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This software quickly computes magnitudes and spectra of rotating stellar models. The models incorporate Roche mass distribution (where all mass is at the center of the star), solid body rotation, and collinearity of effective gravity and energy flux. The 2020 Astrophysical Journal article by Lipatov and Brandt refers to this version of the software. Please see README.md in the enclosed ZIP file for detailed installation and usage instructions. README.md is a Markdown file, so that it is most easily viewed with a browser or an editor that understands the Markdown language. For a live version of the software, please visit the following website: https://github.com/mlipatov/paint_atmospheres
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 1 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
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