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Sutra: An Integrated Framework for Identification and Characterization of Filaments in the Interstellar Medium

  • Authors: Shivam Kumaran, Ushasi Bhowmick, Vipin Kumar, Manish Chauhan, Munn Vinayak Shukla, Mehul R. Pandya

Shivam Kumaran et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 6.

Schematic illustration of crest detection and physics-guided skeleton refinement in Sutra. (a) Input CD map. (b) Corresponding crest-likelihood map Pcrest(xy) produced by the trained U-Net ridge detection model, where high-probability values trace filament spines. (c) Binary skeleton obtained after thresholding the crest-likelihood map and medial axis refinement. Beam-sized segments (numbered) are evaluated individually through radial profile analysis. The bottom panels show examples of (d) a “good” beam segment (green marker) yielding a low reduced χ2 and (e) shows an example of a rejected beam (red marker), due to a poor Plummer fit, on the left side and an immediate dip (≤ beam size) due to a nearby filament on the right side. The solid black line (panel (c)) shows the final skeleton.

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