Template matching method for the analysis of interstellar cloud structure
M. Juvela (1, 2) ((1) University of Helsinki (2) Institut UTINAM,, CNRS UMR 6213, OSU THETA, Universite de Bourgogne Franche-Comte)

TL;DR
This paper introduces a fast, robust template-matching method for analyzing filamentary and other structures in interstellar medium maps, demonstrating its effectiveness compared to existing techniques like RHT.
Contribution
The paper presents a novel template-matching algorithm for map analysis that is more robust and versatile than previous methods, capable of identifying various structures at different scales.
Findings
TM method is comparable to RHT in performance
TM is more robust to input parameter variations
TM can identify diverse structures at multiple scales
Abstract
The structure of interstellar medium can be characterised at large scales in terms of its global statistics (e.g. power spectra) and at small scales by the properties of individual cores. Interest has been increasing in structures at intermediate scales, resulting in a number of methods being developed for the analysis of filamentary structures. We describe the application of the generic template-matching (TM) method to the analysis of maps. Our aim is to show that it provides a fast and still relatively robust way to identify elongated structures or other image features. We present the implementation of a TM algorithm for map analysis. The results are compared against rolling Hough transform (RHT), one of the methods previously used to identify filamentary structures. We illustrate the method by applying it to Herschel surface brightness data. The performance of the TM method is found…
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