It does this by saying that star images on a 50 minute exposure would be fuzzy, but a transient lasting a fraction of a second would be sharp. Yes, but so would a plate anomaly. So Handley and Blair's criticism is not refuted; it remains the case that these anomalies are overwhelmingly more likely to be flaws in the plate rather than alien satellites. To quote the PASP paper:
Note as well that any transient longer than a second or so would show a line, not a dot - and all these lines would be precisely aligned with the rotation of the telescope as it compensates for Earth's rotation. But there Is no evidence for such extended lines. So somehow all these NTA satellites are specifically configured to only glint for a fraction of a second. These satellites must be very strange shapes, too; they have tiny reflective surfaces that are only visible for a fraction of a second, but rarely rotate so that the glints are visible at regularly spaced intervals. One imagines a large black sphere with a tiny hand mirror glued to the side.
Any glint from a real object that lasted 0.5 seconds (the figure suggested in the paper) would be reduced in apparent brightness by a factor of 6000 (0.5 seconds over 50 minutes). This would result in a decrease in the apparent brightness on the plate by a factor of 10.4 magnitudes, not 9 magnitudes as stated in the paper.
As well as these incredibly dim anomalies that last a fraction of a second, we should also see a selection of longer transients, 1 or more seconds in length, which would show an easily recognisable signature of elongation parallel to the Earth's rotation. But we don't.
Not to mention glints from satellites in much closer orbits - if you want to observe events on the surface of a planet, a network of spy satellites in low Earth orbit would give a much clearer view than a grid thirty-five thousand kilometres away.