Optimising and comparing source extraction tools using objective segmentation quality criteria
Caroline Haigh (1), Nushkia Chamba (2,3), Aku Venhola (4,5), Reynier, Peletier (4), Lars Doorenbos (1), Matthew Watkins (1), Michael H. F., Wilkinson (1) ((1) Bernoulli Institute for Mathematics, Computer Science and, Artificial Intelligence, Groningen, Netherlands

TL;DR
This paper compares and optimizes astronomical source extraction tools using objective segmentation quality criteria, highlighting their strengths and limitations in detecting faint and diffuse sources.
Contribution
It introduces an automated parameter optimization method using Bayesian techniques and evaluates four source extraction tools on simulated and real data.
Findings
MTObjects achieves the highest overall scores.
NoiseChisel and MTObjects detect faint outskirts better.
No tool balances speed and accuracy for large-scale use.
Abstract
With the growth of the scale, depth, and resolution of astronomical imaging surveys, there is an increased need for highly accurate automated detection and extraction of astronomical sources from images. This also means there is a need for objective quality criteria, and automated methods to optimise parameter settings for these software tools. We present a comparison of several tools which have been developed to perform this task: namely SExtractor, ProFound, NoiseChisel, and MTObjects. In particular, we focus on evaluating performance in situations which present challenges for detection -- for example, faint and diffuse galaxies; extended structures, such as streams; and objects close to bright sources. Furthermore, we develop an automated method to optimise the parameters for the above tools. We present four different objective segmentation quality measures, based on precision,…
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