Abstract
During the 2nd semester of 2016, a new Deformable Secondary Mirror (DSM), part of the Adaptive Optics Facility Project at Paranal Observatory, was installed on the Unit Telescope 4. Starting end of November 2016, we then re-commissioned the telescope and the following three instruments : HAWK-I, MUSE and SINFONI. It is important to understand how a DSM, even if used in non-adaptive optics mode (i.e., in its rest/at position), can impact the operations and the quality of the observations. We discuss here the results of this telescope and instrument re-commissioning, the challenges and problems we met, and compare the new performance to the ones obtained previously with the traditional Dornier Secondary Mirror.
Original language | English |
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DOIs | |
Publication status | Published - 2017 |
Externally published | Yes |
Event | 5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017 - Tenerife, Canary Islands, Spain Duration: 25 Jun 2017 → 30 Jun 2017 https://web.archive.org/web/20200117115411/https://research.iac.es/congreso/AO4ELT5/pages/proceedings.html https://web.archive.org/web/20240710213944/http://research.iac.es/congreso/AO4ELT5/index.html |
Conference
Conference | 5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017 |
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Abbreviated title | AO4ELT5 |
Country/Territory | Spain |
City | Tenerife, Canary Islands |
Period | 25/06/17 → 30/06/17 |
Other | The fifth Adaptive Optics for Extremely Large Telescopes (AO4ELT5) meeting will be taking place in June 2017 at the Hotel Botánico in Puerto de la Cruz, Tenerife. One of the major challenges that face the future extremely large aperture telescopes (ELT's) is adaptive optics, and the goal of the meeting is to gather specialists to review and discuss the latest developments on this field. The topics of the conference include ELT’s current design in terms of AO systems, related instruments and science goals, and also pathfinder projects planned or implemented on existing telescopes, including solar telescopes, which provide relevant results for the next ELT’s design phase. Special attention will be given to new developments in several areas, such as mirrors, laser technologies, wavefront sensing and control, and new post-processing tools required to increase the image quality and increase the scientific return of the instruments. |
Internet address |