We present the results of an on-sky point spread function reconstruction (PSF-R) experiment for the Gemini North telescope adaptive optics system, Altair, in the simplest mode, bright on-axis natural guise star. We demonstrate that our PSF-R method does work for system performance diagnostic but suffers from hidden telescope and system aberrations that are not accounted for in the model, making the reconstruction unsuccessful for Altair, for now. We discuss the probable origin of the discrepancy. In the last section, we propose alternative PSF-R methods for future multiple natural and laser guide stars systems
International audienceIn preparation of future multiobject spectrographs (MOS) whose one of the majo...
Adaptive optics (AO) allows one to derive the point spread function (PSF) simultaneously to the scie...
Context. Modeling the optical point spread function (PSF) is particularly challenging for adaptive o...
We present the results of an on-sky point spread function reconstruction (PSF-R) experiment for the ...
We present the results of an on-sky point spread function reconstruction (PSF-R) experiment for the ...
We present the results of an on-sky point spread function reconstruction (PSF-R) experiment for the ...
We discuss in this paper the last results of our adaptive optics point spread function reconstructio...
We present the final development of our point spread function reconstruction algorithm for the Keck-...
The progress achieved in implementing Point Spread Function reconstruction (PSF-R) capability at W. ...
We present in this paper an analysis of our preliminary results for point spread function reconstruc...
Accepted for publication in A&A; 6 pages, 3 figuresInternational audienceContext. The knowledge of t...
International audienceScientific exploitation in ground-based astronomy is improved thanks to adapti...
From analyzing adaptive optics (AO) images of stars obtained at Keck (10 m telescope) and Gemini Nor...
Context.The knowledge of the point-spread function compensated by adaptive optics is of prime import...
International audienceContext. Modeling the optical point spread function (PSF) is particularly chal...
International audienceIn preparation of future multiobject spectrographs (MOS) whose one of the majo...
Adaptive optics (AO) allows one to derive the point spread function (PSF) simultaneously to the scie...
Context. Modeling the optical point spread function (PSF) is particularly challenging for adaptive o...
We present the results of an on-sky point spread function reconstruction (PSF-R) experiment for the ...
We present the results of an on-sky point spread function reconstruction (PSF-R) experiment for the ...
We present the results of an on-sky point spread function reconstruction (PSF-R) experiment for the ...
We discuss in this paper the last results of our adaptive optics point spread function reconstructio...
We present the final development of our point spread function reconstruction algorithm for the Keck-...
The progress achieved in implementing Point Spread Function reconstruction (PSF-R) capability at W. ...
We present in this paper an analysis of our preliminary results for point spread function reconstruc...
Accepted for publication in A&A; 6 pages, 3 figuresInternational audienceContext. The knowledge of t...
International audienceScientific exploitation in ground-based astronomy is improved thanks to adapti...
From analyzing adaptive optics (AO) images of stars obtained at Keck (10 m telescope) and Gemini Nor...
Context.The knowledge of the point-spread function compensated by adaptive optics is of prime import...
International audienceContext. Modeling the optical point spread function (PSF) is particularly chal...
International audienceIn preparation of future multiobject spectrographs (MOS) whose one of the majo...
Adaptive optics (AO) allows one to derive the point spread function (PSF) simultaneously to the scie...
Context. Modeling the optical point spread function (PSF) is particularly challenging for adaptive o...