Initial stellar mass function (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:Initial stellar mass function
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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:145 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
-
Reionization of the Intergalactic MediumFerrara, A. / Pandolfi, S. et al. | 2014
- 1
-
Lecture I: The Intergalactic Medium| 2014
- 2
-
Historical background| 2014
- 2
-
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
-
Basic physical processes| 2014
- 11
-
Photoionization| 2014
- 14
-
The UV background| 2014
- 16
-
Proximity effect| 2014
- 17
-
Gunn-peterson effect| 2014
- 18
-
HI evolution| 2014
- 20
-
Primordial cooling function| 2014
- 21
-
Equation of state| 2014
- 23
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Temperature evolution| 2014
- 24
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Ab initio models| 2014
- 24
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Galaxy-IGM interplay| 2014
- 24
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IGM mass content| 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
-
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
-
``Hello world'' reionization model| 2014
- 35
-
Cosmological radiative transfer| 2014
- 37
-
Numerical solution techniques| 2014
- 38
-
Cosmic reionization| 2014
- 40
-
Reionization sources| 2014
- 42
-
Cosmic microwave background| 2014
- 42
-
(More) reionization tests| 2014
- 44
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X-rays effects| 2014
- 45
-
Chemical feedback| 2014
- 46
-
Challenges| 2014
- 47
-
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
-
Observational distortions| 2014
- 71
-
PSF model| 2014
- 73
-
Image simulations| 2014
- 74
-
Lensing by clusters| 2014
- 76
-
Lensing by galaxies| 2014
- 78
-
Halo model| 2014
- 80
-
Halo shapes| 2014
- 81
-
Lensing by large-scale structure| 2014
- 85
-
Photometric redshifts and tomography| 2014
- 87
-
Predictions for the matter power spectrum| 2014
- 91
-
Results from CFHTLenS| 2014
- 92
-
Outlook and conclusions| 2014
- 101
-
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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Anisotropic statistics| 2014
- 103
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Higher-order statistics| 2014
- 104
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The comoving matter power spectrum| 2014
- 104
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The matter-radiation equality scale| 2014
- 105
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Baryons| 2014
- 105
-
Neutrino masses| 2014
- 106
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Linear structure growth| 2014
- 106
-
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
-
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
-
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
-
Redshift-space distortions| 2014
- 121
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Joint AP and RSD measurements| 2014
- 121
-
Primordial non-Gaussianity| 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
-
Galaxy luminosity function| 2014
- 155
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From mass to light: Reconciling theory with observations| 2014
- 156
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Supernova-driven winds| 2014
- 157
-
Entropy barrier| 2014
- 158
-
Tidal disruption| 2014
- 159
-
The core/cusp problem| 2014
- 160
-
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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The role of AGN| 2014
- 169
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Feedback from supermassive black holes| 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
-
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 indirectly| 2014
- 196
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Information accessible directly, over time| 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
-
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
-
Low-Frequency (LF) Arrays - Transition Edge Sensor (TES)| 2014
- 261
-
Arrays of detectors| 2014
- 262
-
DFTS| 2014
- 263
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Polar flights| 2014
- 264
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Discussion and conclusions| 2014
- 265
-
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
-
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
-
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
-
Clustering modeling| 2014
- 289
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DR8 clustering model| 2014
- 290
-
Standard cosmology plus massive neutrinos| 2014
- 290
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DR9 clustering model| 2014
- 291
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Dark energy and massive neutrinos| 2014
- 292
-
Curvature and massive neutrinos| 2014
- 295
-
Optical modelling of the Planck multi-mode channelsAuley, M. / Murphy, J.A. / Wilson, D. / O Sullivan, C. et al. | 2014
- 295
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Computational modelling of horn antennas| 2014
- 297
-
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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Observational probes| 2014
- 311
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Supernovae Type-Ia data| 2014
- 312
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Weak lensing (WL) data| 2014
- 312
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Quasar absorption systems data| 2014
- 312
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Redshift-drift 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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The combined method: Minkowski Functionals + Neural Network| 2014
- 322
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Minkowski Functionals| 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
-
Preliminary results| 2014
- 324
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Robustness tests| 2014
- 324
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Conclusions and perspectives| 2014
- 324
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Sensitivity tests| 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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Standard spheres, cosmology and Alcock-Paczynski test| 2014
- 337
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Overcoming redshift-space distortions: real-space density reconstruction| 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
-
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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Comparison with data| 2014
- 378
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Outlook| 2014