Galaxy Line Emission & Absorption Modeling
Basically a class which parses the NIST Atomic Spectra Database and saves the data to a dictionary on HDD. You can pass an matplotlib.axis, and the emissions lines will be plotted with an optional normalization factor.
Automated Line Fitting Algorithm
Empirical analysis of ionised nebulae, with uncertainty propagation
A Python package for calculating emission line flux from stellar spectra, providing automated analysis of Far Ultraviolet emissions for exoplanetary and stellar research.
Code to fit measured line fluxes to a grid of photoionization models based on BPASS
Assessment of sky-subtraction effects on DESI emission-line measurements, with a focus on narrow-line AGN and [OI] sky residual contamination.
Initial reproduction of radial dust-attenuation scaling relations in MaNGA, focusing on E(B-V)_gas and its correlation with N2S2, O3O2, and sigma_Ha across radial bins.
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