IRIS
EVOLI, CARMELO
 Distribuzione geografica
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Continente #
EU - Europa 6.281
NA - Nord America 5.022
AS - Asia 2.941
SA - Sud America 364
Continente sconosciuto - Info sul continente non disponibili 155
AF - Africa 81
OC - Oceania 3
AN - Antartide 1
Totale 14.848
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Nazione #
US - Stati Uniti d'America 4.850
RU - Federazione Russa 4.775
SG - Singapore 933
CN - Cina 829
VN - Vietnam 385
IT - Italia 337
BR - Brasile 285
SE - Svezia 258
DE - Germania 210
HK - Hong Kong 208
BD - Bangladesh 176
UA - Ucraina 167
FR - Francia 137
GB - Regno Unito 113
KR - Corea 86
CA - Canada 85
TR - Turchia 79
IN - India 64
IE - Irlanda 61
MX - Messico 53
ES - Italia 40
CZ - Repubblica Ceca 38
PL - Polonia 37
ZA - Sudafrica 35
IQ - Iraq 32
JP - Giappone 32
NL - Olanda 32
FI - Finlandia 27
AR - Argentina 26
PK - Pakistan 15
PY - Paraguay 14
EC - Ecuador 13
IL - Israele 13
MA - Marocco 10
UZ - Uzbekistan 10
ID - Indonesia 9
AT - Austria 8
CL - Cile 8
EU - Europa 7
HN - Honduras 7
JO - Giordania 7
NP - Nepal 7
SA - Arabia Saudita 7
TN - Tunisia 7
AE - Emirati Arabi Uniti 6
CH - Svizzera 6
CO - Colombia 6
VE - Venezuela 6
BE - Belgio 5
CI - Costa d'Avorio 5
MY - Malesia 5
CR - Costa Rica 4
EG - Egitto 4
JM - Giamaica 4
RO - Romania 4
RS - Serbia 4
TT - Trinidad e Tobago 4
AL - Albania 3
AO - Angola 3
AU - Australia 3
AZ - Azerbaigian 3
BS - Bahamas 3
GE - Georgia 3
GT - Guatemala 3
IR - Iran 3
KE - Kenya 3
LB - Libano 3
NG - Nigeria 3
BB - Barbados 2
BH - Bahrain 2
BO - Bolivia 2
DK - Danimarca 2
DZ - Algeria 2
GR - Grecia 2
KG - Kirghizistan 2
LT - Lituania 2
LU - Lussemburgo 2
MD - Moldavia 2
MN - Mongolia 2
NI - Nicaragua 2
PH - Filippine 2
PS - Palestinian Territory 2
PT - Portogallo 2
TH - Thailandia 2
TW - Taiwan 2
UY - Uruguay 2
AF - Afghanistan, Repubblica islamica di 1
AM - Armenia 1
AQ - Antartide 1
AW - Aruba 1
BF - Burkina Faso 1
BN - Brunei Darussalam 1
BY - Bielorussia 1
CG - Congo 1
CW - ???statistics.table.value.countryCode.CW??? 1
CY - Cipro 1
DJ - Gibuti 1
GA - Gabon 1
GD - Grenada 1
GN - Guinea 1
Totale 14.678
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Città #
Moscow 1.213
Council Bluffs 894
Ashburn 470
Singapore 462
San Jose 445
Chandler 346
Boardman 339
Hong Kong 192
San Mateo 184
New York 167
The Dalles 159
Los Angeles 156
Chicago 114
Beijing 112
Dong Ket 100
Ho Chi Minh City 92
Milan 92
Lauterbourg 90
Seoul 86
Shanghai 85
Dallas 82
Hefei 82
Kitzingen 73
Phoenix 73
Hanoi 72
Istanbul 65
Dublin 60
Santa Clara 55
Turin 54
Munich 46
Orem 43
São Paulo 42
Ogden 41
Montreal 37
Brno 34
Seattle 33
Stockholm 32
Warsaw 31
Tokyo 29
Atlanta 27
Johannesburg 27
Houston 26
Poplar 25
Mexico City 23
Rome 23
Amsterdam 22
Ann Arbor 22
Denver 22
Frankfurt am Main 22
Guangzhou 21
West Jordan 20
Wilmington 20
Brooklyn 19
London 19
Helsinki 18
Toronto 18
Da Nang 17
Strasbourg 17
Boston 16
Central 16
Manchester 16
Chennai 15
Buffalo 14
L'aquila 13
Shenzhen 13
León 12
San Francisco 12
Mumbai 11
Dhaka 10
New Delhi 10
Tashkent 10
Asunción 9
Haiphong 9
Las Vegas 9
Querétaro 9
Turku 9
Vancouver 9
Baghdad 8
Belo Horizonte 8
Berlin 8
Erbil 8
Hải Dương 8
Kyiv 8
Wuxi 8
Amman 7
Columbus 7
Dongguan 7
Edinburgh 7
Jiaxing 7
Naples 7
Ankara 6
Florence 6
Jerusalem 6
L’Aquila 6
Miami 6
Milwaukee 6
Porto Alegre 6
Pune 6
Quito 6
Augusta 5
Totale 7.569
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Nome #
A consistent interpretation of recent CR nuclei and electron spectra 243
AMS-02 beryllium data and its implication for cosmic ray transport 228
A Combined Interpretation of CR Nuclei and Antiproton High Energy Measurements 228
A combined interpretation of cosmic ray light nuclei and antiproton measurements 219
Atmospheric neutrinos and the knee of the cosmic ray spectrum 215
Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation 205
Demonstrating Agreement between Radio and Fluorescence Measurements of the Depth of Maximum of Extensive Air Showers at the Pierre Auger Observatory 197
Radio measurements of the depth of air-shower maximum at the Pierre Auger Observatory 193
Cosmic-ray antinuclei as messengers of new physics: status and outlook for the new decade 191
Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory 191
Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants 189
Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory 188
Galactic factories of cosmic-ray electrons and positrons 183
Constraints on dark matter annihilations from diffuse gamma-ray emission in the Galaxy 180
Blazar VHE spectral alterations induced by photon-ALP oscillations 178
An alternative solution to the gamma-ray Gradient problem 178
Search for photons above 1018 eV by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory 177
Antiprotons from dark matter annihilation in the Galaxy: Astrophysical uncertainties 177
AugerPrime surface detector electronics 175
Galactic cosmic rays after the AMS-02 observations 174
Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory 172
A signature of anisotropic cosmic-ray transport in the gamma-ray sky 169
Constraining warm dark matter with high-z supernova lensing 168
Cosmic ray electrons, positrons and the synchrotron emission of the Galaxy: consistent analysis and implications 167
Expectations for high energy diffuse galactic neutrinos for different cosmic ray distributions 167
A unified solution to the anisotropy and gradient problems 166
Common Solution to the Cosmic Ray Anisotropy and Gradient Problems 164
Radial distribution of the diffuse gamma-ray emissivity in the Galactic disk 164
Origin of the Cosmic Ray Galactic Halo Driven by Advected Turbulence and Self-Generated Waves 162
Cosmogenic neutrinos and gamma-rays and the redshift evolution of UHECR sources 160
Cosmic microwave background constraints on light dark matter candidates 160
Novel aspects of cosmic ray diffusion in synthetic magnetic turbulence 157
Simulating the Galactic multi-messenger emissions with HERMES 157
Cosmic ray nuclei, antiprotons and gamma rays in the galaxy: a new diffusion model 156
Cosmic Ray Propagation in Galactic Turbulence 154
Signature of Energy Losses on the Cosmic Ray Electron Spectrum 154
Two phase galaxy formation: the gas content of normal galaxies 153
PAMELA and AMS-02 e+ and e- spectra are reproduced by three-dimensional cosmic-ray modeling 148
Cosmic-ray propagation with DRAGON2: II. Nuclear interactions with the interstellar gas 146
Intermediate-mass and heavy Galactic cosmic-ray nuclei: The case of new AMS-02 measurements 146
TeV halos and the role of pulsar wind nebulae as sources of cosmic-ray positrons 145
Self-generated cosmic-ray confinement in TeV halos: Implications for TeV γ -ray emission and the positron excess 144
Diffuse gamma emission of the Galaxy from cosmic rays 144
Two-phase galaxy formation: the evolutionary properties of galaxies 143
Turbulence in the intergalactic medium 143
Dark Matter effects on high-redshift universe 143
The HI content of local late-type galaxies 143
Cosmic-ray propagation with DRAGON2: I. numerical solver and astrophysical ingredients 142
Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre 142
Diffuse galactic gamma rays at intermediate and high latitudes. I. Constraints on the ISM properties 141
Impact of the magnetic horizon on the interpretation of the Pierre Auger Observatory spectrum and composition data 140
Unified interpretation of cosmic ray nuclei and antiproton recent measurements 139
Implications of the cosmic ray electron spectrum and anisotropy measured with Fermi-LAT 139
Stochastic nature of Galactic cosmic-ray sources 139
Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory 138
Energy deposition by weakly interacting massive particles: a comprehensive study 138
Galactic electron and positron properties from cosmic ray and radio observations 138
The origin of Galactic cosmic rays: Challenges to the standard paradigm 138
Unveiling the nature of dark matter with high redshift 21 cm line experiments 137
Testing hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory 136
Do cosmic rays heat the early intergalactic medium? 136
The puzzling origin of the Li-6 plateau 136
Diffuse neutrino and gamma-ray emissions of the galaxy above the TeV 135
AugerPrime surface detector electronics 134
Three-Dimensional Model of Cosmic-Ray Lepton Propagation Reproduces Data from the Alpha Magnetic Spectrometer on the International Space Station 133
Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles 133
Discovery of the supernova remnant G351.0-5.4 132
Diffuse Galactic Gamma Rays at Intermediate and High Latitudes, Constraints on ISM Properties 132
Ground observations of a space laser for the assessment of its in-orbit performance 131
Gamma-ray and neutrino diffuse emission of the Galaxy above the TeV 131
Simulating intergalactic quasar scintillation 130
The Galactic Center GeV excess from a series of leptonic cosmic-ray outbursts 130
The Pierre Auger Observatory: Contributions to the 39th International Cosmic Ray Conference (ICRC 2025) 128
Scaler Rates from the Pierre Auger Observatory: A New Proxy of Solar Activity 128
CRPropa: A public framework to propagate UHECRs in the universe 127
Cosmic ray propagation with CRPropa 3 127
Inference of the Mass Composition of Cosmic Rays with Energies from 1018.5 to 1020  eV Using the Pierre Auger Observatory and Deep Learning 126
Cosmic Ray propagation in the Galaxy and diffuse gamma-ray emission 126
Measurement of the depth of maximum of air-shower profiles with energies between 1018.5 and 1020  eV using the surface detector of the Pierre Auger Observatory and deep learning 125
Galactic diffuse gamma rays meet the PeV frontier 124
Secondary antiprotons as a Galactic Dark Matter probe 123
Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory 122
The Pierre Auger Observatory open data 122
Reionization during the dark ages from a cosmic axion background 122
The Distribution of Ultrahigh-energy Cosmic Rays along the Supergalactic Plane Measured at the Pierre Auger Observatory 121
Three dimensional modeling of CR propagation 121
Turbulent axion-photon conversions in the Milky Way 121
Search for a diffuse flux of photons with energies above tens of PeV at the Pierre Auger Observatory 120
Particle energy cascade in the intergalactic medium 119
Quasi‐Constant Time Gap in Multiple Rings of Elves 118
The scintillator surface detector of the Pierre Auger observatory 117
The nature of dark matter from the global high-redshift H I 21 cm signal 114
Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory 113
Demonstrating Agreement between Radio and Fluorescence Measurements of the Depth of Maximum of Extensive Air Showers at the Pierre Auger Observatory 112
Diffuse synchrotron emission from galactic cosmic ray electrons 112
Prospects for γ-ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array 111
Radio measurements of the depth of air-shower maximum at the Pierre Auger Observatory 109
Testing hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory 106
CRPropa 3.0 - a Public Framework for Propagating UHE Cosmic Rays through Galactic and Extragalactic Space 106
The origin of very high-energy diffuse γ-ray emission: The case for galactic source cocoons 83
Totale 14.807
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Categoria #
all - tutte 70.096
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 70.096
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Totale Lug Ago Sett Ott Nov Dic Gen Feb Mar Apr Mag Giu
2021/2022430 0 0 31 282 28 2 5 0 7 53 5 17
2022/2023922 1 2 8 131 125 133 59 146 157 41 116 3
2023/2024683 12 12 132 14 21 79 30 82 2 132 123 44
2024/20251.699 51 203 235 127 95 135 141 58 118 133 256 147
2025/20269.775 510 309 141 741 834 5.017 712 238 315 255 320 383
2026/2027927 249 384 294 0 0 0 0 0 0 0 0 0
Totale 14.848