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Fig. 18

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Zoom-in on the evolution of segmentation results as a function of the classification threshold showing the filamentary structures estimated by UNet++ 10–3 in 160–171° (six top images) and 349–356° (six bottom images) regions of the Galactic plane. The original H2 column density image (top left in each group), the ground-truth input filament mask, and the corresponding segmented image at different thresholds (0.8, 0.5, 0.2, and the optimal threshold) are shown from top left to bottom right. The regions are 2° × 2° wide.

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