I think the cosmology department needs a *fact* check for many of the claims commonly presented to the public

Here is another report on this rate of expansion problem,
Rethinking cosmology: Universe expansion may not be uniform (Update) The report stated, "Astronomers have assumed for decades that the Universe is expanding at the same rate in all directions. A new study based on data from ESA's XMM-Newton, NASA's Chandra and the German-led ROSAT X-ray observatories suggests this key premise of cosmology might be wrong... Widely accepted as a consequence of well-established fundamental physics, the hypothesis has been supported by observations of the cosmic microwave background (CMB). A direct remnant of the Big Bang, the CMB reflects the state of the Universe as it was in its infancy, at only 380 000 years of age. The CMB's uniform distribution in the sky suggests that in those early days the Universe must have been expanding rapidly and at the same rate in all directions. In today's Universe, however, this may no longer be true. "Together with colleagues from the University of Bonn and Harvard University, we looked at the behaviour of over 800 galaxy clusters in the present Universe," says Konstantinos. "If the isotropy hypothesis was correct, the properties of the clusters would be uniform across the sky. But we actually saw significant differences."
Note, the origin of the CMB and redshift used to explain the evolution of the cosmic fireball that created the universe, the uniform or nearly uniform temperature observed in the CMBR today is interpreted to mean *must have been expanding rapidly and at the same rate in all directions. In today's Universe, however, this may no longer be true."
What? This should raise questions here about the various rates of expansion used in cosmology and how these different expansion rates are confirmed. The CMBR uniformity today is considered to represent a redshift where z=1000 or more based upon the expansion rate and size of the universe. However, galaxies with high redshifts are spectral measurements, the CMBR redshift is not, it is an extrapolation dependent on the rate of expansion, this seems to be different now. This is not the same as spectra obtained for high redshift galaxies, but a model dependent interpretation for the redshift or z. For example, ‘Characterizing the Environment Around The Most Distant Known Galaxy’,
https://ui.adsabs.harvard.edu/abs/2019hst..prop15977O/abstract, “The discovery of the very luminous galaxy GN-z11 at only 400 Myr after the Big Bang in the GOODS-North field with an HST grism spectroscopic redshift of z=11.1+/-0.1 presents a real puzzle for early Universe science. Its detection raises significant questions about our understanding of early galaxy formation…”
I note a difference here. *
spectroscopic redshift* vs. the model dependent interpretation of original temperature some 3000K vs. near 3K today for the CMBR where z=1000 or more.
The latest report on expansion rate published, now we read that the rate of expansion used to calculate the z number for the CMBR redshift, the expansion rate may not be uniform and changed. Seems like z=1000 or more may not be confirmed, certainly not confirmed using the same method as GN-z11 redshift.