ratfink said:
Let me put this another way! Instead of just quoting ‘cosmological tests’ it would help if you stated what they are.
The abundances of light elements, the cosmic microwave background, the formation of large scale structure, star formation rate vs. redshift, the Soltan argument, evolution of morphology with redshift, supernova time dilation, GRB time dilation, and much more, I'm sure. The CMB, abundances, and large scale structure all constitute multiple tests of BB predictions.
However the HUDF came along and now the tolman test comes out very
firmly in favour of a static universe.
Eric Lerner is a well-known crank. Those results come about from one of the effects I mentioned above -- the evolution of star formation with redshift. High-z galaxies are nothing like low-z ones, so as you've suggested, the test is not very useful. It may have some value at low redshifts and where galaxies haven't evolved much, but it's still not a very strong test.
CMB? Didn’t you tell me that the axis of evil is still there on the latest data?
The "axis of evil" is a sign of possible contamination in the data at low multipoles. The vast majority of the information in the CMB lies at high multipoles, where the standard model fits the data to very high precision. The CMB is a
very dramatic test of mainstream theory -- it comes as no surprise to me that most of the laymen advocating steady state models don't understand the WMAP results.
Furthermore, the horizon problem in the CMB is only solved by inflation and that has no experimental verification whatsoever!
Wrong again. Inflation is actually doing quite well lately. The universe has continued to be consistent with flat, now to a precision of a few percent. Furthermore, the fluctuations in both the CMB and large scale structure (see the "genus" test) have been shown to be gaussian, another prediction of inflation. Finally, the WMAP measurements indicate a spectral slope just slightly deviant from unity, just as predicted by inflation.