標(biāo)題: Titlebook: Data Analysis in Cosmology; Vicent J. Martinez,Enn Saar,Maria Jesus Pons-Borde Book 2009 Springer-Verlag Berlin Heidelberg 2009 Cosmology. [打印本頁] 作者: 滋養(yǎng)物質(zhì) 時間: 2025-3-21 17:57
書目名稱Data Analysis in Cosmology影響因子(影響力)
書目名稱Data Analysis in Cosmology影響因子(影響力)學(xué)科排名
書目名稱Data Analysis in Cosmology網(wǎng)絡(luò)公開度
書目名稱Data Analysis in Cosmology網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Data Analysis in Cosmology被引頻次
書目名稱Data Analysis in Cosmology被引頻次學(xué)科排名
書目名稱Data Analysis in Cosmology年度引用
書目名稱Data Analysis in Cosmology年度引用學(xué)科排名
書目名稱Data Analysis in Cosmology讀者反饋
書目名稱Data Analysis in Cosmology讀者反饋學(xué)科排名
作者: 單調(diào)性 時間: 2025-3-21 23:17
Divertikulitis und Diversionskolitisistical properties of the polarization fields. We then discuss some of the key aspects of the analysis of CMB polarization data, focusing on the additional complications that arise compared to temperature data due to the tensor character of the polarization field.作者: Explosive 時間: 2025-3-22 01:02 作者: 壓倒 時間: 2025-3-22 08:02 作者: 粗鄙的人 時間: 2025-3-22 11:24 作者: 不公開 時間: 2025-3-22 16:29
Introduction to Higher Order Spatial Statistics in Cosmologycan have one through three, or even more dimensions; their degree of non- Gaussianity ranges from tiny to significant. Yet, there are several techniques and ideas, which are applicable to virtually all cosmological random fields, be it Lyman-a forests, LSS, or CMB.作者: 不公開 時間: 2025-3-22 18:09
Book 2009elopment of sophisticated algorithms and pipelines..Aiming at students and researchers the lecture notes in this volume explain in pedagogical manner the best techniques used to extract information from cosmological data, as well as reliable methods that should help us improve our view of?the universe..作者: STYX 時間: 2025-3-22 22:01
Chronisch entzündliche Darmerkrankungenmajor 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. [36], Mandolesi et al. [41], Lamarre et al. [35]), as well as for next-generation instruments dedicated to the observation of CMB polarization.作者: 解開 時間: 2025-3-23 03:20 作者: inhumane 時間: 2025-3-23 06:55 作者: 細(xì)查 時間: 2025-3-23 12:08
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. [36], Mandolesi et al. [41], Lamarre et al. [35]), as well as for next-generation instruments dedicated to the observation of CMB polarization.作者: 大漩渦 時間: 2025-3-23 17:15 作者: 發(fā)微光 時間: 2025-3-23 18:22
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.作者: Cacophonous 時間: 2025-3-24 00:49 作者: 帶來墨水 時間: 2025-3-24 02:35 作者: vocation 時間: 2025-3-24 10:31 作者: Goblet-Cells 時間: 2025-3-24 12:18 作者: 愉快嗎 時間: 2025-3-24 15:17 作者: Apoptosis 時間: 2025-3-24 22:18
Data Analysis in Cosmology978-3-540-44767-2Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: florid 時間: 2025-3-24 23:10
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.作者: incision 時間: 2025-3-25 06:41 作者: 酷熱 時間: 2025-3-25 10:09
Grenzbereiche der Dosierung von Mesalazinm the statistical distribution of the temperature random field. We review some recent developments in the study of the cosmic microwave background (CMB) anisotropies and present a description of the novel tools developed to analyse the properties of the CMB anisotropies beyond the power spectrum.作者: travail 時間: 2025-3-25 12:46 作者: 溝通 時間: 2025-3-25 17:03 作者: MEET 時間: 2025-3-25 21:13 作者: 廣口瓶 時間: 2025-3-26 01:45
https://doi.org/10.1007/978-3-540-44767-2Cosmology; Gravity; Likelihood; Universe; correlation; cosmic microwave background; data analysis; gravitat作者: Virtues 時間: 2025-3-26 07:51
978-3-642-06305-3Springer-Verlag Berlin Heidelberg 2009作者: sterilization 時間: 2025-3-26 11:55 作者: admission 時間: 2025-3-26 13:36 作者: NUL 時間: 2025-3-26 20:42
Cosmic Microwave Background Anisotropies: The Power Spectrum and Beyondm the statistical distribution of the temperature random field. We review some recent developments in the study of the cosmic microwave background (CMB) anisotropies and present a description of the novel tools developed to analyse the properties of the CMB anisotropies beyond the power spectrum.作者: 靦腆 時間: 2025-3-27 00:19
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.作者: 小步走路 時間: 2025-3-27 02:19 作者: 沙發(fā) 時間: 2025-3-27 06:46 作者: Hirsutism 時間: 2025-3-27 12:52 作者: FATAL 時間: 2025-3-27 16:56 作者: Glycogen 時間: 2025-3-27 21:06
Grundprinzipien der CED-BehandlungI describe the process of generating sky maps and estimating the power spectra from the raw CMB time stream data.作者: 非秘密 時間: 2025-3-28 00:50 作者: conference 時間: 2025-3-28 03:30
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.作者: Devastate 時間: 2025-3-28 08:24
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.作者: 喧鬧 時間: 2025-3-28 10:28
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.作者: expansive 時間: 2025-3-28 18:04
Chronisch entzündliche Darmerkrankungening examples: galaxy classification with principle component analysis, photometric redshift estimation with artificial neural networks and multi-parameter estimation with Markov chain Monte Carlo in a Bayesian framework.作者: OATH 時間: 2025-3-28 20:53 作者: VICT 時間: 2025-3-28 23:25 作者: 頂點(diǎn) 時間: 2025-3-29 06:22
Chronisch entzündliche Darmerkrankungenthe cosmic microwave background (CMB). The detector sensitivities of modern experiments have permitted to measure fluctuations of the CMB temperature with such a sensitivity that the contamination of the data by astrophysical foreground radiations, rather than by instrumental noise, is becoming the 作者: projectile 時間: 2025-3-29 10:15 作者: Amorous 時間: 2025-3-29 14:17
Dirk O. Stichtenoth,Oliver Bachmannnction or its Fourier transform, the power spectrum. In this review, we explain how our knowledge of cosmic structures, encapsulated by these statistical descriptors, has evolved since their first use when applied on the early galaxy catalogues to the present generation of wide and deep redshift sur作者: 偏狂癥 時間: 2025-3-29 16:25
Funktionelle Eigenschaften des Tr?nenfilmsealed through the painstaking efforts of redshift survey campaigns, it has completely revised our view of the matter distribution on these cosmological scales. The web-like spatial arrangement of galaxies and mass into elongated filaments, sheet-like walls and dense compact clusters, the existence o作者: ARCH 時間: 2025-3-29 23:14
Chronische Conjunctivitis — Trockenes Auges in Cosmology. The lectures offer a pedagogical introduction to the problem of estimating the power spectrum from galaxy surveys. The intention is to focus on concepts rather than on technical detail, but enough mathematics is provided to point the student in the right direction..This first lecture作者: freight 時間: 2025-3-30 03:08
K. W. Ruprecht,G. O. H. Naumann linear scales using maximum likelihood methods. As in the first chapter, the aims are pedagogical, and the emphasis is on concepts rather than technical detail. The chapter covers most of the salient issues, including selection functions, likelihood functions, Karhunen–Loève compression, pair-integ作者: 參考書目 時間: 2025-3-30 05:09
A. Zapletal,J. Zbojan,V. Pohanka,M. ?amanekround (CMB) to the large-scale structure (LSS) of the universe. These random fields are rich in their properties; they can be continuous or discrete; can have one through three, or even more dimensions; their degree of non- Gaussianity ranges from tiny to significant. Yet, there are several techniqu作者: 高歌 時間: 2025-3-30 11:59
Standardisierung der bronchialen Provokation to explain how galaxies and large-scale structure formed in the Universe. In the standard picture (the “concordance” model), a period of accelerated expansion (“inflation”) generated density fluctuations with simple statistical properties through quantum processes (Starobinsky [82], [83], [84]; Gut作者: ANTIC 時間: 2025-3-30 13:26
Abgrenzung zu anderen Erkrankungen. Multiscale methods form a wider and less well-defined area of tools and approaches; the term is used, e.g., in numerical analysis, but the main range of multiscale methods is based on application of wavelets.作者: 經(jīng)典 時間: 2025-3-30 20:00 作者: ASSET 時間: 2025-3-30 23:41 作者: 清洗 時間: 2025-3-31 01:46
Fisher Matrices and All That: Experimental Design and Data Compressiondata 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.作者: Aviary 時間: 2025-3-31 05:54
Data Compression, Classification and Parameter Estimation. Methods: Examples from Astronomying examples: galaxy classification with principle component analysis, photometric redshift estimation with artificial neural networks and multi-parameter estimation with Markov chain Monte Carlo in a Bayesian framework.
