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End to end optical design and wavefront error simulation of METIS

MPS-Authors

Agócs,  Tibor
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Zuccon,  Sara
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Jellema,  Willem
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

van den Born,  Joost
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

ter Horst,  Rik
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Bizenberger,  Peter
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Cardenas Vazquez,  M. Concepcion
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Todd,  Stephen
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Baccichet,  Nicola
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Straubmeier,  Christian
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

External Resource

https://ui.adsabs.harvard.edu/abs/2018SPIE10702E..9OA
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Citation

Agócs, T., Zuccon, S., Jellema, W., van den Born, J., ter Horst, R., Bizenberger, P., et al. (2018). End to end optical design and wavefront error simulation of METIS.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CF4C-E
Abstract
We present the preliminary optical design of METIS, the Mid-infrared E-ELT Imager and Spectrograph, and study the end-to-end performance regarding wavefront errors and non-common path aberrations. We discuss the results of the Monte Carlo simulations that contain the manufacturing and alignment errors of the opto-mechanical system. We elaborate on the wavefront error budget of the instrument detailing all contributors. We investigate the mid and high spatial frequency errors of the optical surfaces, which we model using simulated surface height errors maps of one dimensional Power Spectral Density (PSD) functions.