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Publikováno v:
Modeling, Systems Engineering, and Project Management for Astronomy IX.
The European Southern Observatory (ESO) is managing the Extremely Large Telescope (ELT) system performance and budgets. The Telescope Main Structure, Hosted Optical Units and Scientific Instruments are designed and built outside ESO by contractors an
Autor:
Oliver Dietzel, Liang Rong, Andreas Reinacher, Pascal Bankovic, B. Sedghi, Marc Cayrel, Pablo Zuluaga Ramirez, M. Dimmler, Michael Ebert, Lorenzo Pettazzi, Andreas Zürcher, Timo Maier, Pablo Barriga, Christoph Stiebel
Publikováno v:
Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation IV.
The present paper reports on the results of the validation test campaign of the ELT M1 Position Actuators (M1 PACTs). The main function of these actuators is positioning the 798 segments composing the primary mirror (M1) of the ELT with nanometric tr
Autor:
Jose Abad-Pastor, Ulrich Lampater, Sandro Patti, Serban Leveratto, B. Sedghi, Juan Carlos González-Herrera, Pablo Zuluaga-Ramírez, Michael Müller, Dan Pilbauer, Gerd Jakob
Publikováno v:
Modeling, Systems Engineering, and Project Management for Astronomy IX.
ESO took a systematic approach at earliest phases of the ELT programme to address different aspects of vibration at telescope, from modelling, error budgeting, requirement specifications, to envisaging verification and mitigation methods. Recent acti
Autor:
Christophe Verinaud, E. Vernet, Enrico Marchetti, Lorenzo Pettazzi, Pierre-Yves Madec, Miska Le Louarn, Michael Esselborn, M. Müller, Jerome Paufique, Fabio Biancat-Marchet, M. Dimmler, Sylvain Oberti, B. Sedghi, Nick Kornweibel, Henri Bonnet, Jason Spyromilio, Stefan Stroebele
Publikováno v:
Adaptive Optics Systems VI.
The construction of a diffraction limitable telescope as large as the ESO’s ELT is enabled by its embedded deformable quaternary mirror. Besides its essential function in the telescope control, M4 also contributes to compensating the free atmospher
Autor:
Marcus Schilling, Ulrich Lampater, Heiko Sommer, Nick Kornweibel, Gianluca Chiozzi, B. Sedghi, Mario Kiekebusch
Publikováno v:
Software and Cyberinfrastructure for Astronomy V.
The Extremely Large Telescope (ELT) is a 39 meters optical telescope under construction at an altitude of about 3000m in the Chilean Atacama desert. The optical design is based on a novel five-mirror scheme and incorporates adaptive optics mirrors. T
Publikováno v:
SPIE Proceedings.
The E-ELT primary mirror is 39m in diameter composed of 798 segments. It is exposed to external large but slow amplitude perturbations, mostly gravity, thermal and wind. These perturbations are efficiently rejected by a combination of edge sensor loo
Publikováno v:
SPIE Proceedings.
In this paper we will briefly revisit the optical vibration measurement system (OVMS) at the Large Binocular Telescope (LBT) and how these values are used for disturbance compensation and particularly for the LBT Interferometer (LBTI) and the LBT Int
Autor:
F. Gago, Stefan Ströbele, J. P. Kirchbauer, Antonio Manescau, Norbert Hubin, Sylvain Oberti, J. Quentin, Javier Argomedo, P. La Penna, Robin Arsenault, B. Delabre, Barbara Klein, B. Sedghi, J. L. Lizon, Sebastien Tordo, P. Y. Madec, Mario Kiekebusch, E. Aller Carpentier, P. Gutierrez-Cheetam, Harald Kuntschner, Ralf Conzelmann, M. Suarez Valles, Paul Jolley, Johann Kolb, Christian Soenke, Leander Mehrgan, Rob Donaldson, Joel Vernet, M. Le Louarn
Publikováno v:
Adaptive Optics Systems V.
GALACSI is the Adaptive Optics (AO) module that will serve the MUSE Integral Field Spectrograph. In Wide Field Mode it will enhance the collected energy in a 0.2”×0.2” pixel by a factor 2 at 750 nm over a Field of View (FoV) of 1’×1’ using
Publikováno v:
SPIE Proceedings.
The E-ELT dynamical modeling toolkit is used extensively to understand the effect of vibrations from observatory equipments on the final performance of the telescope. The dynamical and control modeling toolkit uses the finite element model of the tel