I'd like to keep this thread here in the GR forum, but avoid ANY discussion of other websites, personalities, etc, and stick strictly to the GR relevant issues.
There have been quite a few papers written about the apparent superluminal velocity of galaxies. One of the papers that explains many of the common misconceptions is the Lineweaver & Davis paper:
http://arxiv.org/abs/astro-ph/0310808
You can check out it's publication history at
http://publish.csiro.au/paper/AS03040.htm
to see where it was originally published. (Publications of the Astronomical Society of Australia 21(1) 97 - 109 ).
While the Lineweaver and Davis paper is pretty good, there are a few points that one might wish it did make which it does not make. The first point is that there is no truly general, coordinate independent notion of the relative velocity of two distant objects in GR, including distant galaxies.
For a reference for this point, see
http://math.ucr.edu/home/baez/einstein/node2.html
publication history at:
http://scitation.aip.org/getabs/servlet/GetabsServlet?prog=normal&id=AJPIAS000073000007000644000001&idtype=cvips&gifs=yes
( American Journal of Physics -- July 2005 -- Volume 73, Issue 7, pp. 644-652)
In special relativity, we cannot talk about absolute velocities, but only relative velocities. For example, we cannot sensibly ask if a particle is at rest, only whether it is at rest relative to another. The reason is that in this theory, velocities are described as vectors in 4-dimensional spacetime. Switching to a different inertial coordinate system can change which way these vectors point relative to our coordinate axes, but not whether two of them point the same way.
In general relativity, we cannot even talk about relative velocities, except for two particles at the same point of spacetime -- that is, at the same place at the same instant. The reason is that in general relativity, we take very seriously the notion that a vector is a little arrow sitting at a particular point in spacetime. To compare vectors at different points of spacetime, we must carry one over to the other. The process of carrying a vector along a path without turning or stretching it is called `parallel transport'. When spacetime is curved, the result of parallel transport from one point to another depends on the path taken! In fact, this is the very definition of what it means for spacetime to be curved. Thus it is ambiguous to ask whether two particles have the same velocity vector unless they are at the same point of spacetime.
Thus while cosmologists have a standardized and well-defined meaning for the 'velocity of distant galaxies", their definition is coordinate dependent, and they frequently don't point this fact out. A related point is that the cosmologists standard definitions, while standard in the field, aren't very SR friendly.
For some related points see
http://www.astro.ucla.edu/~wright/cosmology_faq.html#FTL
(Which is not peer reviewed in and of itself as far as I know, though Ned Wright is a recognized authority and the author of many peer reviewed papers).
Can objects move away from us faster than the speed of light?
Again, this is a question that depends on which of the many distance definitions one uses. However, if we assume that the distance of an object at time t is the distance from our position at time t to the object's position at time t measured by a set of observers moving with the expansion of the Universe, and all making their observations when they see the Universe as having age t, then the velocity (change in D per change in t) can definitely be larger than the speed of light. This is not a contradiction of special relativity because this distance is not the same as the spatial distance used in SR, and the age of the Universe is not the same as the time used in SR. In the special case of the empty Universe, where one can show the model in both special relativistic and cosmological coordinates, the velocity defined by change in cosmological distance per unit cosmic time is given by v = c ln(1+z), where z is the redshift, which clearly goes to infinity as the redshift goes to infinity, and is larger than c for z > 1.718. For the critical density Universe, this velocity is given by v = 2c[1-(1+z)-0.5] which is larger than c for z > 3 .
Ned Wright is much more "up front" about the issue of "many distances", a point which is sometimes unfortunately glossed over.