Ground-Based and Airborne Instrumentation for Astronomy IX 2022
DOI: 10.1117/12.2629962
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From assembly to the complete integration and verification of the SOXS common path

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“…Both the outputs have two baffle to avoid spurious light from entering the spectrographs. All those elements have been glued in Merate and, after a first check of the results, have been shipped to Padua together with the CP structure for the optical alignment of the subsystem (described in [4]) Other important elements are the kinematic mounts (in blue) used to install the CP on the interface flange and the Acquisition Camera on the CP. On the bottom part of the CP structure, another set of kinematic mounts identical to the acquisition camera one is used to install the calibration unit.…”
Section: Common Path (Cp)mentioning
confidence: 99%
“…Both the outputs have two baffle to avoid spurious light from entering the spectrographs. All those elements have been glued in Merate and, after a first check of the results, have been shipped to Padua together with the CP structure for the optical alignment of the subsystem (described in [4]) Other important elements are the kinematic mounts (in blue) used to install the CP on the interface flange and the Acquisition Camera on the CP. On the bottom part of the CP structure, another set of kinematic mounts identical to the acquisition camera one is used to install the calibration unit.…”
Section: Common Path (Cp)mentioning
confidence: 99%