Zemax file echelle spectrograph2/13/2023 This technique makes it possible to reach high spectral resolutions because it uses the diffraction orders > 20 of a grating. They both complement our expertise to bring you the best solution in echelle spectroscopy for astronomy !Ĭhoice of optical fibre has been made to increase radial velocities measurement accuracy and for a better confort in using the eShel. The software module has been written by Michel Pujol, an expert in Tcl/Tk and AudeLA platform. We designed the spectroscope with Christian Buil, a higly recognized optician expert. This practical experience helped us to design a robust and productive solution in the field. It is based on our strong experience in spectroscopy (with design and manufacturing of the Lhires III and Lhires Lite) and nights of observations including with MuSiCoS & Narval spectroscopes.
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