2008
DOI: 10.1117/12.790342
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Active Phasing Experiment: preliminary results and prospects

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Cited by 16 publications
(8 citation statements)
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“…Finally, we should say that a sensor prototype -the Pyramid Phasing Sensor (PYPS) 10 -is currently being tested at ESO within the framework of the Active Phase Experiment (APE). 11,12 Although there is only one segmented mirror in the APE bench, it will be possible to place additional masks on the optical train to simulate the presence of an additional segmentation. Of course, no double-segmentation control can be fully tested in this way.…”
Section: Conclusion and Further Workmentioning
confidence: 99%
“…Finally, we should say that a sensor prototype -the Pyramid Phasing Sensor (PYPS) 10 -is currently being tested at ESO within the framework of the Active Phase Experiment (APE). 11,12 Although there is only one segmented mirror in the APE bench, it will be possible to place additional masks on the optical train to simulate the presence of an additional segmentation. Of course, no double-segmentation control can be fully tested in this way.…”
Section: Conclusion and Further Workmentioning
confidence: 99%
“…This may be done either with capacitive or inductive discrete edge sensors as in segmented primary mirrors [16,17], or with various optical sensors [18][19][20] that give a more or less averaged measure of the phasing error along the segment edge (see Fig. 3).…”
Section: Control Strategymentioning
confidence: 99%
“…Several types of phasing sensors have been validated on sky using 10 m-class telescopes, such as the Shack-Hartmann [11][12][13], the Pyramid [13] and the Zernike phasing sensors [13][14][15]. These sensors provide comparable performances, reaching about 20 nm rms piston error (wavefront) in closed-loop for a star as faint as 18th magnitude, reaching a piston error as low as 6 nm rms for bright stars.…”
Section: Introductionmentioning
confidence: 99%