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astro-ph2003
Contributions of point extragalactic sources to the Cosmic Microwave Background bispectrum
F. Argüeso, J. González-Nuevo, L. Toffolatti
All the analyses of Cosmic Microwave Background (CMB) temperature maps up--to--date show that CMB anisotropies follow a Gaussian distribution. On the other hand, astrophysical fore…
astro-ph2003
Goodness-of-Fit Tests to study the Gaussianity of the MAXIMA data
L. Cayon, F. Argueso, E. Martinez-Gonzalez +1
Goodness-of-Fit tests, including Smooth ones, are introduced and applied to detect non-Gaussianity in Cosmic Microwave Background simulations. We study the power of three different…