Extended Data Fig. 1: Surface brightness and ionization do not vary significantly with azimuthal angle.
From: An emission map of the disk–circumgalactic medium transition in starburst IRAS 08339+6517
Points are colored as Fig. 2. The large points represent spaxels that have been binned radially for each KCWI pointing (10 radial bins per pointing) and correspond to the CGM points plotted in Fig. 3. Error bars on the binned data points are 1σ errors on the mean. Note that the y-axis ranges differ for each panel to emphasize the azimuthal variations and so the power law slope differences between lines are not reflected here.
