Another loop around the Great Circle of Repetition. Yes, we're going to keep finding baryonic matter until it adds up to 4% of the total mass of the Universe. The BBN and CMB data tell us that the total is 4%, but telescopes have only directly located 2-3%, mostly in the ICM. We're NOT going to find matter that adds up to 25%---it is utterly impossible to hide any known form of matter (not gas, plasma, dust, rocks, planetoids, planets, compact stars, dwarf stars, normal stars, big stars, black holes, IMBHs, or SMBHs) in galaxies or clusters in those amounts.
Again, this is the Nth time I've posted exactly this. But here you're back with another mindless post of the same hidden-baryonic-dark-matter idea. Did you forget how we ruled that idea out? What's next? Tomorrow you'll be claiming it's all rocks (again)? The next day you'll be claiming it's Perratt's magnetic forces (again)?
As for the paper you cited: sure, there are hard-to-find subdwarf galaxies. We've known for decades that they ought to exist and we've been looking for them very hard; there are a dozen or so of them. (I could tell you why they are so interesting, but I doubt you will understand.) We expect that there are 100+ smaller ones as well. These newly-found satellites probably weigh something in the ballpark of 10^7 solar masses, or 0.003% of the mass of the Milky Way. I suspect that you, MM, will fail to appreciate that number, but others will.