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Analysis

This article presents a research paper on modeling disk-galaxy rotation curves using a specific mathematical approach (Ansatz). It focuses on fitting the model to observational data (SPARC), employing Bayesian inference for parameter estimation, and assessing the identifiability of the model's parameters. The research likely contributes to understanding the dynamics of galaxies and the distribution of dark matter.
Reference

The article is a scientific research paper, so there are no direct quotes suitable for this field.