New developments on the Ingot WFS laboratory testing
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| Main Authors: | , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866910641216815104 |
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| author | Machado, Tânia Gomes Di Filippo, Simone Santhakumari, Kalyan K. R. Bergomi, Maria Greggio, Davide Portaluri, Elisa Malik, Dheeraj Nesme, César Arcidiacono, Carmelo Ballone, Alessandro Battaini, Federico Viotto, Valentina Ragazzoni, Roberto Dima, Marco Marafatto, Luca Farinato, Jacopo Magrin, Demetrio Lessio, Luigi Umbriaco, Gabriele |
| author_facet | Machado, Tânia Gomes Di Filippo, Simone Santhakumari, Kalyan K. R. Bergomi, Maria Greggio, Davide Portaluri, Elisa Malik, Dheeraj Nesme, César Arcidiacono, Carmelo Ballone, Alessandro Battaini, Federico Viotto, Valentina Ragazzoni, Roberto Dima, Marco Marafatto, Luca Farinato, Jacopo Magrin, Demetrio Lessio, Luigi Umbriaco, Gabriele |
| contents | The Ingot WFS was designed to overcome some of the challenges present in classical wavefront sensors when they deal with sodium LGSs. This innovative sensor works by sensing the full 3D volume of the elongated LGS and is suitable for use in very large telescopes. A test bench has been assembled at the INAF - Osservatorio Astronomico di Padova laboratories to test and characterize the functioning of the Ingot WFS. In this work, we summarize the main results of the tests performed on a new search algorithm. Then, we move towards a more accurate simulation of the sodium LGS by replicating real time-varying sodium layer profiles. The study of their impact on the ingot pupil signals is described in this work. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_06260 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | New developments on the Ingot WFS laboratory testing Machado, Tânia Gomes Di Filippo, Simone Santhakumari, Kalyan K. R. Bergomi, Maria Greggio, Davide Portaluri, Elisa Malik, Dheeraj Nesme, César Arcidiacono, Carmelo Ballone, Alessandro Battaini, Federico Viotto, Valentina Ragazzoni, Roberto Dima, Marco Marafatto, Luca Farinato, Jacopo Magrin, Demetrio Lessio, Luigi Umbriaco, Gabriele Instrumentation and Methods for Astrophysics The Ingot WFS was designed to overcome some of the challenges present in classical wavefront sensors when they deal with sodium LGSs. This innovative sensor works by sensing the full 3D volume of the elongated LGS and is suitable for use in very large telescopes. A test bench has been assembled at the INAF - Osservatorio Astronomico di Padova laboratories to test and characterize the functioning of the Ingot WFS. In this work, we summarize the main results of the tests performed on a new search algorithm. Then, we move towards a more accurate simulation of the sodium LGS by replicating real time-varying sodium layer profiles. The study of their impact on the ingot pupil signals is described in this work. |
| title | New developments on the Ingot WFS laboratory testing |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2410.06260 |