : ISTEX:17400FD90DBD0C3F55740B5EFC4314F6F2648E4B

English descriptors

Abstract

We describe the future night‐time spectrograph for the GREGOR solar telescope and present its science core projects. The spectrograph provides a 3‐pixel resolution of up to R = 87 000 in 45 échelle orders covering the wavelength range 390‐900 nm with three grating settings. An iodine cell can be used for high‐precision radial velocity work in the 500‐630 nm range. The operation of the spectrograph and the telescope will be fully automated without the presence of humans during night‐time and will be based on the successful STELLA control system. Future upgrades include a second optical camera for even higher spectral resolution, a Stokes‐V polarimeter and a link to the laser‐frequency comb at the Vacuum Tower Telescope. The night‐time core projects are a study of the angular‐momentum evolution of “The Sun in Time” and a continuation of our long‐term Doppler imaging of active stars (© 2012 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

Url:
DOI: 10.1002/asna.201211727

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ISTEX:17400FD90DBD0C3F55740B5EFC4314F6F2648E4B

Le document en format XML

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<div type="abstract" xml:lang="en">We describe the future night‐time spectrograph for the GREGOR solar telescope and present its science core projects. The spectrograph provides a 3‐pixel resolution of up to R = 87 000 in 45 échelle orders covering the wavelength range 390‐900 nm with three grating settings. An iodine cell can be used for high‐precision radial velocity work in the 500‐630 nm range. The operation of the spectrograph and the telescope will be fully automated without the presence of humans during night‐time and will be based on the successful STELLA control system. Future upgrades include a second optical camera for even higher spectral resolution, a Stokes‐V polarimeter and a link to the laser‐frequency comb at the Vacuum Tower Telescope. The night‐time core projects are a study of the angular‐momentum evolution of “The Sun in Time” and a continuation of our long‐term Doppler imaging of active stars (© 2012 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)</div>
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