Computing Non- Gaussian Maps of the CMB
arXiv:astro-ph/0310229
Abstract
We discuss methods to compute maps of the CMB in models featuring active causal sources and in non-Gaussian models ofinflation. We show our large angle results as well as some preliminary results on small angles. We conclude by discussing on-going work.
arXiv commentTo appear in the proceedings of the XVth Rencontres de Blois. Added 2 references
References in corpus (5)
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