Influence of magnetic cycles on stellar prominences and their mass loss rates (dataset)

Data used for figures in the paper.

For the prominence mass (prom_mass), mass loss (prom_mdot), and angular momentum loss (prom_jdot) there are three files, one for each resolution used in the plots. The first column in each is rotation number, and the second column in the corresponding value for each dataset.
For the wind mass loss (wind_mdot) and angular momentum loss (wind_jdot) there are three files, one for each resolution, in the same format as prominence values.
For the prom_locs files, these are the radius (solar radii), latitude (degrees from equator) and mass (log10) of the prominence locations, with separate files for the two resolutions discussed, and around cyyle minimum and cycle maximum.
All files are in csv format.