Statistical detection of patterns in unidimensional distributions by continuous wavelet transforms
arXiv:1711.07820 · doi:10.1016/j.ascom.2018.04.004
Abstract
Objective detection of specific patterns in statistical distributions, like groupings or gaps or abrupt transitions between different subsets, is a task with a rich range of applications in astronomy: Milky Way stellar population analysis, investigations of the exoplanets diversity, Solar System minor bodies statistics, extragalactic studies, etc. We adapt the powerful technique of the wavelet transforms to this generalized task, making a strong emphasis on the assessment of the patterns detection significance. Among other things, our method also involves optimal minimum-noise wavelets and minimum-noise reconstruction of the distribution density function. Based on this development, we construct a self-closed algorithmic pipeline aimed to process statistical samples. It is currently applicable to single-dimensional distributions only, but it is flexible enough to undergo further generalizations and development.
Accepted by Astronomy & Computing; 23 pages, 5 figures; v3 contains optimized figures and have a reduced PDF size without loosing graphical quality; the software package available for download at http://sourceforge.net/projects/waveletstat/
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Cited by in corpus (5)
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- Fine-resolution analysis of exoplanetary distributions by wavelets: hints of an overshooting iceline accumulation
- Statistical detection of clumps and gaps in a random sample by continuous wavelet transforms: the 2D case