COSMOLOGICAL PARAMETER ESTIMATION WITH LARGE SCALE STRUCTURE AND SUPERNOVAE DATA

Determination of Cosmological Parameters from Cosmic Microwave Background Anisotropies

First results from the Very Small Array -- IV. Cosmological parameter estimation

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High-sensitivity measurements of the cosmic microwave background power spectrum with the extended Very Small Array

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Running-mass inflation model and WMAP

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SPORE series winner. Astronomical perspectives for young children

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The cosmic microwave background power spectrum out to = 1400 measured by the Very Small Array

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The state of the dark energy equation of state

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