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      The MICADO first light imager for the ELT: the PSF Reconstruction Software

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          Abstract

          MICADO is the first-light camera of the ESO ELT, allowing NIR imaging and long-slit spectroscopy assisted by adaptive optics. MICADO is now entering its construction phase, and the software for data reduction is reaching an adequate maturity level. The PSF Reconstruction (PSF-R) of MICADO is a software tool for the blind derivation of the PSF, only using adaptive optics telemetry data. An update of the status of the PSF-R service is provided here. The PSF-R prototype has been tested on ERIS@VLT data in order to check the reconstruction of on- and off-axis PSFs. The on-axis PSF-R is accurate at a few percent level on Strehl, FWHM, Encircled Energy, and half light radius, while for the off-axis case the match is within 10-15 percent at a distance of half isoplanatic angle. The first version of the workflow for the PSF-R pipeline has been developed and verified using the latest release of the ESO data processing system. A set of simulations has been implemented on the morphological analysis of distant galaxies, showing that the accuracy of the PSF-R matches the goals needed to study their morphology. In summary, the PSF-R team is on the right track towards the ELT first light.

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          Author and article information

          Journal
          12 July 2024
          Article
          2407.09132
          6647de75-c2b5-4dcc-9e51-f7010bbb8ef9

          http://creativecommons.org/licenses/by/4.0/

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          Custom metadata
          5 pages, 3 figures, Proceedings for the SPIE Astronomical Telescopes and Instrumentation 2024, Adaptive Optics Systems IX, Paper No.13097-234
          astro-ph.IM

          Instrumentation & Methods for astrophysics
          Instrumentation & Methods for astrophysics

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