Dense Basis SED fitting
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Updated
Dec 31, 2025 - 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.
Package to calculate 3D and 2D power spectra of galaxy and CIB cross-correlation.
This a repo for the Bousso and Leichenauer model of Star Formation
Claculates the column density of interstellar molecular gas
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