{ "id": "2205.00675", "version": "v1", "published": "2022-05-02T06:30:07.000Z", "updated": "2022-05-02T06:30:07.000Z", "title": "Using EAGLE simulations to study the effect of observational constraints on the determination of HI asymmetries in galaxies", "authors": [ "P. V. Bilimogga", "K. A. Oman", "M. A. W. Verheijen", "J. M. van der Hulst" ], "comment": "19 pages, 12 figures and 2 appendices. Accepted for publication in the Monthly Notices of the Royal Astronomical Soceity", "categories": [ "astro-ph.GA" ], "abstract": "We investigate the effect of observational constraints such as signal-to-noise, resolution and column density level on the HI morphological asymmetry ($\\mathrm{A}_\\mathrm{mod}$) and the effect of noise on the HI global profile ($\\mathrm{A}_\\mathrm{flux}$) asymmetry indices. Using mock galaxies from the EAGLE simulations we find an optimal combination of the observational constraints that are required for robust measurement of the $\\mathrm{A}_\\mathrm{mod}$ value of a galaxy: a column density threshold of $5\\times10^{19}cm^{-2}$ or lower at a minimal signal-to-noise of 3 and a galaxy resolved with at least 11 beams. We also use mock galaxies to investigate the effect of noise on the $\\mathrm{A}_\\mathrm{flux}$ values and conclude that a global profile with signal-to-noise ratio greater than 5.5 is required to achieve a robust measurement of asymmetry. We investigate the relation between $\\mathrm{A}_\\mathrm{mod}$ and $\\mathrm{A}_\\mathrm{flux}$ indices and find them to be uncorrelated which implies that $\\mathrm{A}_\\mathrm{flux}$ values cannot be used to predict morphological asymmetries in galaxies.", "revisions": [ { "version": "v1", "updated": "2022-05-02T06:30:07.000Z" } ], "analyses": { "keywords": [ "observational constraints", "eagle simulations", "hi asymmetries", "robust measurement", "mock galaxies" ], "note": { "typesetting": "TeX", "pages": 19, "language": "en", "license": "arXiv", "status": "editable" } } }