Exoplanet Detection via Differentiable Rendering

Fuente: arXiv
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Hauptverfasser: Feng, Brandon Y., Ferrer-Chávez, Rodrigo, Levis, Aviad, Wang, Jason J., Bouman, Katherine L., Freeman, William T.
Format: Preprint
Veröffentlicht: 2025
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author Feng, Brandon Y.
Ferrer-Chávez, Rodrigo
Levis, Aviad
Wang, Jason J.
Bouman, Katherine L.
Freeman, William T.
author_facet Feng, Brandon Y.
Ferrer-Chávez, Rodrigo
Levis, Aviad
Wang, Jason J.
Bouman, Katherine L.
Freeman, William T.
contents Direct imaging of exoplanets is crucial for advancing our understanding of planetary systems beyond our solar system, but it faces significant challenges due to the high contrast between host stars and their planets. Wavefront aberrations introduce speckles in the telescope science images, which are patterns of diffracted starlight that can mimic the appearance of planets, complicating the detection of faint exoplanet signals. Traditional post-processing methods, operating primarily in the image intensity domain, do not integrate wavefront sensing data. These data, measured mainly for adaptive optics corrections, have been overlooked as a potential resource for post-processing, partly due to the challenge of the evolving nature of wavefront aberrations. In this paper, we present a differentiable rendering approach that leverages these wavefront sensing data to improve exoplanet detection. Our differentiable renderer models wave-based light propagation through a coronagraphic telescope system, allowing gradient-based optimization to significantly improve starlight subtraction and increase sensitivity to faint exoplanets. Simulation experiments based on the James Webb Space Telescope configuration demonstrate the effectiveness of our approach, achieving substantial improvements in contrast and planet detection limits. Our results showcase how the computational advancements enabled by differentiable rendering can revitalize previously underexploited wavefront data, opening new avenues for enhancing exoplanet imaging and characterization.
format Preprint
id arxiv_https___arxiv_org_abs_2501_01912
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Exoplanet Detection via Differentiable Rendering
Feng, Brandon Y.
Ferrer-Chávez, Rodrigo
Levis, Aviad
Wang, Jason J.
Bouman, Katherine L.
Freeman, William T.
Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
Computer Vision and Pattern Recognition
Image and Video Processing
Direct imaging of exoplanets is crucial for advancing our understanding of planetary systems beyond our solar system, but it faces significant challenges due to the high contrast between host stars and their planets. Wavefront aberrations introduce speckles in the telescope science images, which are patterns of diffracted starlight that can mimic the appearance of planets, complicating the detection of faint exoplanet signals. Traditional post-processing methods, operating primarily in the image intensity domain, do not integrate wavefront sensing data. These data, measured mainly for adaptive optics corrections, have been overlooked as a potential resource for post-processing, partly due to the challenge of the evolving nature of wavefront aberrations. In this paper, we present a differentiable rendering approach that leverages these wavefront sensing data to improve exoplanet detection. Our differentiable renderer models wave-based light propagation through a coronagraphic telescope system, allowing gradient-based optimization to significantly improve starlight subtraction and increase sensitivity to faint exoplanets. Simulation experiments based on the James Webb Space Telescope configuration demonstrate the effectiveness of our approach, achieving substantial improvements in contrast and planet detection limits. Our results showcase how the computational advancements enabled by differentiable rendering can revitalize previously underexploited wavefront data, opening new avenues for enhancing exoplanet imaging and characterization.
title Exoplanet Detection via Differentiable Rendering
topic Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
Computer Vision and Pattern Recognition
Image and Video Processing
url https://arxiv.org/abs/2501.01912