From the uniform distribution to fractals (Englisch)
- Neue Suche nach: Cooray, A.
- Neue Suche nach: Komatsu, E.
- Neue Suche nach: Melchiorri, A.
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ISBN:
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ISSN:
- Aufsatz (Konferenz) / Print
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Titel:From the uniform distribution to fractals
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Beteiligte:
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Kongress:186th, International School of Physics ``Enrico Fermi''; New horizons for observational cosmology; Nuovi orizzonti per la cosmologia osservativa; edited by A. Cooray, E. Komatsu, A. Melchiorri, directors of the course and L. Lamagna ; 2013 ; Varenna, Italy
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Erschienen in:
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Verlag:
- Neue Suche nach: IOS Press
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Erscheinungsort:Amsterdam
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Erscheinungsdatum:01.01.2014
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Format / Umfang:376 pages
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Anmerkungen:Includes bibliographical references
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ISBN:
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ISSN:
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Medientyp:Aufsatz (Konferenz)
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Format:Print
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Sprache:Englisch
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Schlagwörter:
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Datenquelle:
© Metadata Copyright the British Library Board and other contributors. All rights reserved.
Inhaltsverzeichnis Konferenzband
Die Inhaltsverzeichnisse werden automatisch erzeugt und basieren auf den im Index des TIB-Portals verfügbaren Einzelnachweisen der enthaltenen Beiträge. Die Anzeige der Inhaltsverzeichnisse kann daher unvollständig oder lückenhaft sein.
- 1
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Lecture I: The Intergalactic Medium| 2014
- 1
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Reionization of the Intergalactic MediumFerrara, A. / Pandolfi, S. et al. | 2014
- 2
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Historical background| 2014
- 2
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Early confinement models| 2014
- 4
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IGM as a fluctuating density field| 2014
- 5
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IGM phenomenology| 2014
- 7
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QSO absorption spectra| 2014
- 7
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Low resolution spectroscopy| 2014
- 9
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High resolution spectroscopy| 2014
- 10
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Number density evolution of the Ly alpha forest| 2014
- 10
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Absorption line properties| 2014
- 10
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Column density distribution| 2014
- 11
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Photoionization| 2014
- 11
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Basic physical processes| 2014
- 14
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The UV background| 2014
- 16
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Proximity effect| 2014
- 17
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Gunn-peterson effect| 2014
- 18
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HI evolution| 2014
- 20
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Primordial cooling function| 2014
- 21
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Equation of state| 2014
- 23
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Temperature evolution| 2014
- 24
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IGM mass content| 2014
- 24
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Ab initio models| 2014
- 24
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Galaxy-IGM interplay| 2014
- 26
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Overcooling problem| 2014
- 28
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Heating and metal enrichment| 2014
- 30
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Introduction| 2014
- 30
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Lecture II: Cosmic reionization| 2014
- 31
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Basic theory| 2014
- 31
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Propagation of ionization fronts in the IGM| 2014
- 34
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Statistical approach| 2014
- 35
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Cosmological radiative transfer| 2014
- 35
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``Hello world'' reionization model| 2014
- 37
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Numerical solution techniques| 2014
- 38
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Cosmic reionization| 2014
- 40
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Reionization sources| 2014
- 42
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(More) reionization tests| 2014
- 42
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Cosmic microwave background| 2014
- 44
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X-rays effects| 2014
- 45
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Chemical feedback| 2014
- 46
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Challenges| 2014
- 47
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Global reionization models| 2014
- 49
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Parameter uncertainties| 2014
- 50
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Escape fraction| 2014
- 51
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Specific ionizing photon production| 2014
- 52
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Reionization and cosmology| 2014
- 59
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Weak gravitational lensingHoekstra, H. et al. | 2014
- 61
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Gravitational lensing| 2014
- 61
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Lens equation| 2014
- 62
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Delay| 2014
- 63
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Differential deflection| 2014
- 63
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Deflection| 2014
- 66
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Mass reconstructions| 2014
- 68
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Mass estimates| 2014
- 69
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Measuring galaxy shapes| 2014
- 70
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Observational distortions| 2014
- 71
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PSF model| 2014
- 73
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Image simulations| 2014
- 74
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Lensing by clusters| 2014
- 76
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Lensing by galaxies| 2014
- 78
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Halo model| 2014
- 80
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Halo shapes| 2014
- 81
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Lensing by large-scale structure| 2014
- 85
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Photometric redshifts and tomography| 2014
- 87
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Predictions for the matter power spectrum| 2014
- 91
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Results from CFHTLenS| 2014
- 92
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Outlook and conclusions| 2014
- 101
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Large-scale structure observationsPercival, W.J. et al. | 2014
- 101
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Clustering statistics| 2014
- 101
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The over-density field| 2014
- 102
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The correlation function| 2014
- 102
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The power spectrum| 2014
- 103
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Anisotropic statistics| 2014
- 103
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Higher-order statistics| 2014
- 104
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The matter-radiation equality scale| 2014
- 104
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The comoving matter power spectrum| 2014
- 105
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Baryons| 2014
- 105
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Neutrino masses| 2014
- 106
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Physical processes| 2014
- 106
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Linear structure growth| 2014
- 107
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Spherical collapse| 2014
- 109
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Press-Schechter theory| 2014
- 109
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Galaxy bias| 2014
- 111
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Overview of galaxy surveys| 2014
- 111
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Galaxy survey basics| 2014
- 112
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Measuring over-densities| 2014
- 113
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Measuring the power spectrum| 2014
- 114
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Measuring the correlation function| 2014
- 115
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Reconstructing the linear density| 2014
- 116
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Ly- alpha forest surveys| 2014
- 117
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Projection and the Alcock-Paczynski (AP) effect| 2014
- 117
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Observational effects| 2014
- 118
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Redshift-space distortions| 2014
- 121
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Primordial non-Gaussianity| 2014
- 121
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Joint AP and RSD measurements| 2014
- 122
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Summary| 2014
- 122
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Making cosmological-model inferences| 2014
- 123
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Exploring parameter space| 2014
- 124
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Model selection| 2014
- 125
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Future surveys| 2014
- 125
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The next 5 years| 2014
- 126
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5-20 years time| 2014
- 126
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Fisher methods| 2014
- 128
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Predictions for future surveys| 2014
- 137
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Galaxy formationSilk, J. / Di Cintio, A. / Dvorkin, I. et al. | 2014
- 138
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Initial mass function and star formation| 2014
- 140
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Star formation: general considerations| 2014
- 144
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The first stars| 2014
- 145
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Initial stellar mass function| 2014
- 146
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From linear theory to galaxy formation| 2014
- 148
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Linear theory| 2014
- 150
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Non-linear theory| 2014
- 153
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Halo mass function| 2014
- 154
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Comparison with observations| 2014
- 155
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From mass to light: Reconciling theory with observations| 2014
- 155
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Galaxy luminosity function| 2014
- 156
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Supernova-driven winds| 2014
- 157
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Entropy barrier| 2014
- 158
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Tidal disruption| 2014
- 159
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The core/cusp problem| 2014
- 160
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Cosmic reionization by dwarf galaxies| 2014
- 161
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Computational methods in galaxy formation| 2014
- 163
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A global star formation law| 2014
- 166
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Formation of disk galaxies and spin alignment| 2014
- 166
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Disk galaxies| 2014
- 168
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Bulgeless disk galaxies| 2014
- 169
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Feedback from supermassive black holes| 2014
- 169
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The role of AGN| 2014
- 170
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Modes of AGN feedback| 2014
- 171
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Positive feedback from AGN| 2014
- 172
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SMBH formation| 2014
- 173
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Gas accretion in galaxies| 2014
- 174
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Evolution of early-type galaxies (ETG)| 2014
- 174
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The two modes of star formation| 2014
- 174
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The SFR main sequence and starburst galaxies| 2014
- 175
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Multiple stellar populations and the AGN connection| 2014
- 178
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Specific star formation rate| 2014
- 178
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Efficiency of galaxy formation and downsizing of galaxies| 2014
- 180
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Current issues| 2014
- 189
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Cosmology: From theory to data, from data to theoryLeclercq, F. / Pisani, A. / Wandelt, B.D. et al. | 2014
- 190
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Introduction: the big picture| 2014
- 191
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Cosmological probes| 2014
- 191
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Observable and knowable| 2014
- 194
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Limits to cosmological knowledge, causal diagrams| 2014
- 195
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Information accessible directly, now| 2014
- 196
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Information accessible directly, over time| 2014
- 196
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Information accessible indirectly| 2014
- 198
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Primordial perturbations and the CMB| 2014
- 198
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The birth of perturbations| 2014
- 202
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Gaussian random fields| 2014
- 202
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Definition| 2014
- 202
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Moments of Gaussian random fields and Wick's theorem| 2014
- 203
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Marginals and conditionals of Gaussian random fields| 2014
- 203
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(Mis)-conceptions about Gaussian random fields| 2014
- 204
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The linear physics CMB time-machine| 2014
- 206
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Bayesian cosmostatistics| 2014
- 206
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What is Bayesian analysis?| 2014
- 207
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Prior choice| 2014
- 210
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First level inference: Bayesian parameter inference| 2014
- 211
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Exploration of the posterior| 2014
- 213
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Markov Chain Monte Carlo techniques for parameter inference| 2014
- 216
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Second level inference: Bayesian model comparison| 2014
- 219
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Bayesian non-linear inference of the initial conditions from large-scale structure surveys| 2014
- 219
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Applications of inference| 2014
- 220
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Planck results on primordial non-Gaussianity| 2014
- 222
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Bispectra, the inflationary landscape and non-Gaussianity| 2014
- 225
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The late-time bispectrum| 2014
- 226
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Primordial non-Gaussianity inference| 2014
- 229
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Planck constraints on inflationary models| 2014
- 229
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Conclusion: From theory to data - There and Back Again ... A cosmologist's tale| 2014
- 237
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Constraints on sterile neutrinos from the latest cosmological dataArchidiacono, M. et al. | 2014
- 238
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Analysis method: Data sets and parameters| 2014
- 239
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Results| 2014
- 241
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Conclusions| 2014
- 243
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Constraints on inflationary features in the primordial power spectrum with the Planck dataBenetti, M. et al. | 2014
- 244
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Model and analysis method| 2014
- 245
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Results and discussion| 2014
- 248
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Concluding remarks| 2014
- 251
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Mechanical Anti-Reflection Structure for optical devices in the mm bandBuzi, D. / De Petris, M. / Lamagna, L. / De Gregori, S. et al. | 2014
- 252
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Simulations and optical performance| 2014
- 255
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Next steps and scientific goals| 2014
- 257
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A 4-bands imaging spectro-photometer for balloon-borne observations of the Sunyaev-Zel'dovich effectCoppolecchia, A. / Amico, G. / Battistelli, E.S. / de Bernardis, P. / Cruciani, A. / D Addabbo, A. / D Alessandro, G. / De Gregori, S. / De Petris, M. / Gualtieri, R. et al. | 2014
- 258
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Science| 2014
- 259
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Payload and optics| 2014
- 260
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Cryostat| 2014
- 261
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Arrays of detectors| 2014
- 261
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Low-Frequency (LF) Arrays - Transition Edge Sensor (TES)| 2014
- 261
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High-Frequency (HF) Arrays - Semiconductor Bolometers| 2014
- 262
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DFTS| 2014
- 263
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Polar flights| 2014
- 264
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Discussion and conclusions| 2014
- 265
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Dark radiationDi Valentino, E. et al. | 2014
- 266
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Effective mass| 2014
- 266
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Sterile neutrino constraints| 2014
- 267
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Neutrino mixing parameters| 2014
- 269
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Extended dark sector models| 2014
- 273
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Modeling the hierarchical evolution of galaxy clustersDvorkin, I. et al. | 2014
- 274
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Modeling cluster evolution| 2014
- 276
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SZ power spectrum| 2014
- 276
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Intracluster gas| 2014
- 277
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Discussion| 2014
- 279
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Neutrino anisotropies after PlanckGerbino, M. / Di Valentino, E. / Said, N. et al. | 2014
- 281
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Data analysis method| 2014
- 287
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Description| 2014
- 287
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Constraints on neutrino masses from Planck and Galaxy Clustering dataGiusarma, E. et al. | 2014
- 288
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Data and cosmological parameters| 2014
- 289
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DR8 clustering model| 2014
- 289
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Clustering modeling| 2014
- 290
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DR9 clustering model| 2014
- 290
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Standard cosmology plus massive neutrinos| 2014
- 291
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Dark energy and massive neutrinos| 2014
- 292
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Curvature and massive neutrinos| 2014
- 295
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Computational modelling of horn antennas| 2014
- 295
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Optical modelling of the Planck multi-mode channelsAuley, M. / Murphy, J.A. / Wilson, D. / O Sullivan, C. et al. | 2014
- 297
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The Planck-HFI multi-mode horns| 2014
- 298
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Fitting pre-launch multi-mode measurements| 2014
- 301
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Full Planck model and beam patterns on the sky| 2014
- 303
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Updated constraints from PLANCK on f(R) theoriesMarchini, A. / Salvatelli, V. et al. | 2014
- 304
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Parametrized Modified Gravity| 2014
- 305
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Analysis and results| 2014
- 309
-
Future constraints on scalar field driven Dark Energy coupled with electromagnetismMartinelli, M. / Pandolfi, S. / Calabrese, E. / Cardone, V.F. / Martins, C.J.A.P. / Spiro, S. / Vielzeuf, P.E. et al. | 2014
- 310
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Theoretical models| 2014
- 311
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Supernovae Type-Ia data| 2014
- 311
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Observational probes| 2014
- 312
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Redshift-drift data| 2014
- 312
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Quasar absorption systems data| 2014
- 312
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Weak lensing (WL) data| 2014
- 313
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Atomic clocks bounds| 2014
- 317
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Constraining variations of the fine-structure constant with PlanckMenegoni, E. / Galli, S. / Melchiorri, A. et al. | 2014
- 318
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Analysis| 2014
- 321
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Looking for primordial non-Gaussianity using Minkowski Functionals and Neural NetworksNovaes, C.P. / Wuensche, C.A. / Bernui, A. / Ferreira, I.S. et al. | 2014
- 322
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Minkowski Functionals| 2014
- 322
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The combined method: Minkowski Functionals + Neural Network| 2014
- 323
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Neural Networks| 2014
- 323
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Simulated data| 2014
- 324
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Preliminary results| 2014
- 324
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Analyses of simulated CMB maps| 2014
- 324
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Sensitivity tests| 2014
- 324
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Robustness tests| 2014
- 324
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Conclusions and perspectives| 2014
- 327
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Probing dark energy with redshift driftPandolfi, S. / Martinelli, M. et al. | 2014
- 328
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The redshift-drift test| 2014
- 329
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CODEX and the Ly alpha forest of QSO| 2014
- 330
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Analysis method| 2014
- 335
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The challenge of cosmic voidsPisani, A. / Wandelt, B.D. et al. | 2014
- 336
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Sparsity and void stacking| 2014
- 337
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Overcoming redshift-space distortions: real-space density reconstruction| 2014
- 337
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Standard spheres, cosmology and Alcock-Paczynski test| 2014
- 339
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Results: Simulation and SDSS data| 2014
- 340
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Conclusion: The future| 2014
- 341
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Dark energy equation of state: a PCA approachSaid, N. et al. | 2014
- 342
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Data| 2014
- 344
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CMB+SNIa+BAO| 2014
- 344
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Adding HST and H(z)| 2014
- 345
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Comparison with alternatives to ACDM| 2014
- 349
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New constraints on interacting dark energy from Planck experimentSalvatelli, V. / Marchini, A. et al. | 2014
- 350
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Dark interaction parameterization| 2014
- 357
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Measuring sigma ~8, bias and the cross-correlation coefficient on DES-SV MICE simulationsSanchez, C. / Bonnett, C. / Crocce, M. / Fosalba, P. / Gaztanaga, E. / Miquel, R. et al. | 2014
- 358
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Method| 2014
- 365
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Probing the EoR with atomic and molecular linesSilva, M. / Santos, M. / Gong, Y. / Cooray, A. et al. | 2014
- 366
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Intensity mapping of CII emission| 2014
- 368
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Intensity mapping of Lyman alpha emission| 2014
- 370
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Cross correlation| 2014
- 373
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A new geometrical approach to void statisticsWerner, M.C. et al. | 2014
- 374
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From sphere geometry to de Sitter| 2014
- 374
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de Sitter configuration space| 2014
- 376
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From the uniform distribution to fractals| 2014
- 377
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Comparison with structure formation theory| 2014
- 377
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Application to cosmology| 2014
- 378
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Outlook| 2014
- 378
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Comparison with data| 2014