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We comment on arXiv:1112.1320 and point out that baryonic oscillations of thematter power spectrum, while predicted by theories that do not incorporatecollisionless cold dark matter, are strongly suppressed by the statisticalwindow function that is used to process finite-sized galaxy samples. We assertthat with present-day data sets, the slope of the matter power spectrum is amuch stronger indicator of a theory's validity. We also argue that MOND shouldnot be used as a strawman theory as it is not in general representative ofmodified gravity theories; some theories, notably our scalar-vector-tensorMOdified Gravity (MOG), offer much more successful predictions of cosmologicalobservations.

Comment on "The Real Problem with MOND" by Scott Dodelson, arXiv:1112.1320