Image Details
Caption: Figure 9.
Polarization spectra computed over constant ﹩{N}_{{{\rm{H}}}_{2}}﹩ distributions for all of the data (left), the near regime smoothed to 0.052 pc (middle), and the far regime smoothed to 0.32 pc (right). The blue spectra are the median p values of the 1000 samples. The gray lines show the p for each of the 1000 trials. The inset histograms show the distribution of ﹩{N}_{{{\rm{H}}}_{2}}﹩ every band is fixed to. The pink data points are the same as the common resolution data medians reported in Figure 6.
© 2026. The Author(s). Published by the American Astronomical Society.