CRIS Current Research Information System

VAZZA, FRANCO
 Distribuzione geografica
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Continente #
NA - Nord America 7.557
AS - Asia 6.172
EU - Europa 5.761
SA - Sud America 414
AF - Africa 373
OC - Oceania 10
Continente sconosciuto - Info sul continente non disponibili 2
Totale 20.289
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Nazione #
US - Stati Uniti d'America 7.446
SG - Singapore 1.971
GB - Regno Unito 1.859
CN - Cina 1.805
IT - Italia 1.029
VN - Vietnam 897
DE - Germania 682
HK - Hong Kong 605
SE - Svezia 557
FR - Francia 393
IN - India 352
BR - Brasile 304
RU - Federazione Russa 258
KR - Corea 254
IE - Irlanda 183
FI - Finlandia 176
CI - Costa d'Avorio 143
NL - Olanda 112
ZA - Sudafrica 94
UA - Ucraina 87
EE - Estonia 74
TG - Togo 71
CA - Canada 66
ID - Indonesia 65
JO - Giordania 60
JP - Giappone 55
AR - Argentina 54
AT - Austria 51
BG - Bulgaria 49
PL - Polonia 48
MX - Messico 37
BE - Belgio 29
GR - Grecia 28
NG - Nigeria 26
SC - Seychelles 25
TR - Turchia 25
RO - Romania 23
ES - Italia 21
HR - Croazia 21
HU - Ungheria 17
BD - Bangladesh 16
CZ - Repubblica Ceca 14
CH - Svizzera 13
EC - Ecuador 13
CO - Colombia 12
IR - Iran 12
CL - Cile 11
AU - Australia 9
IQ - Iraq 7
LB - Libano 7
LU - Lussemburgo 7
EG - Egitto 6
PE - Perù 6
PT - Portogallo 6
IL - Israele 5
UY - Uruguay 5
UZ - Uzbekistan 5
AE - Emirati Arabi Uniti 4
AL - Albania 4
LT - Lituania 4
MA - Marocco 4
DK - Danimarca 3
LV - Lettonia 3
MD - Moldavia 3
PH - Filippine 3
PK - Pakistan 3
PY - Paraguay 3
TH - Thailandia 3
TW - Taiwan 3
VE - Venezuela 3
AZ - Azerbaigian 2
BA - Bosnia-Erzegovina 2
BH - Bahrain 2
DO - Repubblica Dominicana 2
GY - Guiana 2
HT - Haiti 2
JM - Giamaica 2
KE - Kenya 2
MY - Malesia 2
SA - Arabia Saudita 2
A2 - ???statistics.table.value.countryCode.A2??? 1
AM - Armenia 1
BO - Bolivia 1
BY - Bielorussia 1
BZ - Belize 1
EU - Europa 1
HN - Honduras 1
KW - Kuwait 1
KZ - Kazakistan 1
MK - Macedonia 1
MM - Myanmar 1
NO - Norvegia 1
NP - Nepal 1
NZ - Nuova Zelanda 1
OM - Oman 1
PS - Palestinian Territory 1
RE - Reunion 1
RS - Serbia 1
SK - Slovacchia (Repubblica Slovacca) 1
SN - Senegal 1
Totale 20.289
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Città #
Southend 1.558
Singapore 1.282
Ashburn 921
Fairfield 814
Hong Kong 603
Hefei 493
Chandler 491
Bologna 390
Woodbridge 379
Dallas 331
Santa Clara 320
Houston 315
Wilmington 305
Seattle 304
Cambridge 281
Seoul 251
Ho Chi Minh City 247
Princeton 237
Ann Arbor 236
Beijing 221
Hanoi 194
Boardman 178
Dublin 178
Abidjan 143
Los Angeles 125
Munich 102
Berlin 92
Lappeenranta 92
Westminster 91
Dong Ket 85
Nanjing 84
Turin 77
Lomé 71
Redondo Beach 68
Padova 64
Helsinki 61
San Diego 61
Amman 60
San Jose 60
Jinan 57
Bengaluru 55
Jakarta 54
Milan 53
Buffalo 52
Shenyang 50
Saint Petersburg 49
Sofia 48
São Paulo 48
Tokyo 43
Chicago 42
Redmond 40
Modena 39
Frankfurt am Main 38
Phoenix 38
Tongling 37
Fremont 36
New York 36
Nuremberg 36
Rome 35
Guangzhou 33
Norwalk 33
Warsaw 33
London 32
Medford 32
Vienna 31
Mcallen 30
Haiphong 29
Hebei 29
Nanchang 29
Shanghai 28
Falls Church 27
Redwood City 27
Changsha 26
Des Moines 26
Tianjin 26
Jiaxing 24
Abeokuta 23
Orem 23
Ninh Bình 22
Washington 22
Zhengzhou 22
Brussels 21
Dearborn 21
Hangzhou 21
Turku 21
Da Nang 20
Slough 19
Brooklyn 18
Curitiba 18
Falkenstein 18
Paris 18
Montreal 17
Montréal 17
Quận Bình Thạnh 17
Biên Hòa 16
San Francisco 16
The Dalles 16
Chennai 15
Yubileyny 15
Toronto 14
Totale 13.696
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Nome #
LOFAR discovery of radio emission in MACSJ0717.5+3745 396
The turbulent pressure support in galaxy clusters revisited 328
The Quantitative Comparison Between the Neuronal Network and the Cosmic Web 269
A comparison of cosmological codes: Properties of thermal gas and shock waves in large-scale structures 253
A LOFAR study of non-merging massive galaxy clusters 251
Gas clumping in galaxy clusters 247
The mixing and transport properties of the intra cluster medium: A numerical study using tracers particles 242
The scatter in the radial profiles of X-ray luminous galaxy clusters as diagnostic of the thermodynamical state of the ICM 239
The coma cluster at low frequency array frequencies. I. Insights into particle acceleration mechanisms in the radio bridge 227
Fundamental physics with the Square Kilometre Array 223
How complex is the cosmic web? 207
Non-thermal pressure support in X-COP galaxy clusters 204
The Northern Cross fast radio burst project – I. Overview and pilot observations at 408 MHz 198
The gas distribution in the outer regions of galaxy clusters 193
Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample 191
A radio ridge connecting two galaxy clusters in a filament of the cosmic web 189
A new double radio relic in PSZ1 G096.89+24.17 and a radio relic mass-luminosity relation 188
A shock front at the radio relic of Abell 2744 185
New mysteries and challenges from the Toothbrush relic: wideband observations from 550 MHz to 8 GHz 182
Second-order Fermi Reacceleration Mechanisms and Large-Scale Synchrotron Radio Emission in Intracluster Bridges 182
Sardinia Radio Telescope observations of Abell 194: The intra-cluster magnetic field power spectrum 181
The challenge of detecting intracluster filaments with Faraday rotation 177
Resolved magnetic dynamo action in the simulated intracluster medium 174
Physical insights from the spectrum of the radio halo in MACS J0717.5+3745 170
Observations of the galaxy cluster CIZA J2242.8+5301 with the Sardinia Radio Telescope 167
Understanding the radio relic emission in the galaxy cluster MACS J0717.5+3745: Spectral analysis 164
Simulations and observational tests of primordial magnetic fields from Cosmic Microwave Background constraints 163
Enhancing the Spectral Hardening of Cosmic TeV Photons by Mixing with Axionlike Particles in the Magnetized Cosmic Web 162
Shocks and Non-thermal Particles in Clusters of Galaxies 162
Detecting shocked intergalactic gas with X-ray and radio observations 160
Deep learning based detection of cosmological diffuse radio sources 158
Spectro-polarimetric observations of the CIZA J2242.8+5301 northern radio relic: no evidence of high-frequency steepening 158
Forecasts for the detection of the magnetised cosmic web from cosmological simulations 156
Particle re-acceleration and Faraday-complex structures in the RXC J1314.4-2515 galaxy cluster 156
Probing the origin of extragalactic magnetic fields with Fast Radio Bursts 155
Massive and refined: A sample of large galaxy clusters simulated at high resolution. I: Thermal gas and properties of shock waves 154
Modelling injection and feedback of cosmic rays in grid-based cosmological simulations: Effects on cluster outskirts 154
Simulations of extragalactic magnetic fields and of their observables 153
Magnetic fields and relativistic electrons fill entire galaxy cluster 152
Turbulence and vorticity in Galaxy clusters generated by structure formation 150
Discovering the most elusive radio relic in the sky: Diffuse shock acceleration caught in the act? 150
Convolutional deep denoising autoencoders for radio astronomical images 150
Magnetogenesis and the cosmic web: A joint challenge for radio observations and numerical simulations 150
On the Connection between Turbulent Motions and Particle Acceleration in Galaxy Clusters 145
A survey of the thermal and non-thermal properties of cosmic filaments 145
Unravelling the origin of large-scale magnetic fields in galaxy clusters and beyond through Faraday Rotation Measures with the SKA 142
Abell 746: A Highly Disturbed Cluster Undergoing Multiple Mergers 141
A perfect power-law spectrum even at the highest frequencies: The Toothbrush relic 141
Evolution of vorticity and enstrophy in the intracluster medium 141
Radio haloes in Sunyaev-Zel'dovich-selected clusters of galaxies: The making of a halo? 140
Constraining magnetic fields in galaxy clusters 140
Turbulent magnetic fields in the merging galaxy cluster MACS J0717.5+3745 140
Deep low-frequency radio observations of Abell 2256. II. The ultra-steep spectrum radio halo 139
Do radio relics challenge diffusive shock acceleration? 139
Fast radio burst dispersion measures and rotation measures and the origin of intergalactic magnetic fields 138
Polarized accretion shocks from the cosmic web 137
Efficiency of Turbulent Reacceleration by Solenoidal Turbulence and Its Application to the Origin of Radio Megahalos in Cluster Outskirts 137
Thermal and non-thermal traces of agn feedback: Results from cosmological amr simulations 137
Morphology of radio relics-I. What causes the substructure of synchrotron emission? 137
Dissecting nonthermal emission in the complex multiple-merger galaxy cluster Abell 2744: Radio and X-ray analysis 137
Constraining the efficiency of cosmic ray acceleration by cluster shocks 136
Analytical model for cluster radio relics 136
Turbulence in the ICM from mergers, cool-core sloshing, and jets: Results from a new multi-scale filtering approach 135
The X-ray/SZ view of the virial region: II. Gas mass fraction 134
Numerical cosmology on the GPU with Enzo and Ramses 134
The thermal and non-thermal components within and between galaxy clusters Abell 399 and Abell 401 133
Why are central radio relics so rare? 133
Simulations of cosmic rays in large-scale structures: Numerical and physical effects 132
Propagation of ultrahigh energy cosmic rays in extragalactic magnetic fields: A view from cosmological simulations 131
The Coma Cluster at LOFAR Frequencies. II. the Halo, Relic, and a New Accretion Relic 130
Turbulence in the Intracluster Medium 130
New filamentary remnant radio emission and duty cycle constraints in the radio galaxy NGC 6086 129
Discovery of radio haloes and double relics in distant MACS galaxy clusters: clues to the efficiency of particle acceleration 129
The entropy core in galaxy clusters: Numerical and physical effects in cosmological grid simulations 129
The intracluster magnetic field in the double relic galaxy cluster Abell 2345 129
Measurements and simulation of Faraday rotation across the Coma radio relic 128
Simulations of ultra-high energy cosmic rays in the local Universe and the origin of cosmic magnetic fields 128
ALMA-SZ DETECTION of A GALAXY CLUSTER MERGER SHOCK at HALF the AGE of the UNIVERSE 127
Magnetic Field Amplification in Galaxy Clusters and Its Simulation 127
On the alignment of haloes, filaments and magnetic fields in the simulated cosmic web 127
Magnetic field evolution in cosmic filaments with LOFAR data 126
Turbulent gas motions in galaxy cluster simulations: The role of smoothed particle hydrodynamics viscosity 124
Galaxy clusters enveloped by vast volumes of relativistic electrons 123
Turbulent pressure support and hydrostatic mass-bias in the intracluster medium 123
An intergalactic medium temperature from a giant radio galaxy 122
Electron and proton acceleration efficiency by merger shocks in galaxy clusters 122
Constraints on the magnetic field in the intercluster bridge A399- A401 121
Studying the Effect of Shock Obliquity on the γ-ray and Diffuse Radio Emission in Galaxy Clusters 121
Polarization of radio relics in galaxy clusters 120
On the amplification of magnetic fields in cosmic filaments and galaxy clusters 119
On the Non-Thermal Energy Content of Cosmic Structures 119
New constraints on the magnetization of the cosmic web using LOFAR Faraday rotation observations 119
New constraints on the magnetic field in cosmic web filaments 119
Radio relics radio emission from ltishock scenario 119
The Complexity and Information Content of Simulated Universes 119
Shock waves in Eulerian cosmological simulations: Main properties and acceleration of cosmic rays 118
On the complexity and the information content of cosmic structures 118
Joint inference on the redshift distribution of fast radio burst and on the intergalactic baryon content 118
Properties of cosmological filaments extracted from Eulerian simulations 117
Voyage through the hidden physics of the cosmic web 117
Totale 15.667
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Categoria #
all - tutte 59.982
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 59.982
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Totale Lug Ago Sett Ott Nov Dic Gen Feb Mar Apr Mag Giu
2020/20211.190 0 0 0 0 0 0 148 240 156 239 61 346
2021/20222.464 177 90 178 108 261 123 122 274 259 137 377 358
2022/20232.691 244 424 222 333 152 177 115 145 501 104 189 85
2023/2024782 42 117 42 49 83 121 49 45 14 132 25 63
2024/20253.713 124 471 245 294 530 251 249 141 78 163 273 894
2025/20265.291 1.204 964 1.064 604 820 497 138 0 0 0 0 0
Totale 20.900