Dark Energy: Is it Q or Lambda ?
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New observations of Cosmic Microwave Background Anisotropies, Supernovae luminosity distances and Galaxy Clustering are sharpening our knowledge about dark energy. Here we present the latest constraints.
4 pages, 2 figures, to appear in proceedings of the XVIIIth IAP Colloquium `On the Nature of Dark Energy', IAP, Paris
4 pages, 2 figures, to appear in proceedings of the XVIIIth IAP Colloquium `On the Nature of Dark Energy', IAP, Paris