
MESA inlists used for modelling zero-metallicity stars in "Spectral Evolution of Rotating Population III Stars" (2025). These were run using version r24.08.1 of MESA and version 24.7.1 of the MESA SDK. Details on the inlists are described in the README.txt file.
| 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). | 0 | |
| 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 |
