Extended Data Fig. 3: The completeness distribution of the WD populations of M13 and M3.
From: Slowly cooling white dwarfs in M13 from stable hydrogen burning
a, Completeness parameter as a function of the F275W magnitude and colour-coded in terms of the distance from the cluster centre (see colour bars) for each WD detected in M13. b, The same for M3. The mean error (1 s.e.m.) is also reported.
