Paper
11 July 2008 X-shooter-backbone and UV-blue and visible spectrographs: final AIV and measured performances
Per Kjærgaard Rasmussen, Filippo M. Zerbi, Hans Dekker, Joel Vernet, Jeppe J. Andersen, Vincenzo De Caprio, Paolo Dimarcantonio, Sandro D'Odorico, Jean-Louis Lizon, Christian Lucuix, Niels Michaelsen, Emilio Molinari, Preben Nørregaard, Alberto Riva, Marco Riva, Paolo Santin, Anton N. Sørensen, Paolo Spanò, Dennis Wistisen
Author Affiliations +
Abstract
X-shooter is a wide band (U to K) intermediate resolution (4000-14000) single object three-arms spectrograph for the VLT. Currently in the last phase of integration, X-shooter will see the first light at ESO Paranal as the first of the VLT second generation instruments in the last quarter of 2008. We describe in this paper the final steps in the integration and testing phase of the central Backbone with its key functions (including the active flexure compensation mirrors) and of the two UV-Blue and Visible spectroscopic arms. We report on the stability results of the preslit optics and of the spectrographs and on the remarkable efficiency which is derived from the measurements of the optical components of the instrument.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Per Kjærgaard Rasmussen, Filippo M. Zerbi, Hans Dekker, Joel Vernet, Jeppe J. Andersen, Vincenzo De Caprio, Paolo Dimarcantonio, Sandro D'Odorico, Jean-Louis Lizon, Christian Lucuix, Niels Michaelsen, Emilio Molinari, Preben Nørregaard, Alberto Riva, Marco Riva, Paolo Santin, Anton N. Sørensen, Paolo Spanò, and Dennis Wistisen "X-shooter-backbone and UV-blue and visible spectrographs: final AIV and measured performances", Proc. SPIE 7014, Ground-based and Airborne Instrumentation for Astronomy II, 70143Z (11 July 2008); https://doi.org/10.1117/12.788745
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KEYWORDS
Spectrographs

Mirrors

Cameras

Optics manufacturing

Telescopes

Optical components

Optical filters

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