Peter,
Thinking more about the additional effects contributing to galaxy cluster lensing, as you mentioned, I recalled seeing the Nature News article back in June, Galaxy clusters caught in motion, clearly describing the recent identification of the kSZ effect. That had been my first exposure to either the tSZ of kSZ effect.
Interestingly, I commented back then, speculating that the SZ effects should apply not only to CMB photons but all others as well, likely contributing to weak lensing effects produced by galaxy clusters that are now attributed only to gravitational effects. I further speculated that the result may be the overestimation of the total galaxy cluster mass necessary to produce the identified weak lensing effects. This then would at a minimum result in the overestimation of dark matter present within galaxy clusters.
My assertion is that the hypothesized enormous amounts of galactic dark matter have been misconceived, and that huge galactic DM halos do not actually exist.
That would not necessarily preclude the existence of dark matter to explain observed galaxy cluster lensing, or its inference (however that's accomplished) as the structural backbone of the 'cosmic web'.
I strongly suspect that, at large scales, no enormous dark matter halos envelop galaxies. I'm also beginning to suspect that, at very large scales, much of the effects attributed to dark matter in and among galaxy clusters may be the product of ICM and amorphous plasmas, as I think you suggest.
Best wishes on your work (although I suggest you focus on galaxy clusters & above :-) Jim