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
Claculates the column density of interstellar molecular gas
Package to calculate 3D and 2D power spectra of galaxy and CIB cross-correlation.
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