SIMBAD references

2020MNRAS.493.3854H - Mon. Not. R. Astron. Soc., 493, 3854-3865 (2020/April-2)

Comparison of galaxy spiral arm pitch angle measurements using manual and automated techniques.

HEWITT I.B. and TREUTHARDT P.

Abstract (from CDS):

The pitch angle (PA) of arms in spiral galaxies has been found to correlate with a number of important parameters that are normally time intensive and difficult to measure. Accurate PA measurements are therefore important in understanding the underlying physics of disc galaxies. We introduce a semi-automated method that improves upon a parallelized two-dimensional fast Fourier transform algorithm (P2DFFT) to estimate PA. Rather than directly inputting deprojected, star subtracted, and galaxy centred images into P2DFFT, our method (P2DFFT:TRACED) takes visually traced spiral arms from deprojected galaxy images as input. The tracings do not require extensive expertise to complete. This procedure ignores foreground stars, bulge and/or bar structures, and allows for better discrimination between arm and interarm regions, all of which reduce noise in the results. We compare P2DFFT:TRACED to other manual and automated methods of measuring PA using both simple barred and non-barred spiral galaxy models and a small sample of observed spiral galaxies with different representative morphologies. We find that P2DFFT:TRACED produces results that, in general, are more accurate and precise than the other tested methods and it strikes a balance between total automation and time-consuming manual input to give reliable PA measurements.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): methods: analytical - techniques: miscellaneous - software: data analysis - galaxies: fundamental parameters - galaxies: spiral - galaxies: structure

Simbad objects: 9

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2020.07.14-00:30:41

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