Paper: astro-ph/0603539
Date: Mon, 20 Mar 2006 19:47:01 GMT (97kb)

Title: Inflation models after WMAP year three

Authors: Laila Alabidi and David H. Lyth

Comments: 4 pages
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The survey of models in astro-ph/0510441 is updated. For the first time, a
large fraction of the models are ruled out at more than $3\sigma$.

\\ ( http://arXiv.org/abs/astro-ph/0603539 , 97kb)

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Paper: astro-ph/0508383

replaced with revised version Sun, 19 Mar 2006 18:26:23 GMT (282kb)

Title: A blind estimation of the power spectrum of CMB anisotropy from WMAP

Authors: Rajib Saha (IUCAA, IIT Kanpur), Pankaj Jain (IIT Kanpur) and Tarun
Souradeep (IUCAA)

Comments: 5 pages, 3 figures, (trimmed to 4 pages) Matches WMAP team estimate
exactly. The small excess is shown to be consistent with a significantly
tempered residual power from unresolved point sources, simulations include
foreground contamination, Suppl. details at:

http://meghnad.iucaa.ernet.in/~tarun/sup0508383

Report-no: IUCAA-34/2005

\\ ( http://arXiv.org/abs/astro-ph/0508383 , 282kb)