May I also bring this up
http://arxiv.org/abs/0801.4380
for the laymen among us:
VII. CONCLUSIONS
In this paper, we have measured the cross-correlation
between the CMB and a large range of probes of the
density in a consistent way, and have calculated their
covariance taking into account their overlapping sky cov-
erage and redshift distributions. While individual mea-
surements vary somewhat depending on how the data are
cleaned and how the covariance is calculated, the overall
significance of the detection of cross-correlations is at the
∼4 5 level.
This means we looked at a hell of a lot of stuff that other people have done, loads of different ways of "looking" at the universe, and found that they pretty much all tell the same story to a very high degree of confidence.
These observations provide important independent ev-
idence for the existence and nature of the dark energy.
The observed cross-correlations are consistent with the
expected signal arising from the integrated Sachs-Wolfe
effect in the concordance model with a cosmological con-
stant. The observed signal is slightly higher than ex-pected,
higher than the expectation from WMAP best fit
model by about 1 , thus favouring models with a lower
Chances are dark energy is not just pie in the sky but a real "thing".
. However, we do not see any significant trend for the
excess as a function of redshift, and so there is no indi-cation
of an evolving dark energy density. By combining
these results with other cosmological data, we find a gen-erally
consistent picture of the behaviour of the Universe,
which is converging towards the CDM model although
the uncertainties remain considerable. The only partial
exception to this picture is the BAO result which, even
when combined with our ISW measurement, is in slight
tension with the CDM model (at ∼1 ).
No one here is claiming its all done and dusted, but we gave our best theory a serious beating (again) and its still standing up very well.
http://arxiv.org/abs/0801.4380
for the laymen among us:
VII. CONCLUSIONS
In this paper, we have measured the cross-correlation
between the CMB and a large range of probes of the
density in a consistent way, and have calculated their
covariance taking into account their overlapping sky cov-
erage and redshift distributions. While individual mea-
surements vary somewhat depending on how the data are
cleaned and how the covariance is calculated, the overall
significance of the detection of cross-correlations is at the
∼4 5 level.
This means we looked at a hell of a lot of stuff that other people have done, loads of different ways of "looking" at the universe, and found that they pretty much all tell the same story to a very high degree of confidence.
These observations provide important independent ev-
idence for the existence and nature of the dark energy.
The observed cross-correlations are consistent with the
expected signal arising from the integrated Sachs-Wolfe
effect in the concordance model with a cosmological con-
stant. The observed signal is slightly higher than ex-pected,
higher than the expectation from WMAP best fit
model by about 1 , thus favouring models with a lower
Chances are dark energy is not just pie in the sky but a real "thing".
. However, we do not see any significant trend for the
excess as a function of redshift, and so there is no indi-cation
of an evolving dark energy density. By combining
these results with other cosmological data, we find a gen-erally
consistent picture of the behaviour of the Universe,
which is converging towards the CDM model although
the uncertainties remain considerable. The only partial
exception to this picture is the BAO result which, even
when combined with our ISW measurement, is in slight
tension with the CDM model (at ∼1 ).
No one here is claiming its all done and dusted, but we gave our best theory a serious beating (again) and its still standing up very well.