CRIS Current Research Information System

VAZZA, FRANCO
 Distribuzione geografica
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Continente #
NA - Nord America 6.005
EU - Europa 4.957
AS - Asia 1.774
AF - Africa 238
SA - Sud America 41
OC - Oceania 9
Continente sconosciuto - Info sul continente non disponibili 2
Totale 13.026
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Nazione #
US - Stati Uniti d'America 5.962
GB - Regno Unito 1.808
IT - Italia 906
CN - Cina 690
SE - Svezia 551
SG - Singapore 537
DE - Germania 511
FR - Francia 345
IN - India 264
IE - Irlanda 181
RU - Federazione Russa 138
VN - Vietnam 112
FI - Finlandia 91
UA - Ucraina 83
ZA - Sudafrica 74
EE - Estonia 73
TG - Togo 70
CI - Costa d'Avorio 65
JO - Giordania 56
ID - Indonesia 51
BG - Bulgaria 48
CA - Canada 37
BR - Brasile 32
BE - Belgio 28
GR - Grecia 28
NG - Nigeria 23
PL - Polonia 22
HR - Croazia 21
NL - Olanda 20
AT - Austria 19
TR - Turchia 19
HU - Ungheria 17
ES - Italia 14
CH - Svizzera 12
CZ - Repubblica Ceca 11
IR - Iran 11
RO - Romania 9
AU - Australia 8
JP - Giappone 8
LU - Lussemburgo 7
LB - Libano 6
IL - Israele 5
CL - Cile 4
MX - Messico 4
SC - Seychelles 4
DK - Danimarca 3
HK - Hong Kong 3
KR - Corea 3
PT - Portogallo 3
TW - Taiwan 3
CO - Colombia 2
LV - Lettonia 2
MD - Moldavia 2
UZ - Uzbekistan 2
A2 - ???statistics.table.value.countryCode.A2??? 1
AR - Argentina 1
BY - Bielorussia 1
BZ - Belize 1
EC - Ecuador 1
EG - Egitto 1
EU - Europa 1
JM - Giamaica 1
MA - Marocco 1
MY - Malesia 1
NO - Norvegia 1
NZ - Nuova Zelanda 1
PE - Perù 1
PH - Filippine 1
RS - Serbia 1
SA - Arabia Saudita 1
SK - Slovacchia (Repubblica Slovacca) 1
TH - Thailandia 1
Totale 13.026
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Città #
Southend 1.558
Fairfield 814
Ashburn 513
Singapore 497
Chandler 494
Woodbridge 379
Bologna 361
Houston 312
Santa Clara 306
Wilmington 305
Seattle 292
Cambridge 281
Princeton 237
Ann Arbor 236
Dublin 177
Boardman 176
Berlin 92
Westminster 91
Dong Ket 85
Nanjing 83
Turin 75
Lomé 70
Lappeenranta 66
Abidjan 65
Padova 62
San Diego 61
Jinan 57
Amman 56
Jakarta 51
Saint Petersburg 49
Shenyang 48
Sofia 48
Milan 46
Modena 40
Redmond 40
Fremont 36
Norwalk 33
Medford 32
Mcallen 30
Rome 30
Hebei 29
Nanchang 28
Falls Church 27
Redwood City 27
Beijing 26
Changsha 26
Des Moines 26
Guangzhou 26
Tianjin 26
Helsinki 24
Jiaxing 24
Abeokuta 23
Munich 23
Dearborn 21
Brussels 20
Phoenix 20
Washington 20
London 19
Los Angeles 19
Slough 19
Zhengzhou 19
Paris 18
Hangzhou 17
Montréal 17
Shanghai 17
Vienna 17
Baja 13
Warsaw 12
Fuzhou 11
Olalla 11
São Paulo 11
Toronto 11
Haikou 10
Curitiba 9
Jacksonville 9
Taizhou 9
Frankfurt am Main 8
New York 8
Rotherham 8
Shenzhen 8
Taiyuan 8
Wuhan 8
Bühl 7
Madrid 7
Rijeka 7
San Francisco 7
Chicago 6
Foshan 6
Frankfurt Am Main 6
Hesperange 6
Istanbul 6
Kesir 6
Kraainem 6
Krasnodar 6
Kunming 6
Langfang 6
Leawood 6
Münster 6
Ningbo 6
Ottawa 6
Totale 9.128
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Nome #
LOFAR discovery of radio emission in MACSJ0717.5+3745 361
The scatter in the radial profiles of X-ray luminous galaxy clusters as diagnostic of the thermodynamical state of the ICM 187
The coma cluster at low frequency array frequencies. I. Insights into particle acceleration mechanisms in the radio bridge 183
Fundamental physics with the Square Kilometre Array 179
How complex is the cosmic web? 173
The Quantitative Comparison Between the Neuronal Network and the Cosmic Web 173
A LOFAR study of non-merging massive galaxy clusters 168
A comparison of cosmological codes: Properties of thermal gas and shock waves in large-scale structures 164
Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample 161
Non-thermal pressure support in X-COP galaxy clusters 159
The gas distribution in the outer regions of galaxy clusters 158
The turbulent pressure support in galaxy clusters revisited 147
Resolved magnetic dynamo action in the simulated intracluster medium 145
Shocks and Non-thermal Particles in Clusters of Galaxies 142
The challenge of detecting intracluster filaments with Faraday rotation 140
Second-order Fermi Reacceleration Mechanisms and Large-Scale Synchrotron Radio Emission in Intracluster Bridges 140
The Northern Cross fast radio burst project – I. Overview and pilot observations at 408 MHz 139
Modelling injection and feedback of cosmic rays in grid-based cosmological simulations: Effects on cluster outskirts 136
Deep learning based detection of cosmological diffuse radio sources 135
A radio ridge connecting two galaxy clusters in a filament of the cosmic web 133
New mysteries and challenges from the Toothbrush relic: wideband observations from 550 MHz to 8 GHz 133
Sardinia Radio Telescope observations of Abell 194: The intra-cluster magnetic field power spectrum 132
Forecasts for the detection of the magnetised cosmic web from cosmological simulations 129
Enhancing the Spectral Hardening of Cosmic TeV Photons by Mixing with Axionlike Particles in the Magnetized Cosmic Web 129
Massive and refined: A sample of large galaxy clusters simulated at high resolution. I: Thermal gas and properties of shock waves 126
Simulations of extragalactic magnetic fields and of their observables 125
Probing the origin of extragalactic magnetic fields with Fast Radio Bursts 125
Simulations and observational tests of primordial magnetic fields from Cosmic Microwave Background constraints 125
Detecting shocked intergalactic gas with X-ray and radio observations 122
Observations of the galaxy cluster CIZA J2242.8+5301 with the Sardinia Radio Telescope 121
Do radio relics challenge diffusive shock acceleration? 120
Constraining the efficiency of cosmic ray acceleration by cluster shocks 120
A survey of the thermal and non-thermal properties of cosmic filaments 120
Turbulence and vorticity in Galaxy clusters generated by structure formation 117
Physical insights from the spectrum of the radio halo in MACS J0717.5+3745 115
Numerical cosmology on the GPU with Enzo and Ramses 114
Analytical model for cluster radio relics 114
Understanding the radio relic emission in the galaxy cluster MACS J0717.5+3745: Spectral analysis 114
The mixing and transport properties of the intra cluster medium: A numerical study using tracers particles 113
Thermal and non-thermal traces of agn feedback: Results from cosmological amr simulations 113
A shock front at the radio relic of Abell 2744 113
Turbulence in the ICM from mergers, cool-core sloshing, and jets: Results from a new multi-scale filtering approach 111
Propagation of ultrahigh energy cosmic rays in extragalactic magnetic fields: A view from cosmological simulations 111
Simulations of ultra-high energy cosmic rays in the local Universe and the origin of cosmic magnetic fields 110
On the Connection between Turbulent Motions and Particle Acceleration in Galaxy Clusters 110
Gas clumping in galaxy clusters 109
Fast radio burst dispersion measures and rotation measures and the origin of intergalactic magnetic fields 109
Spectro-polarimetric observations of the CIZA J2242.8+5301 northern radio relic: no evidence of high-frequency steepening 108
Turbulence in the Intracluster Medium 107
Particle re-acceleration and Faraday-complex structures in the RXC J1314.4-2515 galaxy cluster 106
A new double radio relic in PSZ1 G096.89+24.17 and a radio relic mass-luminosity relation 105
A perfect power-law spectrum even at the highest frequencies: The Toothbrush relic 105
The X-ray/SZ view of the virial region: II. Gas mass fraction 104
Radio haloes in Sunyaev-Zel'dovich-selected clusters of galaxies: The making of a halo? 104
Constraining magnetic fields in galaxy clusters 104
Discovering the most elusive radio relic in the sky: Diffuse shock acceleration caught in the act? 104
Evolution of vorticity and enstrophy in the intracluster medium 104
Why are central radio relics so rare? 103
Discovery of radio haloes and double relics in distant MACS galaxy clusters: clues to the efficiency of particle acceleration 102
ALMA-SZ DETECTION of A GALAXY CLUSTER MERGER SHOCK at HALF the AGE of the UNIVERSE 102
Magnetic Field Amplification in Galaxy Clusters and Its Simulation 101
On the Non-Thermal Energy Content of Cosmic Structures 99
Electron and proton acceleration efficiency by merger shocks in galaxy clusters 99
Unravelling the origin of large-scale magnetic fields in galaxy clusters and beyond through Faraday Rotation Measures with the SKA 99
Morphology of radio relics-I. What causes the substructure of synchrotron emission? 99
The intracluster magnetic field in the double relic galaxy cluster Abell 2345 98
Convolutional deep denoising autoencoders for radio astronomical images 98
Simulations of cosmic rays in large-scale structures: Numerical and physical effects 97
Turbulent gas motions in galaxy cluster simulations: The role of smoothed particle hydrodynamics viscosity 97
On the amplification of magnetic fields in cosmic filaments and galaxy clusters 96
Shock waves in Eulerian cosmological simulations: Main properties and acceleration of cosmic rays 95
The Complexity and Information Content of Simulated Universes 95
Turbulent magnetic fields in the merging galaxy cluster MACS J0717.5+3745 95
Testing cosmic ray acceleration with radio relics: A high-resolution study using MHD and tracers 94
Measurements and simulation of Faraday rotation across the Coma radio relic 94
Properties of cosmological filaments extracted from Eulerian simulations 94
Detecting the cosmic web with radio surveys 93
Magnetogenesis and the cosmic web: A joint challenge for radio observations and numerical simulations 93
Turbulent motions and shocks waves in galaxy clusters simulated with adaptive mesh refinement 92
Studying the Effect of Shock Obliquity on the γ-ray and Diffuse Radio Emission in Galaxy Clusters 92
On the complexity and the information content of cosmic structures 91
The entropy core in galaxy clusters: Numerical and physical effects in cosmological grid simulations 91
Influence of adaptive mesh refinement and the hydro solver on shear-induced mass stripping in a minor-merger scenario 90
Joint inference on the redshift distribution of fast radio burst and on the intergalactic baryon content 90
Polarization of radio relics in galaxy clusters 89
Turbulent velocity fields in smoothed particle hydrodymanics simulated galaxy clusters: Scaling laws for the turbulent energy 89
Combining X-Ray and SZ Observations to Characterize Cluster Outskirts: Current Work and Future Prospects 88
Massive and refined: II. the statistical properties of turbulent motions in massive galaxy clusters with high spatial resolution 87
Dissecting nonthermal emission in the complex multiple-merger galaxy cluster Abell 2744: Radio and X-ray analysis 86
Properties of gas clumps and gas clumping factor in the intra-cluster medium 85
Discovery of magnetic fields along stacked cosmic filaments as revealed by radio and X-ray emission 85
The X-ray/SZ view of the virial region: I. Thermodynamic properties 84
New constraints on the magnetization of the cosmic web using LOFAR Faraday rotation observations 84
null 83
The impact of the SZ effect on cm-wavelength (1-30 GHz) observations of galaxy cluster radio relics 82
Evolution of cosmic filaments and of their galaxy population from MHD cosmological simulations 81
New constraints on the magnetic field in cosmic web filaments 79
Shock waves in the magnetized cosmic web: the role of obliquity and cosmic ray acceleration 78
On the alignment of haloes, filaments and magnetic fields in the simulated cosmic web 78
Turbulent pressure support and hydrostatic mass-bias in the intracluster medium 77
Totale 11.498
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Categoria #
all - tutte 37.615
article - articoli 0
book - libri 0
conference - conferenze 0
curatela - curatele 0
other - altro 0
patent - brevetti 0
selected - selezionate 0
volume - volumi 0
Totale 37.615
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Totale Lug Ago Sett Ott Nov Dic Gen Feb Mar Apr Mag Giu
2019/20202.256 0 0 0 0 315 280 350 392 396 204 125 194
2020/20212.215 295 177 82 139 177 155 148 240 156 239 61 346
2021/20222.464 177 90 178 108 261 123 122 274 259 137 377 358
2022/20232.701 244 424 222 333 153 180 115 147 504 104 190 85
2023/2024794 42 118 42 49 83 121 49 45 14 143 25 63
2024/20251.670 125 471 250 294 530 0 0 0 0 0 0 0
Totale 13.588