A multi-scale filament extraction method: getfilaments

TL;DR

This paper introduces getfilaments, a multi-scale filament extraction method that improves the robustness of source detection in filamentary backgrounds by effectively separating filaments from sources and noise in Herschel far-infrared images.

Contribution

The paper presents a novel filament extraction technique, getfilaments, that enhances source extraction accuracy by subtracting filaments during detection, improving analysis of star-forming regions.

Findings

Enhanced filament detection accuracy in Herschel images.

Reduced contamination of source catalogs by filamentary structures.

Provided clean filament images for further analysis.

Abstract

Far-infrared imaging surveys of Galactic star-forming regions with Herschel have shown that a substantial part of the cold interstellar medium appears as a fascinating web of omnipresent filamentary structures. This highly anisotropic ingredient of the interstellar material further complicates the difficult problem of the systematic detection and measurement of dense cores in the strongly variable but (relatively) isotropic backgrounds. Observational evidence that stars form in dense filaments creates severe problems for automated source extraction methods that must reliably distinguish sources not only from fluctuating backgrounds and noise, but also from the filamentary structures. A previous paper presented the multi-scale, multi-wavelength source extraction method getsources based on a fine spatial scale decomposition and filtering of irrelevant scales from images. In this paper, a multi-scale, multi-wavelength filament extraction method getfilaments is presented that solves this problem, substantially improving the robustness of source extraction with getsources in filamentary backgrounds. The main difference is that the filaments extracted by getfilaments are now subtracted by getsources from detection images during source extraction, greatly reducing the chances of contaminating catalogs with spurious sources. The intimate physical relationship between forming stars and filaments seen in Herschel observations demands that accurate filament extraction methods must remove the contribution of sources and that accurate source extraction methods must be able to remove underlying filamentary structures. Source extraction with getsources now provides researchers also with clean images of filaments, free of sources, noise, and isotropic backgrounds.