HARMONI at ELT: modelling the optical performance of a diffraction limited integral field spectrograph

HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 470 nm to 2450 nm with resolving powers from 3300 to 18000 and spatial sampling from 60 mas to 4 mas. It can operate in two Adaptive Optics modes - SCAO (including a High Contrast capability) and LTAO - or with NOAO. To model the optical performance we include manufacturing and alignment tolerances alongside other static and dynamic effects. Diffraction of both image and pupil become significant when the spectrograph slit width matches the diffraction limited point spread function. A set of Zemax OpticStudio macros and Python scripts are used to bring together the subsystem models that make up HARMONI and combine them to include all these effects. We present an overview of our approach to modelling this complex instrument and key results predicting the optical performance of HARMONI.

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Published
2024-08-23
DOI
https://doi.org/10.1117/12.3019747
Primary Topic
Astronomy and Astrophysical Research
Type
article
Field-Weighted Citation Impact
0.00

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article

HARMONI at ELT: modelling the optical performance of a diffraction limited integral field spectrograph

Álvaro Menduiña-Fernández, E. Harvey, Fraser Clarke, Matthias Tecza et al.
Astronomy and Astrophysical Research
article

HARMONI at ELT: modelling the optical performance of a diffraction limited integral field spectrograph

Álvaro Menduiña-Fernández, E. Harvey, Fraser Clarke, Matthias Tecza, Charlotte Z. Bond, Stephen Todd
article en

Abstract

HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 470 nm to 2450 nm with resolving powers from 3300 to 18000 and spatial sampling from 60 mas to 4 mas. It can operate in two Adaptive Optics modes - SCAO (including a High Contrast capability) and LTAO - or with NOAO. To model the optical performance we include manufacturing and alignment tolerances alongside other static and dynamic effects. Diffraction of both image and pupil become significant when the spectrograph slit width matches the diffraction limited point spread function. A set of Zemax OpticStudio macros and Python scripts are used to bring together the subsystem models that make up HARMONI and combine them to include all these effects. We present an overview of our approach to modelling this complex instrument and key results predicting the optical performance of HARMONI.

Vol. 6675
Civil Aviation Authority (GB), University of Oxford (GB), UK Astronomy Technology Centre (GB)
Science and Technology Facilities Council
Affordable and clean energy
Openalex Percentile: Top 89%
Astronomy and Astrophysical Research
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HARMONI at ELT: modelling the optical performance of a diffraction limited integral field spectrograph — Álvaro Menduiña-Fernández, E. Harvey, et al. · (2024) | TGRS Research Map | TGRS