TORMEN, GIUSEPPE
 Distribuzione geografica
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Continente #
NA - Nord America 5.247
EU - Europa 426
AS - Asia 259
Continente sconosciuto - Info sul continente non disponibili 1
Totale 5.933
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Nazione #
US - Stati Uniti d'America 5.244
CN - Cina 205
FI - Finlandia 101
UA - Ucraina 91
DE - Germania 77
IT - Italia 49
GB - Regno Unito 39
SE - Svezia 36
VN - Vietnam 27
IN - India 20
BE - Belgio 10
IE - Irlanda 10
TR - Turchia 7
BG - Bulgaria 4
NL - Olanda 4
CA - Canada 3
RO - Romania 3
EU - Europa 1
FR - Francia 1
RU - Federazione Russa 1
Totale 5.933
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Città #
Fairfield 948
Woodbridge 743
Houston 525
Ann Arbor 378
Jacksonville 376
Ashburn 363
Seattle 355
Cambridge 313
Wilmington 309
Chandler 228
Princeton 169
San Diego 87
Roxbury 68
Beijing 64
Nanjing 41
Helsinki 32
Dong Ket 27
Boardman 21
Des Moines 16
London 16
Medford 16
Hebei 14
Jiaxing 14
Washington 14
Jinan 13
Nanchang 11
Brussels 10
Dublin 10
Indiana 9
Norwalk 9
Padova 9
Shenyang 9
Tianjin 9
Yenibosna 7
Changsha 5
Hangzhou 5
Mestre 5
Kharkiv 4
New York 4
Ningbo 4
Redmond 4
Siena 4
Sofia 4
Borås 3
Dallas 3
Legnaro 3
Motta Di Livenza 3
San Francisco 3
Taiyuan 3
Tappahannock 3
Toronto 3
Yellow Springs 3
Zhengzhou 3
Busto Arsizio 2
Chicago 2
Falls Church 2
Haikou 2
Majano 2
Orange 2
Pettorazza Grimani 2
Rockville 2
San Mateo 2
Taizhou 2
Timisoara 2
Albignasego 1
Auburn Hills 1
Bari 1
Buffalo 1
Camisano 1
Changchun 1
Coriano 1
Ercolano 1
Fuzhou 1
Grafing 1
Groningen 1
Guangzhou 1
Guidonia 1
Horia 1
Islington 1
Milan 1
New Bedfont 1
Portici 1
Rovato 1
Shenzhen 1
Udine 1
Totale 5.345
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Nome #
The structure and dynamical evolution of dark matter haloes 127
null 119
The importance of merging activity for the kinetic polarization of the Sunyaev-Zel'dovich signal from galaxy clusters 111
The impact of cluster mergers on arc statistics 110
Survival of substructure within dark matter haloes 109
Testing the Velocity Field in Non-Scale Invariant Cold Dark Matter Models 107
The rise and fall of satellites in galaxy clusters 105
Turbulent velocity fields in smoothed particle hydrodymanics simulated galaxy clusters: scaling laws for the turbulent energy 103
The diffuse light in simulations of galaxy clusters 103
Formation times and masses of dark matter haloes 102
The assembly of matter in galaxy clusters 102
Velocity Dipoles in Cold Dark Matter Cosmologies 102
Properties of galaxy clusters in cosmologies with dark energy 100
X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation 100
Effects of cluster galaxies on arc statistics 100
Analytical approach to subhalo population in dark matter haloes 100
The mass function and average mass-loss rate of dark matter subhaloes 99
Large-scale bias and the peak background split 98
The scaling relations of galaxy clusters and their dark matter halos 98
Turbulent gas motions in galaxy cluster simulations: The role of smoothed particle hydrodynamics viscosity 98
Mismatch between X-ray and emission-weighted temperatures in galaxy clusters: Cosmological implications 98
Arc statistics with numerical cluster models in of dark energy cosmologies 95
Properties of cluster satellites in hydrodynamical simulations 94
BeppoSAX temperature maps of galaxy clusters in the Corona Borealis supercluster: A2061, A2067 and A2124 92
The substructure hierarchy in dark matter haloes 90
A dynamical model for the distribution of dark matter and gas in galaxy clusters 89
An improved model for the formation times of dark matter haloes 89
Simulating the soft X-ray excess in clusters of galaxies 88
Strong lensing by cluster-sized halos in dark energy cosmologies 88
Sunyaev-Zel'dovich profiles and scaling relations: modelling effects and observational biases 87
Collisional dark matter and the structure of dark halos 85
Constraining the distribution of dark matter in dwarf spheroidal galaxies with stellar tidal streams 84
Dark matter annihilation in the halo of the Milky Way 84
Substructures in cold dark matter haloes 84
The population of dark matter subhaloes: mass functions and average mass-loss rates 82
Ellipsoidal halo finders and implications for models of triaxial halo formation 82
Some like it triaxial: the universality of dark matter halo shapes and their evolution along the cosmic time 82
The shapes of BCGs and normal ellipticals in nearby clusters 82
Velocity fields in non-Gaussian cold dark matter models. 81
Giant cluster arcs as a constraint on the scattering cross- section of dark matter 81
A reassessment of the evidence of the Integrated Sachs-Wolfe effect through the WMAP-NVSS correlation 80
Virial scaling of massive dark matter halos: Why clusters prefer a high normalization cosmology 80
Weakly self-interacting dark matter and the structure of dark halos 79
Systematics in the X-ray cluster mass estimators 79
Simulating Chandra observations of galaxy clusters 79
Hot and cooled baryons in smoothed particle hydrodynamic simulations of galaxy clusters: physics and numerics 79
Measuring cluster peculiar velocities with the Sunyaev- Zel'dovich effect: scaling relations and systematics 78
Cosmology through arc statistics I: sensitivity to Ωm and σ8 78
On the environmental dependence of halo formation 77
The universality of the virial halo mass function and models for non-universality of other halo definitions 77
An excursion set model of hierarchical clustering: ellipsoidal collapse and the moving barrier 75
Evolution at z >= 0.5 of the X-ray properties of simulated galaxy clusters: comparison with observational constraints 73
The Galaxy Velocity Field and Cold Dark Matter Models 73
Evolution of dark-matter haloes in a variety of dark-energy cosmologies 73
Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes 71
Strong lensing efficiency of galaxy clusters in dark energy cosmologies 68
The satellite population of the Milky Way in a Lambda CDM universe 66
A merger tree with microsolar mass resolution: application to gamma-ray emission from subhalo population 66
Numerical study of halo concentrations in dark-energy cosmologies 66
Comparing the temperatures of galaxy clusters from hydrodynamical N-body simulations to Chandra and XMM-Newton observations 65
Adding long-wavelength modes to an N-body simulation 63
RECALIBRATION OF THE H(-0.5)-MAGNITUDES OF SPIRAL GALAXIES 58
The shapes of BCGs and normal ellipticals in nearby clusters. 54
Testing students' ability to use derivatives, integrals, and vectors in a purely mathematical context and in a physical context 54
Formation times, mass growth histories and concentrations of dark matter haloes 53
Populating a cluster of galaxies - I. Results at z=0 46
A look into the inside of haloes: A characterization of the halo shape as a function of overdensity in the Planck cosmology 46
Modelling the shapes of the largest gravitationally bound objects 45
Derivatives, integrals and vectors in introductory mechanics: the development of a multi-representation test for university students 38
Dynamical evolution of the ICM 34
Assessment of students' understandings about the use of mathematical concepts in mechanics: results of the FisicaMente test 32
Le esperienze sul campo: la testimonianza dei docenti 32
Developing a Modern Physics curriculum: a collaborative training course for in-service teachers 31
FisicaMente: supporting first-year students in transferring mathematical skills and knowledge to a physical context. 31
Dynamics of stellar black holes in young star clusters with different metallicities - II. Black hole-black hole binaries 14
Dynamics of stellar black holes in young star clusters with different metallicities - II. Black hole-black hole binaries 14
Hydrodynamic Simulations of Galaxy Formation 12
Totale 5.969
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Categoria #
all - tutte 14.465
article - articoli 13.637
book - libri 0
conference - conferenze 0
curatela - curatele 0
other - altro 146
patent - brevetti 0
selected - selezionate 0
volume - volumi 89
Totale 28.337
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Totale Lug Ago Sett Ott Nov Dic Gen Feb Mar Apr Mag Giu
2018/2019736 0 0 104 3 5 7 10 40 1 129 242 195
2019/20201.319 178 29 26 102 133 115 122 164 125 166 110 49
2020/20211.231 40 62 11 86 121 220 62 60 307 52 134 76
2021/20221.051 40 90 210 39 50 81 58 80 70 35 123 175
2022/2023575 161 34 17 35 95 75 0 46 73 7 23 9
2023/2024105 19 39 47 0 0 0 0 0 0 0 0 0
Totale 5.969