neat

Nebular Empirical Analysis Tool

Description

NEAT analyses lists of emission line fluxes measured from the spectra of photoionised nebulae such as planetary nebulae and HII regions. It determines the extinction, and then adopts a three zone model to determine temperatures, densities, and ionic and total abundances, from collisionally excited lines and recombination lines. It calculates uncertainties if required, using a Monte Carlo technique.

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Homepage

https://github.com/rwesson/NEAT


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