Extended Data Fig. 1: Parametric profile fitting results for 23 FRB host galaxies using the AutoProf package.
From: Selection bias obfuscates the discovery of fast radio burst sources
For each galaxy, we show three images - (left) r-band image of the host, (center) best-fitted galaxy model, and (right) resultant residual. The numbers in the top left of each r-band image correspond to the host number and the estimated inclination angle (in degrees, quoted in parentheses), as shown in Table 1. The X-axis and Y-axis of all plots represent right ascension and declination, respectively.
