Dazzle: Oversampled Image Reconstruction and Difference-Imaging Photometry for the Nancy Grace Roman Space Telescope

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Publicado en:arXiv.org (Dec 9, 2024), p. n/a
Autor principal: Albrow, Michael D
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Cornell University Library, arXiv.org
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Acceso en línea:Citation/Abstract
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022 |a 2331-8422 
035 |a 3143058004 
045 0 |b d20241209 
100 1 |a Albrow, Michael D 
245 1 |a Dazzle: Oversampled Image Reconstruction and Difference-Imaging Photometry for the Nancy Grace Roman Space Telescope 
260 |b Cornell University Library, arXiv.org  |c Dec 9, 2024 
513 |a Working Paper 
520 3 |a We present algorithms and software for constructing high-precision difference images to detect and measure transients, such as microlensing events, in crowded stellar fields using the Nancy Grace Roman Space Telescope. Our method generates difference images by subtracting an over-sampled reference, with iterative masking to address outlier pixels. We also provide an analytic correction for small dither offset errors. Microlensing event detection is achieved through a three-dimensional matched-filtering technique, optimized with Gaussian kernels to capture varying event durations, and verified through synthetic tests with high recovery rates. Transient photometry is performed via PSF fitting on difference images, using Nelder-Mead optimization for sub-pixel accuracy. The software, Dazzle, is available as an open-source Python package built on widely used libraries, offering accessible tools for the detection and characterization of transient phenomena in crowded fields. 
653 |a Microlenses 
653 |a Data analysis 
653 |a Algorithms 
653 |a Python 
653 |a Three dimensional analysis 
653 |a Transients (astronomy) 
653 |a Pixels 
653 |a Image reconstruction 
653 |a Photometry 
653 |a Image filters 
653 |a Software 
653 |a Space telescopes 
773 0 |t arXiv.org  |g (Dec 9, 2024), p. n/a 
786 0 |d ProQuest  |t Engineering Database 
856 4 1 |3 Citation/Abstract  |u https://www.proquest.com/docview/3143058004/abstract/embedded/6A8EOT78XXH2IG52?source=fedsrch 
856 4 0 |3 Full text outside of ProQuest  |u http://arxiv.org/abs/2412.06905