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## Main Question or Discussion Point

Found the following. I leave the comment to the experts.

http://infoscience.epfl.ch/record/108833/files/

Y. Wiaux, P. Vielva, R.B. Barreiro, E. MartÃnez-González and P. Vandergheynst, Non-Gaussianity analysis on local morphological measures of WMAP data, Mon. Not. R. Astron. Soc., Vol. 385, pp. 939, 2008.

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Probing dark energy with steerable wavelets through correlation of WMAP and NVSS local morphological measures

Mcewenetal-MNRAS384-1289-2008

http://infoscience.epfl.ch/record/108833/files/

Y. Wiaux, P. Vielva, R.B. Barreiro, E. MartÃnez-González and P. Vandergheynst, Non-Gaussianity analysis on local morphological measures of WMAP data, Mon. Not. R. Astron. Soc., Vol. 385, pp. 939, 2008.

**“The observed non-Gaussianity is therefore probably to be imputed to the CMB temperature field itself, thereby questioning the basic inflationary scenario upon which the concordance cosmological model relies”**--------

Probing dark energy with steerable wavelets through correlation of WMAP and NVSS local morphological measures

Mcewenetal-MNRAS384-1289-2008