I am trying to plot the distribution of CCSNe in the Galaxy and the LMC+SMC using the Adams et al. 2013 data in /data/stellar/. Below is a minimal example. I find duplicate values for the distance (e.g. 60 kpc) and a non-monotonous array for the distances. After 62.5 kpc the distances jump back to 53.75 kpc.
from asteria.stellardist import StellarDensity
distribtion = StellarDensity("path/to/asteria/data/stellar/sn_radial_distrib_adams.fits", add_LMC=True, add_SMC=True)
dist = distribtion.dist
cdf = distribtion.cdf
plt.plot(dist, cdf)
plt.xlim(50,66) # zoom in on the jump
plt.ylim(0.97,1)
plt.xlabel("distance")
plt.ylabel("cdf")
I also noticed that the paper does not show any probability beyond the edge of the Milky Way. How is the LMC+SMC data provided in ASTERIA?