http://arxiv.org/abs/1612.04680
The SPIFFI integral field spectrometer is operated as a subunit of the AO instrument SINFONI on the VLT. It will be upgraded and reused as SPIFFIER in the new VLT instrument ERIS. In January 2016 an early upgrade of several optical components was carried out to make use of new technological developments before ERIS will be commissioned in 2020.
This Master’s thesis focuses on the determination and detailed description of the gain in performance due to the upgrade, with a particular focus on measurements of the exchanged diamond turned mirrors of SPIFFI. An analysis of the surface deformation of these mirrors is done, followed by a determination of the resulting collimator wavefront and its influence on the line spread function of the spectrometer. A careful analysis on the shapes, the variations and the changes of the spectral line profiles due to the upgrade is done. Furthermore, the spectral resolution, the image quality an the relative pre- and post- upgrade throughput ratio are evaluated. Finally these observed quantities are linked to critical optical components that limit the performance of the instrument.
D. Graff
Thu, 15 Dec 16
41/59
Comments: This is a Master’s Thesis written at the Max Planck Institute For Extraterrestrial Physics and the Technical University of Munich. The working title of the thesis was: “Upgrade of the SPIFFI instrument with new optics, and characterization of the upgraded instrument”
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