Bayesian model reconstruction based on astronomical spectral line observations.
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Updated
Nov 7, 2024 - Python
Bayesian model reconstruction based on astronomical spectral line observations.
Python library to create interactive 3D visualisations of astrophysical spectral line data.
Friendly user interface to estimate vsini, using high resolution spectra, based on Fourier's method.
Galaxy Line Emission & Absorption Modeling
Repository of line spectra estimators used in the published article "Real-time sinusoidal parameter estimation for damage growth monitoring during ultrasonic very high cycle fatigue tests".
Bayesian spectral decomposition and model fitting using Nested Sampling
Nested sampling of pyspeckit models with PyMultiNest.
Robishaw/Heiles SToKes IDL package to process single-dish spectropolarimetric radio astronomical data.
Deep learning for the automated spectral classification of supernovae
A Python Spectral Typing Suite
Labeled Latent Dirichlet Allocation model implementation for spectral line classification on ALMA Astronomy Datacubes
This is the start of a major spectroscopy absorption and emission data base. These are going to be all of my spectral and lab data files from all my experiments from my spectrometer prototypes from Hackaday.com
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