MOSCARDINI, LAURO
 Distribuzione geografica
Continente #
NA - Nord America 5.661
AS - Asia 543
EU - Europa 439
AF - Africa 1
Continente sconosciuto - Info sul continente non disponibili 1
OC - Oceania 1
SA - Sud America 1
Totale 6.647
Nazione #
US - Stati Uniti d'America 5.657
CN - Cina 259
SG - Singapore 217
FI - Finlandia 104
UA - Ucraina 85
DE - Germania 72
IT - Italia 51
GB - Regno Unito 36
FR - Francia 35
SE - Svezia 33
VN - Vietnam 29
IN - India 20
TR - Turchia 12
IE - Irlanda 9
HK - Hong Kong 5
CA - Canada 4
NL - Olanda 4
LT - Lituania 2
RU - Federazione Russa 2
AT - Austria 1
AU - Australia 1
BE - Belgio 1
BG - Bulgaria 1
BY - Bielorussia 1
CO - Colombia 1
EE - Estonia 1
EU - Europa 1
JP - Giappone 1
RO - Romania 1
SC - Seychelles 1
Totale 6.647
Città #
Fairfield 918
Woodbridge 779
Ann Arbor 514
Houston 499
Ashburn 410
Jacksonville 379
Seattle 318
Cambridge 314
Wilmington 312
Chandler 195
Princeton 175
Singapore 173
Santa Clara 172
Boardman 95
San Diego 95
Beijing 64
Roxbury 54
Helsinki 35
Nanjing 34
Dong Ket 29
Des Moines 15
Jiaxing 15
Nanchang 15
Changsha 14
London 14
Shenyang 14
Norwalk 12
Yenibosna 12
Padova 11
Hebei 10
Dublin 9
Jinan 8
New York 7
Tianjin 7
Falls Church 6
Indiana 6
Tappahannock 6
Hangzhou 5
Hong Kong 5
Bari 4
Toronto 4
Washington 4
Kilburn 3
Medford 3
Ningbo 3
Shanghai 3
Verona 3
Bologna 2
Borås 2
Catania 2
Columbus 2
Hendon 2
Hounslow 2
Kharkiv 2
Milan 2
North Bergen 2
Redmond 2
San Francisco 2
San Mateo 2
Shenzhen 2
Taizhou 2
Zhengzhou 2
Acton 1
Albignasego 1
Andover 1
Auburn Hills 1
Bogotá 1
Breda Di Piave 1
Brussels 1
Buffalo 1
Calvizzano 1
Changchun 1
Chiswick 1
Coriano 1
Foshan 1
Frankfurt am Main 1
Genoa 1
Guangzhou 1
Guidonia 1
Haikou 1
Keila 1
Kunming 1
Lappeenranta 1
Los Angeles 1
Mahé 1
Minsk 1
Modesto 1
Nanyang 1
New Bedfont 1
Ogden 1
Paris 1
Perth 1
Pune 1
Quanzhou 1
Redwood City 1
Rockville 1
Rome 1
Rovato 1
San Pietro di Feletto 1
Shaoyang 1
Totale 5.850
Nome #
Large-Scale Bias in the Universe: II Redshift Space Bispectrum 146
Weighted Bias and Galaxy Clustering 146
Non-Gaussian Initial Conditions in Cosmological N-body Simulations: II. Cold Dark Matter Models 138
Testing the Frozen Flow Approximation 133
The impact of cluster mergers on arc statistics 127
The importance of merging activity for the kinetic polarization of the Sunyaev-Zel'dovich signal from galaxy clusters 121
The diffuse light in simulations of galaxy clusters 116
Effects of cluster galaxies on arc statistics 115
Skewness as a Test of Non-Gaussian Primordial Density Fluctuations 114
Measuring and modelling the redshift evolution of clustering: the Hubble Deep Field North 114
X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation 113
Testing the Velocity Field in Non-Scale Invariant Cold Dark Matter Models 113
Properties of galaxy clusters in cosmologies with dark energy 112
Modelling Galaxy Clustering at High Redshift 111
Non-Gaussian Initial Conditions in Cosmological N-body Simulations: III. Groups in Cold Dark Matter Models 109
Imprints of Primordial Non-Gaussianities in X-ray and SZ Signals from Galaxy Clusters 108
Arc statistics with numerical cluster models in of dark energy cosmologies 108
Large-Scale Angular Correlations in Cold Dark Matter Models 107
Mismatch between X-ray and emission-weighted temperatures in galaxy clusters: Cosmological implications 107
BeppoSAX temperature maps of galaxy clusters in the Corona Borealis supercluster: A2061, A2067 and A2124 106
The Epoch of Structure Formation in Blue Mixed Dark Matter Models 105
Predicting the Clustering Properties of Galaxy Clusters Detectable by the Planck satellite 104
Primordial non-Gaussianities in the intergalactic medium 104
Constraints on Extended Quintessence from High-Redshift Supernovae 103
The Variance of Quasar Counts in Cells 103
The Large-Scale Structure of the Universe in Skewed Cold Dark Matter Models 103
Redshift Evolution of Clustering 102
A Frozen-Flow Approximation to the Evolution of Large-Scale Structures in the Universe 101
A dynamical model for the distribution of dark matter and gas in galaxy clusters 101
Strong lensing by cluster-sized halos in dark energy cosmologies 100
Sunyaev-Zel'dovich profiles and scaling relations: modelling effects and observational biases 99
Topology in Two Dimensions-IV. CDM Models with Non-Gaussian Initial Conditions 98
Measuring the Redshift Evolution of Clustering: the Hubble Deep Field South 97
Eulerian Perturbation Theory in Non-Flat Universes: Second Order Approximation 97
Simulating the soft X-ray excess in clusters of galaxies 97
Properties of cluster satellites in hydrodynamical simulations 97
Higher Order Moments of the Matter Distribution in Scale-Free Cosmological Simulations with Large Dynamic Range 96
Giant cluster arcs as a constraint on the scattering cross- section of dark matter 93
The correlation function of X ray galaxy clusters in the ROSAT All Sky Survey 1 Bright Sample 91
Measuring cluster peculiar velocities with the Sunyaev- Zel'dovich effect: scaling relations and systematics 91
Simulating Chandra observations of galaxy clusters 91
Hot and cooled baryons in smoothed particle hydrodynamic simulations of galaxy clusters: physics and numerics 91
Systematics in the X-ray cluster mass estimators 90
Evolution of dark-matter haloes in a variety of dark-energy cosmologies 90
The clustering of galaxy clusters in cosmological models with non-Gaussian initial conditions: Predictions for future surveys 89
Virial scaling of massive dark matter halos: Why clusters prefer a high normalization cosmology 89
The integrated bispectrum as a test of cosmic microwave background non-Gaussianity: detection power and limits on f_NL with WMAP data 88
Cosmology through arc statistics I: sensitivity to Ωm and σ8 88
The mass density field in simulated non-Gaussian scenarios 86
Evolution at z >= 0.5 of the X-ray properties of simulated galaxy clusters: comparison with observational constraints 84
The potential of X-ray cluster surveys to constrain primordial non-Gaussianity. 84
Evolution of Massive Haloes in non-Gaussian Scenarios 82
The universality of the virial halo mass function and models for non-universality of other halo definitions 82
Numerical study of halo concentrations in dark-energy cosmologies 82
Constraining Cosmological Parameters with the Clustering Properties of Galaxy Clusters in Optical and X-ray Bands 81
The Effect of Primordial Non-Gaussianity on the Topology of Large-Scale Structure 79
Strong lensing efficiency of galaxy clusters in dark energy cosmologies 79
Comparing the temperatures of galaxy clusters from hydrodynamical N-body simulations to Chandra and XMM-Newton observations 78
A numerical study of the effects of primordial non-Gaussianities on weak lensing statistics 78
The Galaxy Velocity Field and Cold Dark Matter Models 78
Primordial non-Gaussianity: local curvature method and statistical significance of constraints on f_NL from WMAP data 77
Non-Gaussian Halo Assembly Bias 77
The clustering of Lyman break galaxies 77
Non-Gaussian Initial Conditions in Cosmological N-body Simulations: I. Space-Uncorrelated Models 76
Large-scale non-Gaussian mass function and halo bias: tests on N-body simulations 68
High-Resolution Simulations of Cosmic Microwave Background non-Gaussian Maps in Spherical Coordinates 68
Predicting the Clustering of X-ray Selected Galaxy Clusters in Flux-Limited Surveys 61
Euclid: Forecasts from the void-lensing cross-correlation 40
Dependency of halo concentration on mass, redshift and fossilness in Magneticum hydrodynamic simulations 37
Euclid preparation XIX. Impact of magnification on photometric galaxy clustering 34
The effect of primordial non-Gaussianity on the cosmological reionization 31
Erratum: Euclid preparation: XXI. Intermediate-redshift contaminants in the search for z > 6 galaxies within the Euclid Deep Survey (A&A (2022) 666 (A200) DOI: 10.1051/0004-6361/202243950 17
Totale 6.698
Categoria #
all - tutte 24.753
article - articoli 24.753
book - libri 0
conference - conferenze 0
curatela - curatele 0
other - altro 0
patent - brevetti 0
selected - selezionate 0
volume - volumi 0
Totale 49.506


Totale Lug Ago Sett Ott Nov Dic Gen Feb Mar Apr Mag Giu
2019/2020728 0 0 0 0 0 0 120 161 128 165 91 63
2020/2021950 36 75 11 84 44 153 32 72 228 46 102 67
2021/20221.038 44 106 207 54 33 61 66 97 41 26 151 152
2022/2023571 159 27 9 31 90 77 0 57 75 1 36 9
2023/2024252 16 34 28 20 15 31 13 17 3 0 37 38
2024/2025577 1 124 71 62 248 71 0 0 0 0 0 0
Totale 6.698