Poster + Paper
27 August 2024 The MICADO first light imager for the ELT: MISTHIC simulation pipeline for the high contrast mode of MICADO
Author Affiliations +
Conference Poster
Abstract
We present the Python pipeline that was developed to simulate the high contrast mode images of the MICADO instrument. This mode will comprise three classical Lyot coronagraphs with different occulting spot sizes, one vector apodized phase plate, and two sparse aperture masks. One critical aspect of these modes lies in their sensitivity to aberrations, requiring careful integration of non common path aberrations, as well as turbulent adaptive optics (AO) residuals. Besides, they will be operated following a specific observing strategy based on pupil tracking mode. For these reasons, we have developed the MICADO SimulaTor for HIgh Contrast (MISTHIC) pipeline to simulate realistic image cubes and derive the expected performance of these modes. Several sources of aberrations can be included: turbulent AO residuals, but also static or rotating aberrations, amplitude aberrations, simple Zernike screens. Including MICADO’s specific features, such as the absence of atmospheric dispersion prior to the coronagraphic focal plane mask, our intent is to make this pipeline available to the community. This tool can be used to prepare scientific observations with the high contrast mode of MICADO, by predicting the performance to be expected within the most realistic assumptions.
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
E. Huby, P. Baudoz, F. Vidal, H. Baran, Y. Clénet, and R. Davies "The MICADO first light imager for the ELT: MISTHIC simulation pipeline for the high contrast mode of MICADO", Proc. SPIE 13097, Adaptive Optics Systems IX, 1309776 (27 August 2024); https://doi.org/10.1117/12.3020009
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KEYWORDS
Coronagraphy

Pupil aberrations

Stars

Point spread functions

Computer simulations

Device simulation

Planets

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