Results 201 to 210 of about 345,237 (255)
In situ pressure calibration for piston cylinder cells via ruby fluorescence with fiber optics
K Koyama-Nakazawa +3 more
openalex +2 more sources
David Moalem Maron +18 more
openalex +2 more sources
Adaptive optics for array telescopes using piston-and-tilt wave-front sensing
Peter Wizinowich +8 more
openalex +2 more sources
Martin Lapisa +4 more
openalex +2 more sources
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Model-based large-dynamic iterative piston correction using extended objects.
Optics Letters, 2023Cophasing is crucial for segmented or sparse aperture telescopes to achieve high resolution. In this Letter, we propose a novel, to the best of our knowledge, model-based piston correction method that can remove large-scale piston errors within a few ...
Zexia Zhang, Bing Dong
semanticscholar +1 more source
Astronomical Telescopes + Instrumentation, 2022
The success of the Keck telescopes’ segmented mirror technology provided a basis for the development of other large and extremely large telescopes. We investigate ways to optimize the performance of the segmented mirror telescope further to (1) take on ...
S. Ragland, L. Gers
semanticscholar +1 more source
The success of the Keck telescopes’ segmented mirror technology provided a basis for the development of other large and extremely large telescopes. We investigate ways to optimize the performance of the segmented mirror telescope further to (1) take on ...
S. Ragland, L. Gers
semanticscholar +1 more source
Journal of Astronomical Telescopes Instruments and Systems, 2022
. The Giant Magellan Telescope (GMT) design consists of seven circular 8.4-m diameter mirrors, together forming a single 25.4-m diameter primary mirror. This large aperture and collecting area can help extreme adaptive optics (ExAO) systems such as GMT’s
A. Hedglen +16 more
semanticscholar +1 more source
. The Giant Magellan Telescope (GMT) design consists of seven circular 8.4-m diameter mirrors, together forming a single 25.4-m diameter primary mirror. This large aperture and collecting area can help extreme adaptive optics (ExAO) systems such as GMT’s
A. Hedglen +16 more
semanticscholar +1 more source
Design and development of a 331-segment tip–tilt–piston mirror array for space-based adaptive optics
Jason B. Stewart +5 more
openalex +2 more sources
Piston-tip-tilt mirror array in the wide field phasing testbed for the Giant Magellan Telescope
Astronomical Telescopes + Instrumentation, 2022The Wide Field Phasing Testbed (WFPT) will be used to test phasing and active optics systems planned for the doubly segmented Giant Magellan Telescope (GMT). The testbed consists of a set of optical relays including segmented and deformable mirrors (DMs)
Daniel Catropa +14 more
semanticscholar +1 more source
Differential piston sensing with LIFT: application to the GMT
Astronomical Telescopes + Instrumentation, 2022The Giant Magellan Telescope’s primary and deformable secondary mirror are each composed of 7 segments. The Natural Guide Star (NGS) wavefront sensor has the critical task to keep these 7 segments in phase in addition to the classical Adaptive Optics (AO)
A. Cheffot +13 more
semanticscholar +1 more source

