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Titlebook: Data Analysis in Cosmology; Vicent J. Martinez,Enn Saar,Maria Jesus Pons-Borde Book 2009 Springer-Verlag Berlin Heidelberg 2009 Cosmology.

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31#
發(fā)表于 2025-3-27 00:19:22 | 只看該作者
Techniques for Compact Source Extraction in CMB Mapsiew of different techniques developed for the detectionand extraction of compact sources, with an especial focus on theirapplication to the field of the cosmic microwave backgroundradiation. In particular, we will consider the detection ofextragalactic point sources and the thermal and kinematicSunyaev–Zeldovich effects from clusters of galaxies.
32#
發(fā)表于 2025-3-27 02:19:30 | 只看該作者
33#
發(fā)表于 2025-3-27 06:46:10 | 只看該作者
34#
發(fā)表于 2025-3-27 12:52:26 | 只看該作者
35#
發(fā)表于 2025-3-27 16:56:57 | 只看該作者
36#
發(fā)表于 2025-3-27 21:06:10 | 只看該作者
Grundprinzipien der CED-BehandlungI describe the process of generating sky maps and estimating the power spectra from the raw CMB time stream data.
37#
發(fā)表于 2025-3-28 00:50:14 | 只看該作者
38#
發(fā)表于 2025-3-28 03:30:57 | 只看該作者
Determination of Cosmological Parameters from Cosmic Microwave Background AnisotropiesNew cosmic microwave background anisotropies data are increasingly improving our understanding of the evolution and formation of structures in the universe. Here we briefly discuss the cosmological parameters extraction methods, review the latest results and comment about possible modifications to the standard model.
39#
發(fā)表于 2025-3-28 08:24:11 | 只看該作者
Cosmic Microwave Background Data Analysis: From Time-Ordered Data to Angular Power SpectraI describe the process of generating sky maps and estimating the power spectra from the raw CMB time stream data.
40#
發(fā)表于 2025-3-28 10:28:38 | 只看該作者
Pouchitis und Diversionskolitisdata are taken, to see whether the survey will actually do what is required. We also take a look at data compression methods, such as Karhunen–Loève and MOPED, which can be extremely valuable for speeding up analysis of large data sets, and making the analysis more stable.
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