TORMEN, GIUSEPPE
 Distribuzione geografica
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Continente #
NA - Nord America 5.258
EU - Europa 412
AS - Asia 274
Continente sconosciuto - Info sul continente non disponibili 1
Totale 5.945
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Nazione #
US - Stati Uniti d'America 5.255
CN - Cina 213
FI - Finlandia 100
UA - Ucraina 88
DE - Germania 75
IT - Italia 58
GB - Regno Unito 36
SE - Svezia 33
VN - Vietnam 27
IN - India 20
IE - Irlanda 10
TR - Turchia 7
BG - Bulgaria 4
NL - Olanda 4
CA - Canada 3
HK - Hong Kong 3
RO - Romania 3
SG - Singapore 3
EU - Europa 1
KZ - Kazakistan 1
RU - Federazione Russa 1
Totale 5.945
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Città #
Fairfield 933
Woodbridge 721
Houston 507
Ashburn 432
Ann Arbor 368
Jacksonville 364
Seattle 364
Cambridge 310
Wilmington 301
Chandler 226
Princeton 169
San Diego 86
Beijing 69
Roxbury 68
Nanjing 40
Helsinki 32
Dong Ket 27
Boardman 20
Des Moines 16
Medford 16
Hebei 14
Jiaxing 14
Jinan 13
Washington 13
London 11
Nanchang 11
Dublin 10
Indiana 9
Norwalk 9
Padova 9
Shenyang 9
Tianjin 9
Yenibosna 7
New York 6
Changsha 5
Hangzhou 5
Mestre 5
Kharkiv 4
Ningbo 4
San Francisco 4
Siena 4
Sofia 4
Borås 3
Dallas 3
Hong Kong 3
Hounslow 3
Legnaro 3
Marcignago 3
Milan 3
Motta Di Livenza 3
Redmond 3
Taiyuan 3
Tappahannock 3
Toronto 3
Vicenza 3
Yellow Springs 3
Zhengzhou 3
Busto Arsizio 2
Falls Church 2
Guangzhou 2
Haikou 2
Kilburn 2
Majano 2
Orange 2
Pettorazza Grimani 2
Rockville 2
San Mateo 2
Taizhou 2
Timisoara 2
Acton 1
Albignasego 1
Astana 1
Bari 1
Buffalo 1
Camisano 1
Changchun 1
Chicago 1
Clifton 1
Coriano 1
Ercolano 1
Fontana 1
Fuzhou 1
Grafing 1
Groningen 1
Guidonia 1
Horia 1
Islington 1
New Bedfont 1
Ogden 1
Portici 1
Prescot 1
Rovato 1
Santa Clara 1
Secaucus 1
Shenzhen 1
Trieste 1
Udine 1
Totale 5.345
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Nome #
The structure and dynamical evolution of dark matter haloes 126
The importance of merging activity for the kinetic polarization of the Sunyaev-Zel'dovich signal from galaxy clusters 113
The impact of cluster mergers on arc statistics 111
Survival of substructure within dark matter haloes 107
Testing the Velocity Field in Non-Scale Invariant Cold Dark Matter Models 107
Turbulent velocity fields in smoothed particle hydrodymanics simulated galaxy clusters: scaling laws for the turbulent energy 105
The rise and fall of satellites in galaxy clusters 105
The diffuse light in simulations of galaxy clusters 105
Velocity Dipoles in Cold Dark Matter Cosmologies 103
Formation times and masses of dark matter haloes 102
X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation 102
Effects of cluster galaxies on arc statistics 102
Analytical approach to subhalo population in dark matter haloes 102
The assembly of matter in galaxy clusters 102
Large-scale bias and the peak background split 101
Properties of galaxy clusters in cosmologies with dark energy 101
Turbulent gas motions in galaxy cluster simulations: The role of smoothed particle hydrodynamics viscosity 100
The mass function and average mass-loss rate of dark matter subhaloes 100
Mismatch between X-ray and emission-weighted temperatures in galaxy clusters: Cosmological implications 99
Arc statistics with numerical cluster models in of dark energy cosmologies 99
The scaling relations of galaxy clusters and their dark matter halos 98
BeppoSAX temperature maps of galaxy clusters in the Corona Borealis supercluster: A2061, A2067 and A2124 95
Properties of cluster satellites in hydrodynamical simulations 94
A dynamical model for the distribution of dark matter and gas in galaxy clusters 93
Strong lensing by cluster-sized halos in dark energy cosmologies 92
An improved model for the formation times of dark matter haloes 91
The substructure hierarchy in dark matter haloes 90
Sunyaev-Zel'dovich profiles and scaling relations: modelling effects and observational biases 89
Dark matter annihilation in the halo of the Milky Way 88
Simulating the soft X-ray excess in clusters of galaxies 87
Constraining the distribution of dark matter in dwarf spheroidal galaxies with stellar tidal streams 86
Collisional dark matter and the structure of dark halos 85
A reassessment of the evidence of the Integrated Sachs-Wolfe effect through the WMAP-NVSS correlation 85
Some like it triaxial: the universality of dark matter halo shapes and their evolution along the cosmic time 85
Ellipsoidal halo finders and implications for models of triaxial halo formation 84
Substructures in cold dark matter haloes 84
Velocity fields in non-Gaussian cold dark matter models. 83
Systematics in the X-ray cluster mass estimators 83
The shapes of BCGs and normal ellipticals in nearby clusters 83
The population of dark matter subhaloes: mass functions and average mass-loss rates 82
Virial scaling of massive dark matter halos: Why clusters prefer a high normalization cosmology 82
Simulating Chandra observations of galaxy clusters 81
Giant cluster arcs as a constraint on the scattering cross- section of dark matter 80
Measuring cluster peculiar velocities with the Sunyaev- Zel'dovich effect: scaling relations and systematics 80
Hot and cooled baryons in smoothed particle hydrodynamic simulations of galaxy clusters: physics and numerics 80
Weakly self-interacting dark matter and the structure of dark halos 79
Evolution of dark-matter haloes in a variety of dark-energy cosmologies 79
An excursion set model of hierarchical clustering: ellipsoidal collapse and the moving barrier 78
The universality of the virial halo mass function and models for non-universality of other halo definitions 78
Cosmology through arc statistics I: sensitivity to Ωm and σ8 78
On the environmental dependence of halo formation 77
Evolution at z >= 0.5 of the X-ray properties of simulated galaxy clusters: comparison with observational constraints 75
The Galaxy Velocity Field and Cold Dark Matter Models 74
Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes 74
Strong lensing efficiency of galaxy clusters in dark energy cosmologies 70
Numerical study of halo concentrations in dark-energy cosmologies 70
Testing students' ability to use derivatives, integrals, and vectors in a purely mathematical context and in a physical context 70
A merger tree with microsolar mass resolution: application to gamma-ray emission from subhalo population 69
Comparing the temperatures of galaxy clusters from hydrodynamical N-body simulations to Chandra and XMM-Newton observations 67
Adding long-wavelength modes to an N-body simulation 66
The satellite population of the Milky Way in a Lambda CDM universe 66
RECALIBRATION OF THE H(-0.5)-MAGNITUDES OF SPIRAL GALAXIES 58
The shapes of BCGs and normal ellipticals in nearby clusters. 55
Formation times, mass growth histories and concentrations of dark matter haloes 54
A look into the inside of haloes: A characterization of the halo shape as a function of overdensity in the Planck cosmology 50
Populating a cluster of galaxies - I. Results at z=0 46
Derivatives, integrals and vectors in introductory mechanics: the development of a multi-representation test for university students 46
Modelling the shapes of the largest gravitationally bound objects 44
Dynamical evolution of the ICM 39
Le esperienze sul campo: la testimonianza dei docenti 36
Developing a Modern Physics curriculum: a collaborative training course for in-service teachers 35
Assessment of students' understandings about the use of mathematical concepts in mechanics: results of the FisicaMente test 35
FisicaMente: supporting first-year students in transferring mathematical skills and knowledge to a physical context. 32
Dynamics of stellar black holes in young star clusters with different metallicities - II. Black hole-black hole binaries 16
Hydrodynamic Simulations of Galaxy Formation 12
Totale 5.980
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Categoria #
all - tutte 19.989
article - articoli 18.834
book - libri 0
conference - conferenze 0
curatela - curatele 0
other - altro 176
patent - brevetti 0
selected - selezionate 0
volume - volumi 123
Totale 39.122
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Totale Lug Ago Sett Ott Nov Dic Gen Feb Mar Apr Mag Giu
2018/2019554 0 0 0 0 0 0 0 0 0 126 237 191
2019/20201.293 174 28 26 99 131 112 119 161 123 163 110 47
2020/20211.208 39 58 11 81 121 219 61 57 304 50 132 75
2021/20221.039 39 90 208 37 49 81 57 77 69 35 122 175
2022/2023555 161 34 17 34 94 73 0 44 66 4 19 9
2023/2024255 17 36 42 30 26 54 15 22 8 5 0 0
Totale 5.980