After about 15 years of operation with astronomical instruments, adaptive optics has now reached maturity: it is routinely used at several large telescopes and transparent for the astronomer. Though, adaptive optics assisted images have specificities compared to seeing-limited images, such as their point spread function profile or spatial/temporal variability, that I review in the following. Adaptive optics imaging, unlike seeing-limited imaging, offers the possibility to calibrate the PSF simultaneously to the scientific observations, using real-time measurements of the adaptive optics system itself. I introduce here this PSF reconstruction and review the different PSF reconstruction algorithms developed till now, in particular the one for NAOS. © 2008 Springer-Verlag Berlin Heidelberg.
CITATION STYLE
Clénet, Y., Gendron, E., Rousset, G., Fusco, T., Lidman, C., Kasper, M., … Marco, O. (2008). Imaging and treatment of the PSF in AO instruments: Application to NACO. In ESO Astrophysics Symposia (Vol. 2008, pp. 259–269). https://doi.org/10.1007/978-3-540-76963-7_36
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