A practical guide to Basic Statistical Techniques for Data Analysis in Cosmology
arXiv:0712.3028
Abstract
This is the summary of 4 Lectures given at the XIX Canary islands winter school of Astrophysics ''The Cosmic Microwave Background, from Quantum Fluctuations to the present Universe''. Lectures were intended for master/beginning PhD students in cosmology.
To appear in the proceedings of the XIX Canary Island Winter School "The Cosmic Microwave Background: from Quantum fluctuations to the present Universe", comments welcome. (fixed entry of table1)
References in corpus (1)
Cited by in corpus (9)
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- Galaxy bispectrum, primordial non-Gaussianity and redshift space distortions
- Interacting Ricci-like holographic dark energy
- Strong lensing systems and galaxy cluster observations as probe to the cosmic distance duality relation
- Accelerated expansion of the universe and chasing photons from the CMB to study the late time integrated Sachs-Wolfe effect over different redshift ranges
- Impact of Galactic dust non-Gaussianity on searches for B-modes from inflation
- Accelerating MCMC algorithms through Bayesian Deep Networks
- Cosmic Kite: Auto-encoding the Cosmic Microwave Background
- Number counts, confusion, mapping issues and sky coverage analysis for radio continuum surveys through EMU Early Science, EMU-ASKAP, and WODAN especially for cosmology science goals