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| Indexado |
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| DOI | 10.1117/12.2562735 | ||||
| Año | 2020 | ||||
| Tipo | proceedings paper |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
An electrodynamic exciter was used to impart known dynamic forces into the telescope structure. Acceleration responses were measured at numerous locations on the telescope, including on M1 and M2, using the facility Vibration Monitoring System (VMS) accelerometers. This paper describes the equipment, the experimental approach, and will summarize initial results from these tests.
| Revista | ISSN |
|---|---|
| Proceedings Of Spie The International Society For Optical Engineering | 0277-786X |
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Byrnes, Peter W. G. | Hombre |
Natl Res Council Canada - Canadá
National Research Council Canada - Canadá |
| 2 | Hayward, Thomas L. | Hombre |
Observatorio Gemini - Chile
Gemini ObservatorySouthern Operations Center - Chile |
| 3 | Chinn, Brian | Hombre |
Observatorio Gemini - Chile
Gemini ObservatorySouthern Operations Center - Chile |
| 4 | Marshall, HK | - | |
| 5 | Spyromilio, J | - | |
| 6 | Usuda, T | - |
| Fuente |
|---|
| National Programs Office of the National Research Council of Canada |
| Herzberg Astronomy and Astrophysics Research Centre Astronomy Technology Directorate |
| Agradecimiento |
|---|
| The authors gratefully acknowledge the support of the National Programs Office of the National Research Council of Canada for funding this project, the Herzberg Astronomy and Astrophysics Research Centre Astronomy Technology Directorate for additional support, and of the Gemini observatories for their generosity in allowing access to the telescope and facilities, in particular for their agility in scheduling the work, and for the excellent assistance provided by the observatory staff. |
| The authors gratefully acknowledge the support of the National Programs Office of the National Research Council of Canada for funding this project, the Herzberg Astronomy and Astrophysics Research Centre Astronomy Technology Directorate for additional support, and of the Gemini observatories for their generosity in allowing access to the telescope and facilities, in particular for their agility in scheduling the work, and for the excellent assistance provided by the observatory staff. |