Measuring galaxy shapes (English)
- New search for: Cooray, A.
- New search for: Komatsu, E.
- New search for: Melchiorri, A.
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ISBN:
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ISSN:
- Conference paper / Print
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Title:Measuring galaxy shapes
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Contributors:
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Conference: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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Published in:
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Publisher:
- New search for: IOS Press
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Place of publication:Amsterdam
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Publication date:2014-01-01
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Size:69 pages
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Remarks:Includes bibliographical references
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ISBN:
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ISSN:
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Type of media:Conference paper
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Type of material:Print
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Language:English
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Keywords:
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Source:
© Metadata Copyright the British Library Board and other contributors. All rights reserved.
Table of contents conference proceedings
The tables of contents are generated automatically and are based on the data records of the individual contributions available in the index of the TIB portal. The display of the Tables of Contents may therefore be incomplete.
- 1
-
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
-
Low resolution spectroscopy| 2014
- 7
-
QSO absorption spectra| 2014
- 9
-
High resolution spectroscopy| 2014
- 10
-
Column density distribution| 2014
- 10
-
Absorption line properties| 2014
- 10
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Number density evolution of the Ly alpha forest| 2014
- 11
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Photoionization| 2014
- 11
-
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
-
Equation of state| 2014
- 23
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Temperature evolution| 2014
- 24
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Galaxy-IGM interplay| 2014
- 24
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IGM mass content| 2014
- 24
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Ab initio models| 2014
- 26
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Overcooling problem| 2014
- 28
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Heating and metal enrichment| 2014
- 30
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Lecture II: Cosmic reionization| 2014
- 30
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Introduction| 2014
- 31
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Propagation of ionization fronts in the IGM| 2014
- 31
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Basic theory| 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
-
Cosmic reionization| 2014
- 40
-
Reionization sources| 2014
- 42
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(More) reionization tests| 2014
- 42
-
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
-
Parameter uncertainties| 2014
- 50
-
Escape fraction| 2014
- 51
-
Specific ionizing photon production| 2014
- 52
-
Reionization and cosmology| 2014
- 59
-
Weak gravitational lensingHoekstra, H. et al. | 2014
- 61
-
Lens equation| 2014
- 61
-
Gravitational lensing| 2014
- 62
-
Delay| 2014
- 63
-
Deflection| 2014
- 63
-
Differential deflection| 2014
- 66
-
Mass reconstructions| 2014
- 68
-
Mass estimates| 2014
- 69
-
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
-
Predictions for the matter power spectrum| 2014
- 91
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Results from CFHTLenS| 2014
- 92
-
Outlook and conclusions| 2014
- 101
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Large-scale structure observationsPercival, W.J. et al. | 2014
- 101
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The over-density field| 2014
- 101
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Clustering statistics| 2014
- 102
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The power spectrum| 2014
- 102
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The correlation function| 2014
- 103
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Higher-order statistics| 2014
- 103
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Anisotropic 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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Linear structure growth| 2014
- 106
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Physical processes| 2014
- 107
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Spherical collapse| 2014
- 109
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Press-Schechter theory| 2014
- 109
-
Galaxy bias| 2014
- 111
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Galaxy survey basics| 2014
- 111
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Overview of galaxy surveys| 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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Making cosmological-model inferences| 2014
- 122
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Summary| 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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Fisher methods| 2014
- 126
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5-20 years time| 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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The two modes of star formation| 2014
- 174
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The SFR main sequence and starburst galaxies| 2014
- 174
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Evolution of early-type galaxies (ETG)| 2014
- 175
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Multiple stellar populations and the AGN connection| 2014
- 178
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Efficiency of galaxy formation and downsizing of galaxies| 2014
- 178
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Specific star formation rate| 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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Moments of Gaussian random fields and Wick's theorem| 2014
- 202
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Gaussian random fields| 2014
- 202
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Definition| 2014
- 203
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(Mis)-conceptions about Gaussian random fields| 2014
- 203
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Marginals and conditionals of Gaussian random fields| 2014
- 204
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The linear physics CMB time-machine| 2014
- 206
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What is Bayesian analysis?| 2014
- 206
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Bayesian cosmostatistics| 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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Applications of inference| 2014
- 219
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Bayesian non-linear inference of the initial conditions from large-scale structure surveys| 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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Conclusion: From theory to data - There and Back Again ... A cosmologist's tale| 2014
- 229
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Planck constraints on inflationary models| 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
-
Cryostat| 2014
- 261
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High-Frequency (HF) Arrays - Semiconductor Bolometers| 2014
- 261
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Arrays of detectors| 2014
- 261
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Low-Frequency (LF) Arrays - Transition Edge Sensor (TES)| 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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Intracluster gas| 2014
- 276
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SZ power spectrum| 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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Constraints on neutrino masses from Planck and Galaxy Clustering dataGiusarma, E. et al. | 2014
- 287
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Description| 2014
- 288
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Data and cosmological parameters| 2014
- 289
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Clustering modeling| 2014
- 289
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DR8 clustering model| 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
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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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Weak lensing (WL) data| 2014
- 312
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Redshift-drift data| 2014
- 312
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Quasar absorption systems 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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Simulated data| 2014
- 323
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Neural Networks| 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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Preliminary results| 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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Adding HST and H(z)| 2014
- 344
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CMB+SNIa+BAO| 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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de Sitter configuration space| 2014
- 374
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From sphere geometry to de Sitter| 2014
- 376
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From the uniform distribution to fractals| 2014
- 377
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Application to cosmology| 2014
- 377
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Comparison with structure formation theory| 2014
- 378
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Outlook| 2014
- 378
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Comparison with data| 2014