Plans for future optical telescopes of diameter more than 10 m are based on segmented mirrors, made up of hundreds or even thousands of segments. A challenge for these telescopes is the alignment in piston (cophasing) where phase differences between individual segments have to be reduced to a small fraction of the observing wavelength in order to avoid degradation of image quality. Based on the phase discontinuity sensing method used at the Keck telescopes to measure small piston errors using infrared wavelengths, we develop a new method that allows fast high-precision measurements of large piston errors even at visible wavelengths
International audienceWe propose and apply two methods to estimate pupil plane phase discontinuities...
We propose a new phase calibration method, called the sensor-by-sensor phase calibration method (SSP...
International audienceContext. Segmented aperture telescopes require an alignment procedure with suc...
One of the main challenges in space observations is to observe always fainter and more compact objec...
One of the main problems arising in the co-phasing of segmented telescopes is the problem of measure...
To achieve its full diffraction limit in the infrared, the primary mirror of the Keck telescope (now...
International audienceFuture extremely large telescopes will adopt segmented primary mirrors with se...
International audienceThe demand for higher resolution telescopes leads to segmented primary mirrors...
As next-generation large-aperture telescopes, synthetic aperture is a promising method for realizing...
A segmented primary mirror is very important for extra-large astronomical telescopes, in order to de...
Context. Direct imaging of Earth-like exoplanets requires very high contrast imaging capability and ...
Nowadays spaceborne missions for astronomy or Earth imaging need high resolution observation which i...
Context. Segmented aperture telescopes require an alignment procedure with successive steps from coa...
Astronomical telescopes with increasingly large apertures are required to upgrade the limit of diffr...
International audienceWe propose and apply two methods to estimate pupil plane phase discontinuities...
We propose a new phase calibration method, called the sensor-by-sensor phase calibration method (SSP...
International audienceContext. Segmented aperture telescopes require an alignment procedure with suc...
One of the main challenges in space observations is to observe always fainter and more compact objec...
One of the main problems arising in the co-phasing of segmented telescopes is the problem of measure...
To achieve its full diffraction limit in the infrared, the primary mirror of the Keck telescope (now...
International audienceFuture extremely large telescopes will adopt segmented primary mirrors with se...
International audienceThe demand for higher resolution telescopes leads to segmented primary mirrors...
As next-generation large-aperture telescopes, synthetic aperture is a promising method for realizing...
A segmented primary mirror is very important for extra-large astronomical telescopes, in order to de...
Context. Direct imaging of Earth-like exoplanets requires very high contrast imaging capability and ...
Nowadays spaceborne missions for astronomy or Earth imaging need high resolution observation which i...
Context. Segmented aperture telescopes require an alignment procedure with successive steps from coa...
Astronomical telescopes with increasingly large apertures are required to upgrade the limit of diffr...
International audienceWe propose and apply two methods to estimate pupil plane phase discontinuities...
We propose a new phase calibration method, called the sensor-by-sensor phase calibration method (SSP...
International audienceContext. Segmented aperture telescopes require an alignment procedure with suc...