XMM satellites were also presented. Concerning extra-galactic cartography, res ults from the local universe were discussed, like the distribution of super-clusters, and methods to be used with the VLT and the Planck and Hersehe (ESA, 2007) satellites. The latest results from the 2dF galaxy redshift survey were also debated. The Organization of this workshop is indebted to the colleagues of the Local Organizing Comittee for the help and good humour provided before, during and after the workshop. Special thanks are due to Carlos Martins for the great help and effort provided in the critical...
XMM satellites were also presented. Concerning extra-galactic cartography, res ults from the local universe were discussed, like the distribution of s...
The last few years saw the development of a plethora of experiments and surveys probing the cosmological parameters. The Cosmic Microwave Background (CMB), the Supernovae (SN) searches and galaxy cluster data, namely via X-rays and Sunyaev-Zel'dovich effect, are among the most prolific giving detailed information about the geometry, age and structure formation of the Universe.
The program of the WS-HCP workshop was aimed at highlighting the scientific achievements and to discuss the new environment of "precision cosmology" within these three probes. The objective was to analyse...
The last few years saw the development of a plethora of experiments and surveys probing the cosmological parameters. The Cosmic Microwave Backgroun...
The Square Kilometre Array (SKA) will provide more than one order of magnitude improvement in sensitivity compared with any existing radio telescope over a wavelength range of several hundred to one, from decametric to microwave wavelengths. It will revolutionize the study of the most abundant element in the Universe, hydrogen, from the epoch of reionisation to the present-day, probing the onset formation period of the very first stars, will closely scan proto-planets and, through the precision timing of pulsars, will detect the distortions of space-time due to gravitational radiation....
The Square Kilometre Array (SKA) will provide more than one order of magnitude improvement in sensitivity compared with any existing radio telesco...
: The Square Kilometre Array (SKA) will provide more than one order of magnitude improvement in sensitivity compared with any existing radio telescope over a wavelength range of several hundred to one, from decametric to microwave wavelengths. It will revolutionize the study of the most abundant element in the Universe, hydrogen, from the epoch of reionisation to the present-day, probing the onset formation period of the very first stars, will closely scan proto-planets and, through the precision timing of pulsars, will detect the distortions of space-time due to gravitational radiation....
: The Square Kilometre Array (SKA) will provide more than one order of magnitude improvement in sensitivity compared with any existing radio telesc...
