Rescuing JWST's interferometer with end-to-end differentiable forwards models (Conference Presentation)
Abstract
Non-linear detector effects severely limit JWST’s interferometric performance, compromising the stability required for AMI calibration. AMIGO offers a different solution: a fully differentiable forward model spanning the astrophysical source, optical propagation, and non-linear detector charge migration. By predicting unprocessed detector frames directly, AMIGO avoids the precision limits imposed by the JWST reduction pipeline and incorporates detector physics within the inference process itself. Recent calibration observations have further refined the model, leading to improved visibility precision and stronger detections inside the diffraction limit. This talk will present AMIGO’s current capabilities, detections, and discuss its broader implications for next-generation precision astronomy.
Authors 11
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Leiden Univ. (Netherlands)
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Macquarie Univ. (Australia)
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The Univ. of Sydney (Australia)
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The Univ. of Sydney (Australia)
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Affiliation as printed
Univ. of Victoria (Canada)
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Herzberg Institute of Astrophysics · University of Victoria
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NRC-Herzberg Astronomy & Astrophysics (Canada)
Univ. of Victoria (Canada)
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Affiliation as printed
Macquarie Univ. (Australia)
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Space Telescope Science Institute
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Space Telescope Science Institute (United States)
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Affiliation as printed
European Southern Observatory (Germany)
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Space Telescope Science Institute
Affiliation as printed
Space Telescope Science Institute (United States)
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Space Telescope Science Institute
Affiliation as printed
Space Telescope Science Institute (United States)
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