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[en] In our contribution, we outline the different steps in the design of a fiber-fed spectrographic instrument
for stellar astrophysics. Starting from the derivation of theoretical relationships from the scientific requirements
and telescope characteristics, the entire optical design of the spectrograph is presented. Specific optical
elements, such as a toroidal lens, are introduced to improve the instrument’s efficiency. Then the verification
of predicted optical performances is investigated through optical analyses, such as resolution checking.
Centre/Unité de recherche :
CSL - Centre Spatial de Liège - ULiège Groupe d'Astrophysique des Hautes Energies - GAPHE Astrophysique Stellaire Théorique et Astérosismologie - ASTA
Disciplines :
Aérospatiale, astronomie & astrophysique
Auteur, co-auteur :
Kintziger, Christian ; Université de Liège > Département d'aérospatiale et mécanique > Instrumentation et expérimentation spatiales
Desselle, Richard ; Université de Liège > Département d'aérospatiale et mécanique > Instrumentation et expérimentation spatiales
Loicq, Jerôme ; Université de Liège > CSL (Centre Spatial de Liège)
Rauw, Grégor ; Université de Liège > Groupe d'astrophysique des hautes énergies (GAPHE)
Rochus, Pierre ; Université de Liège > CSL (Centre Spatial de Liège)
Langue du document :
Anglais
Titre :
Conception of a near-infrared spectrometer for ground-based observations of massive stars
Date de publication/diffusion :
21 février 2017
Titre du périodique :
Journal of Astronomical Telescopes, Instruments, and Systems
ISSN :
2329-4124
eISSN :
2329-4221
Maison d'édition :
International Society for Optical Engineering (SPIE)
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