One of the challenges faced by the adaptive optics systems on extremely large telescopes, such as the European Extremely Large Telescope (EELT), is the pupil segmentation caused by the secondary mirror support structure (spider). We introduce a sensitivity metric to evaluate the sensitivity of the pyramid wavefront sensor to segment piston and propose a hybrid control method where both modulated and unmodulated pyramid wavefront sensor measurements are used. The modulated measurements correct the bulk of the atmospheric turbulence whilst the unmodulated measurements are used to correct the residual segment piston errors. Our hybrid approach provides a 5.6% improvement in Strehl under poor seeing (r0 =10 cm ) and 2.7% improvement under...
The Giant Segmented Mirror Telescopes (GSMTs) including the Giant Magellan Telescope (GMT), the Thir...
Context. The diffusion of adaptive optics systems in astronomical instrumentation for large ground-b...
The pyramid wavefront sensor (PWFS) is the currently preferred design for high-sensitivity adaptive ...
The next generation of Extremely Large Telescope (24 to 39m diameter) will suffer from the so-called...
Images observed at ground-based telescopes are blurred by Earth’s atmosphere. Adaptive optics syste...
Imaging astronomical objects, such as stars, planets and galaxies, with ground-based telescopes, is ...
Context. The pyramid was proven to be a highly sensitive and versatile wave-front sensor (WFS) and h...
The next generation of Extremely Large Telescope (24 to 39m diameter) will suffer from the so-called...
International audienceThe next generation of Extremely Large Telescope (24 to 39m diameter) will suf...
As already noticed in other telescopes, the presence of large telescope spiders and of a segmented d...
Context. The diffusion of adaptive optics systems in astronomical instrumentation for large ground b...
The Giant Segmented Mirror Telescopes (GSMTs) including the Giant Magellan Telescope (GMT), the Thir...
The Giant Segmented Mirror Telescopes (GSMTs) including the Giant Magellan Telescope (GMT), the Thir...
Context. The diffusion of adaptive optics systems in astronomical instrumentation for large ground-b...
The pyramid wavefront sensor (PWFS) is the currently preferred design for high-sensitivity adaptive ...
The next generation of Extremely Large Telescope (24 to 39m diameter) will suffer from the so-called...
Images observed at ground-based telescopes are blurred by Earth’s atmosphere. Adaptive optics syste...
Imaging astronomical objects, such as stars, planets and galaxies, with ground-based telescopes, is ...
Context. The pyramid was proven to be a highly sensitive and versatile wave-front sensor (WFS) and h...
The next generation of Extremely Large Telescope (24 to 39m diameter) will suffer from the so-called...
International audienceThe next generation of Extremely Large Telescope (24 to 39m diameter) will suf...
As already noticed in other telescopes, the presence of large telescope spiders and of a segmented d...
Context. The diffusion of adaptive optics systems in astronomical instrumentation for large ground b...
The Giant Segmented Mirror Telescopes (GSMTs) including the Giant Magellan Telescope (GMT), the Thir...
The Giant Segmented Mirror Telescopes (GSMTs) including the Giant Magellan Telescope (GMT), the Thir...
Context. The diffusion of adaptive optics systems in astronomical instrumentation for large ground-b...
The pyramid wavefront sensor (PWFS) is the currently preferred design for high-sensitivity adaptive ...