Optimizing Convolution Direction and Template Selection for Difference Image Analysis

Abstract Difference image analysis (DIA) is a powerful tool for studying time-variable phenomena, and has been used by many time-domain surveys. Most DIA algorithms involve matching the spatially varying point-spread function shape between science and template images, and then convolving that shape in one image to match the other. The wrong choice of which image to convolve can introduce one of the largest sources of artifacts in the final difference image. We introduce a quantitative metric to determine the optimal convolution direction that depends not only on the sharpness of the images measured by their FWHM, but also on their exposure depths. With this metric, the optimal convolution direction can be determined a priori, depending only on the FWHM and depth of the images. This not only simplifies the process, but also makes it more robust and less prone to creating suboptimal difference images due to the wrong choice of the convolution direction. As an additional benefit, for a large set of images, we define a Figure-of-Merit based on this metric, which allows us to rank a list of images and determine the ones best suited to be used as templates, thus streamlining and automating the data reduction process.

Authors

Publication Details

Journal
The Astrophysical Journal Supplement Series
Published
2025-09-01
DOI
https://doi.org/10.3847/1538-4365/adf05b
Primary Topic
Infrared Target Detection Methodologies
Type
article
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article

Optimizing Convolution Direction and Template Selection for Difference Image Analysis

Qinan Wang, R. J. Foley, C. D. Kilpatrick, A. Rest et al.
The Astrophysical Journal Supplement Series
Infrared Target Detection Methodologies
article

Optimizing Convolution Direction and Template Selection for Difference Image Analysis

Qinan Wang, R. J. Foley, C. D. Kilpatrick, A. Rest, Jacob E. Jencson, Anthony L. Piro, William P. Blair, D. A. Coulter, C. Rojas-Bravo, Rodrigo Angulo, Xiaolong Li
article en

Abstract

Abstract Difference image analysis (DIA) is a powerful tool for studying time-variable phenomena, and has been used by many time-domain surveys. Most DIA algorithms involve matching the spatially varying point-spread function shape between science and template images, and then convolving that shape in one image to match the other. The wrong choice of which image to convolve can introduce one of the largest sources of artifacts in the final difference image. We introduce a quantitative metric to determine the optimal convolution direction that depends not only on the sharpness of the images measured by their FWHM, but also on their exposure depths. With this metric, the optimal convolution direction can be determined a priori, depending only on the FWHM and depth of the images. This not only simplifies the process, but also makes it more robust and less prone to creating suboptimal difference images due to the wrong choice of the convolution direction. As an additional benefit, for a large set of images, we define a Figure-of-Merit based on this metric, which allows us to rank a list of images and determine the ones best suited to be used as templates, thus streamlining and automating the data reduction process.

The Astrophysical Journal Supplement SeriesVol. 280(1)
Openalex Percentile: Top 69%
Infrared Target Detection Methodologies
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Optimizing Convolution Direction and Template Selection for Difference Image Analysis — Qinan Wang, R. J. Foley, et al. · The Astrophysical Journal Supplement Series (2025) | TGRS Research Map | TGRS