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Update paper.md on web interface
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benjaminpope authored Jul 22, 2024
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authors:
- name: Louis Desdoigts
orcid: 0000-0002-1015-9029
affiliation: 1 # (Multiple affiliations must be quoted)
affiliation: 1
corresponding: true
- name: Benjamin J. S. Pope
affiliation: "2,3"
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orcid: 0000-0001-8125-6494
- name: Adam K. Taras
orcid: 0000-0002-4558-2222
affiliation: 1 # (Multiple affiliations must be quoted)
affiliation: 1
- name: Max Charles
orcid:
affiliation: 1
affiliations:
- name: School of Physics, University of Sydney, Camperdown, NSW 2006, Australia
index: 1
- name: School of Mathematics and Physics, University of Queensland, St Lucia, QLD 4072, Australia
index: 2
- name: Centre for Astrophysics, University of Southern Queensland, West Street, Toowoomba, QLD 4350, Australia
index: 3
date: 9 Feb 2024
date: 22 Jul 2024
bibliography: paper.bib
---

# Summary

<!-- why physical optics in astronomy -->
One of the foundational problems in optical astronomy is that of imaging scenes at resolutions close to the diffraction limit of a telescope. This is important both in ground-based astronomy, where the turbulent atmosphere blurs the

<!-- what is dLux -->
`dLux`[^dlux] is an first open-source Python package for physical optics simulation. Using `jax` [@jax] it is differentiable and deploys natively on CPU, GPU, and parallelized HPC environments. `dLux` can perform Fourier optical simulations using matrix and FFT based propagation, as well as simulate linear and nonlinear detector effects.
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