Ya, but they are still "dark" to us, even in our OWN GALAXY! This brings us right back to my earlier question of the meaning of 'dark' and whether it's dark because of our limited technology (we can't see every photon) or because it's "invisible".
Two points.
First: star counting does see "every photon", or enough of them to count stars very accurately. How do I know? Because stars live in the
disk of the galaxy. The disk has its own gravity that we can measure using a certain component of stellar velocity distributions. When we count the stars and gas in the
disk of the galaxy (The Astrophysical Journal 554 (20 June 2001): 1272–1281 et. seq.), then we measure vertical velocity dispersions to measure the
total mass of the disk (Astronomy and Astrophysics 329 (1998): 920–936), we're getting it right. Our technology is able to see everything it needs to see in the disk of the Milky Way. The disk is made out of stars and gas and we are perfectly competent at adding them up.
Meanwhile, the other component of the velocity (radial/tangential) tells us the mass of the Milky Way
halo. The halo has 4x the mass of the disk (measured gravitationally) but only a tiny, tiny fraction of the stars and gas. The halo is not something strange and far away; some of it is near Earth and as easy to see as the disk is, like Kapetyn's Star.
In other words: you're imagining a telescope error that explains dark matter observations. You have no evidence of such an error; you continue insisting on it in spite of evidence to the contrary; you can't describe what direction this error would have to have gone in. You're making it up out of thin air
without even knowing what you mean and without paying attention to data which might clear it up. You're not even calling it a "hypothesis", you're just assuming that it is the answer by default.
Second: I will help you construct a working baryonic dark matter hypothesis.
Go through the periodic table. That, plus black holes, plus neutron stars, is
everything that baryons can possibly do. Baryons can be hydrogen, they can be helium, carbon, lead, etc. They don't have some secret cabal of other, hard-to-see things they can be, do they? Unobtanium? Dilithium?
Now hypothesize: "The Milky way has a halo made of
known material X (either a chemical element, or neutron star/black hole material), distributed in N chunks of
masses M with probability Y(M), such that the integral (dM) of N M Y(M) is 5x10^11 solar masses." There, I have just written down
all possible baryonic dark matter models.
You want a baryons-as-dark-matter model to be true? OK, go ahead. Tell me X and tell me Y(M) for a model that you think might correctly describe
gravitational observations of the Milky Way.
OK, got one? Ready? If you can't do it alone, let me give you an example: say that X is "carbon" and Y(M) is "100% probability of being between 0.7 and 0.9 Ceres masses". There, that's a "rocks" dark matter hypothesis just for example. You could say "X is Earthlike composition (O, Si, Fe) and Y(M) is a powerlaw M^-3 extending down to M = 30amu (free neutral atoms) and up to M=10^27 kg (Jupters)". You cannot think of a baryons-as-dark-matter hypothesis which could not be described like this.
Got one? One of mine, or your own? OK. You're not going to like this, but:
a) What you just did was
curve fitting. You took some completely unknown parameter space ("We have no direct observations whatsoever of X or of Y(M) since we've never seen these baryons") and hand-picked a subset of it, not because it was super-physically-motivated, but because "any other choice would be ruled out already". Your insistence on "rocks" or "moons" is an informal curve-fit which you are tweaking to avoid a microlensing constraint. You cannot, for example, do a "controlled lab experiment" to show that Y(M) is M^-3. We just pick that number, call it a hypothesis, and evaluate that hypothesis. You know what? That's fine. Don't knock it when scientists do it, even if their hypothesis is different than yours. You can knock their hypothesis if it is ruled out by the data, or made irrelevant by the discovery of something else.
b) If your Y(M) extends to Moon-sized objects it is probably ruled out by microlensing. Sorry, that axes black holes and neutron stars too.
c) If your Y(M) is only in superheavy objects ("loose" SMBHs) then it is ruled out by Galactic disk stability.
d) If your X is anything other than H+He, it is ruled out by the low heavy-metal content of the Galaxy.
e) If your N is very large---as it will be if you're desperately subdividing your moons into pebbles, or (worse) into diffuse gas clouds, to escape the microlensing bounds---then your dark matter is colliding like crazy and can't possibly remain on the halo orbits where the non-disky gravity is coming from.
f) In any case, no matter what your X is, if it's found on the Periodic Table then it is inconsistent with the CMB acoustics.
g) In any case, no matter what your X is, if it's found on the Periodic Table then it is inconsistent with the BBN.
There you go, MM. We have considered, in a standard scientific way (present hypothesis, evaluate observables, compare to data) the baryonic dark matter hypotheses. I believe we have discarded
all possible baryonic dark matter hypotheses via observations a-e, and triply discarded them if we include f and g(which we do).
The possible exception would be a incredibly numerous sort of sub-lunar-mass-black-hole-population---let's call it the "X=neutronium, M < 10^22 kg" hypothesis, not that you have ever suggested such a thing. Maybe not ruled out by data. X and Y picked out of thin air to avoid lensing bounds. Yep, that's crazy-arbitrary curve fitting in the service of avoiding SUSY. How do you like it? Quite frankly, physicists would be considered this incredibly
more exotic and crazy-speculative (how the heck would Nature make such a thing?) than SUSY, axions, and walking technicolor put together.
We didn't reject baryonic dark matter because we love inventing new particles. We rejected it because Nature rejected it, and has given us plenty of evidence that she rejected it. Nature has not YET given us evidence for exactly what she did instead. But we're looking.