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doi: 10.5281/zenodo.48073
This dataset holds all of the cross-correlation functions (CCFs) generated in Gullikson et al. (2016). (update link when I have it). The CCFs are stored as HDF5 files, and are split into 2 GB chunks such that they can go here on zenodo. You will likely want to combine them all together for each instrument. The filenames have the form 'INSTRUMENT_ccfs_n.h5' where n is an integer. This dataset also holds the MCMC samples for the primary star mass, companion mass, and system age for all of the stars listed in Table 1 of the paper. This is again stored as an HDF5 file. Finally, the dataset contains MCMC samples from the posterior distributions that result from fitting the data to a variety of parametric distributions. They files are generated by the pymultinest code, and the samples can be recovered with the same code (See RealData.ipynb notebook in the github repository for details: https://github.com/kgullikson88/BinaryInference).
| 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 |
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