  A pileup near 1~AU in the semimajor axis distribution of giant exoplanets has
been visually identified using log-spaced distribution plots. Here we propose
that looking for features in a log-spaced semimajor axis distribution of giant
planets is problematic. We use the Bayesian Blocks algorithm to analyze the
linear-spaced semimajor axis distribution, and find that the apparent pileup is
not significant.
