This project from the series of "Statistical and Computational Methods in Physics" is a simple image processing project that uses a “Discrete Fourier transform” (DFT) on a collection of fake simple star-cluster images.
This project from the series of "Statistical and Computational Methods in Physics" is a simple image processing project that uses a maximum likelihood technique on a collection of fake simple star-cluster images.
Analysis of NGC-104 globular star cluster.
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