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- W2010657166 abstract "This paper reports the results of the observations made with the VLT Adaptive Optics Prototype System 'COME-ON' at the ESO 3.6 meter telescope. The analysis of uncorrected and corrected images in the near-IR wavelength range (below 5 microns) leads to a detailed assessment of the system performance in terms of improvement of angular resolution that nearly achieves the ideal diffraction profiles down to 1.7 micron wavelength, as well as a Strehl ratio approaching 0.6-0.8 at 3.8 microns. A resolution of 0.12 arcsec has been obtained with this system at 1.7 microns which is wavelength-dependent on the temporal parameters of the observation. The current limiting magnitude for the reference source is m sub R = 11.5 when applying the full correction capabilities of the system, and m sub R = 13 if only the wavefront tilt is corrected." @default.
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- W2010657166 date "1991-12-01" @default.
- W2010657166 modified "2023-10-14" @default.
- W2010657166 title "<title>Adaptive optics system tests at the ESO 3.6-m telescope</title>" @default.
- W2010657166 doi "https://doi.org/10.1117/12.48819" @default.
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