细查
发表于 2025-3-23 12:08:05
Diffuse Source Separation in CMB Observationsmajor source of limitation. This will be the case, in particular, for the upcoming observations by the Planck mission, to be launched by ESA in 2008 (Lamarre et al. , Mandolesi et al. , Lamarre et al. ), as well as for next-generation instruments dedicated to the observation of CMB polarization.
大漩涡
发表于 2025-3-23 17:15:28
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发微光
发表于 2025-3-23 18:22:16
Power Spectrum Estiamtion II. Linear Maximum Likelihoodral bias, Local Group flow, angular or radial systematics (arising for example from extinction), redshift distortions, quadratic compression, decorrelation, and disentanglement. The procedures are illustrated with results from the . PSCz survey. Most of the PSCz graphics included in this chapter have not been published elsewhere.
Cacophonous
发表于 2025-3-24 00:49:38
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带来墨水
发表于 2025-3-24 02:35:08
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vocation
发表于 2025-3-24 10:31:23
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Goblet-Cells
发表于 2025-3-24 12:18:33
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愉快吗
发表于 2025-3-24 15:17:48
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Apoptosis
发表于 2025-3-24 22:18:28
Data Analysis in Cosmology978-3-540-44767-2Series ISSN 0075-8450 Series E-ISSN 1616-6361
florid
发表于 2025-3-24 23:10:39
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.