Dense Basis SED fitting
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Updated
Oct 9, 2024 - Jupyter Notebook
Dense Basis SED fitting
Gaussian process based implementation for galaxy star formation histories with custom kernels
Constraining the delay time distribution of Type-Ia supernovae in clusters with a MCMC Bayesian method and the spectral-population synthesis code Pégase.3.
This a repo for the Bousso and Leichenauer model of Star Formation
Cross-Correlation Analysis of DESI Legacy Imaging Surveys and Planck Cosmic Infrared Background
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