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ChiantiPy is a Python interface to the CHIANTI atomic database for astrophysical spectroscopy. The CHIANTI atomic database for astrophysical spectroscopy provides the information necessary to calculate the emission spectrum from hot plasmas. ChiantiPy provides several top-level classes to access the database and calculate continuum and emission line intensities.

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2010-12-10 07:08 Back to release list
0.3

Esta versão adiciona a classe mspectrum, que permite aos usuários utilizar múltiplos núcleos locais para cálculos espectrais que pode ser demorado. Além disso, há inúmeras correções de bugs.
This release adds the mspectrum class, which allows users to use multiple local CPU cores for spectral calculations that can be time consuming. In addition, there are numerous bugfixes.

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