If you have any idea why the first three references are showing up as blank, I'm all ears... Many references are also out of date, but presumably the editors can take care of that (or punt back to us at a later date like journals always do...)
I would also argue that this approach has not been simulated vetted, as the "simulations" in Mertens' paper were extremely crude. But I understand if you don't want to say that, as it could be considered controversial.
This paragraph seems to come out of nowhere. Presumably it's about fitting foregrounds but the word foreground never shows up here. You also discuss the Mertens paper in detail later, so maybe this is just a relic paragraph that can be removed?
For example, \\citealt{Khoperskov2013MNRAS.428.2311K} investigated molecular cloud formation on the large-scale Galactic disk, finding {\\it Jesus, what did they find can you say it in a word or two?}
Period search in our 10-20 point lightcurves is a joke. 2013MNRAS.434.3423G for example argues that one needs 200 points for the period search to work https://t.co/0DKSadQb4g
It reads like "we just looked at the images and if the variability was" evident by eye - we classified the source as variable". This doesn't sound good enough, but I don't have specific suggestions on how to change it...
Should we have a plot in the Appendix illustrating the Eridanus~II problem? Or are we trying to avoid plotting the threshold in MAD-mag plots, because it looks ugly (has noticeable steps)? -- KS. AB: yes, we are avoiding it
\\LHG{Do you think it's worth emphasizing (here and possibly elsewhere) that the simulations weren't just variations in \\sig and \\om, but included 4 other parameters (plus HOD)? That's a lot of marginalization!}