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

Abstract 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 oversampled reference image, with iterative masking to address outlier pixels. We also provide an analytic correction for small dither offset errors. Microlensing 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 subpixel 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.

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Publication Details

Journal
The Astronomical Journal
Published
2025-05-08
DOI
https://doi.org/10.3847/1538-3881/adc9a1
Primary Topic
Adaptive optics and wavefront sensing
Type
article
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article

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

Michael D. Albrow
The Astronomical Journal
Adaptive optics and wavefront sensing
article

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

Michael D. Albrow
article en

Abstract

Abstract 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 oversampled reference image, with iterative masking to address outlier pixels. We also provide an analytic correction for small dither offset errors. Microlensing 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 subpixel 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.

The Astronomical JournalVol. 169(6)
Openalex Percentile: Top 93%
Adaptive optics and wavefront sensing
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Dazzle: Oversampled Image Reconstruction and Difference-imaging Photometry for the Nancy Grace Roman Space Telescope — Michael D. Albrow · The Astronomical Journal (2025) | TGRS Research Map | TGRS