Design of the opto-mechanical mounts of the ESPRESSO spectograph
2014
ESPRESSOis the next generation European
exoplanethunter, combining the efficiency of a modern echelle spectrograph with extreme
radial velocityand spectroscopic precision. The instrumental
radial velocityprecision will be improved to reach 10 cm/s level, to achieve a gain of two magnitudes with respect to its predecessor
HARPS. The fiber-fed, non-rotating instrument will be installed in the Combined Coude Laboratory of the VLT (Very Large Telescope), which is situated in the Paranal Observatory (Chile). The main challenge in the design of the optical mounts of the instrument has been the extreme long-term stability of big rectangular optical components in a seismic environment. This paper describes the requirements and the adopted solution for the opto-
mechanical designof the collimator mirrors, dichroic lens, field lens and cross dispersers of the instrument.
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