The Ingot WFS ON an ELT-like telescope: the project and simulations
Elisa Portaluri, Simone Di Filippo, Valentina Viotto, Roberto, Ragazzoni, Carmelo Arcidiacono, Davide Greggio, Kalyan Radhakrishnan, Maria, Bergomi, Luca Marafatto, Marco Dima, Jacopo Farinato, Demetrio Magrin,, Gianluca Di Rico, Mauro Centrone, and Domenico Bonaccini

TL;DR
This paper discusses the development and simulation of the Ingot Wavefront Sensor for ELT-like telescopes, aiming to address limitations of laser guide stars through innovative sensor design and performance evaluation.
Contribution
It introduces the Ingot WFS concept, details simulation and laboratory testing plans, and outlines future sky verification for ELT-like telescopes.
Findings
Ingot WFS shows promise in overcoming LGS limitations
Simulations indicate potential performance improvements
Laboratory experiments are planned for validation
Abstract
The Ingot WFS represents an innovative and indispensable class of sensors conceived to overcome some limitations due to the LGSs geometry, which is significantly different from the point-object originated by a NGS. Here we overview the project, aiming at investigating the performance of an ELT-like telescope equipped with the Ingot WFS, facing different aspects of the program: the needs for numerical simulations and laboratory experiments, the prototype and, finally the future plan for the verification on sky.
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Adaptive optics and wavefront sensing
