A multi-scale filament extraction method: getfilaments
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. Although getsources performed
very well in benchmarks, strong unresolved filamentary structures caused difficulties for
reliable source extraction. 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 getfilaments method shares its
general philosophy and approach with getsources, and it is an integral
part of the source extraction code. 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 the new version of getsources provides researchers not
only with the catalogs of sources, but also with clean images of filamentary structures,
free of sources, noise, and isotropic backgrounds.
Origin : Publication funded by an institution
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