Paper 14154-331
The MICADO first light imager for the ELT: manufacturing of the large dichroic plate of its SCAO module
5 July 2026 • 17:30 - 19:00 CEST | Room B2-M4
Abstract
MICADO, a first-light instrument on the European Extremely Large Telescope, operates in the NIR, offering imaging, astrometry, spectroscopy, and high-contrast capabilities. The optical design of its single conjugate adaptive optics (SCAO) module features a 305 mm CaF₂ dichroic plate that splits light between AO and the scientific camera, achieving over 97% transmission from 960–2450 nm and >92% reflectivity from 589–960 nm. The front surface has a thin-film optical filter optimized to minimize coating-induced stress and sensitivity to manufacturing errors. Deposition was performed via ion-beam sputtering with careful control of thermal gradients and post-deposition annealing to release internal stress. The back side has a 16-layer broadband anti-reflective coating ensuring >98.5% transmission. Post-coating characterization confirmed uniform transmission over a 290 mm aperture and reflected wavefront errors within specifications, demonstrating high optical performance.
Presenter
Lab. des Matériaux Avancés, Institut de Physique des 2 Infinis de Lyon, Univ. Claude Bernard Lyon 1, CNRS (France)
Benoit Sassolas is a research engineer at LMA/IP2I (Villeurbanne - France) with 20 years of experience in coatings research. He was involved in the developments of the large mirrors for the second generation gravitational waves detectors (Advanced LIGO, Advanced Virgo, KAGRA), the Fabry-Perot etalon for the DKIS telescope or the fabrication of large dichroic plates for PFS of the SUBARU telescope and 4MOST of the VISTA telecope. He works on thin-film design, manufacturing and characterization of very large optical filters by PVD techniques.