By Sébastien Fabbro (auth.), Domingos Barbosa, António José Da Silva, Ana Maria Mourão (eds.)
The previous few years observed the advance of a plethora of experiments and surveys probing the cosmological parameters. The Cosmic Microwave historical past (CMB), the Supernovae (SN) searches and galaxy cluster facts, particularly through X-rays and Sunyaev-Zel'dovich impact, are one of the such a lot prolific giving targeted information regarding the geometry, age and constitution formation of the Universe.
The application of the WS-HCP workshop used to be geared toward highlighting the medical achievements and to debate the recent surroundings of "precision cosmology" inside of those 3 probes. the target used to be to examine varied observational innovations, universal difficulties specifically foregrounds, and to evaluate the influence of observational uncertainties within the decision of key cosmological parameters which describe the primordial universe and the big scale constitution formation mechanism.
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Extra info for 3K, SN’s, Clusters: Hunting the Cosmological Parameters with Precision Cosmology: A JENAM 2002 Workshop Porto, Portugal 3–5 September 2002
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B- V colour at maximum for nearby and distant SNe Ia (from Leibundgut 200 I) the absorption, but a significant difference between a sample of nearby SNe Ia and distant ones has been pointed out (Figure 2; Leibundgut, 2001 ). The majority of the distant objects is bluer than the bluest SNe Ia in the nearby universe. This can not be due to dust as we expect to observe at least some of the nearby objects with their intrinsic colours and not affected by dust in the host galaxies. Although there could be a selection effect at work, this distinction is worrisome.
3K, SN’s, Clusters: Hunting the Cosmological Parameters with Precision Cosmology: A JENAM 2002 Workshop Porto, Portugal 3–5 September 2002 by Sébastien Fabbro (auth.), Domingos Barbosa, António José Da Silva, Ana Maria Mourão (eds.)