IRIS
EVOLI, CARMELO
 Distribuzione geografica
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Continente #
EU - Europa 6.198
NA - Nord America 3.632
AS - Asia 2.729
SA - Sud America 348
AF - Africa 80
Continente sconosciuto - Info sul continente non disponibili 9
OC - Oceania 3
AN - Antartide 1
Totale 13.000
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Nazione #
RU - Federazione Russa 4.775
US - Stati Uniti d'America 3.490
SG - Singapore 888
CN - Cina 808
VN - Vietnam 384
BR - Brasile 273
IT - Italia 265
SE - Svezia 257
DE - Germania 210
HK - Hong Kong 204
UA - Ucraina 167
FR - Francia 136
GB - Regno Unito 108
KR - Corea 84
TR - Turchia 78
CA - Canada 68
IN - India 63
IE - Irlanda 61
MX - Messico 50
BD - Bangladesh 48
ES - Italia 39
CZ - Repubblica Ceca 38
PL - Polonia 37
ZA - Sudafrica 35
IQ - Iraq 31
JP - Giappone 30
NL - Olanda 30
FI - Finlandia 27
AR - Argentina 24
PK - Pakistan 15
PY - Paraguay 14
IL - Israele 13
EC - Ecuador 12
UZ - Uzbekistan 10
MA - Marocco 9
AT - Austria 8
ID - Indonesia 8
CL - Cile 7
EU - Europa 7
JO - Giordania 7
SA - Arabia Saudita 7
TN - Tunisia 7
CH - Svizzera 6
CO - Colombia 6
HN - Honduras 6
NP - Nepal 6
VE - Venezuela 6
AE - Emirati Arabi Uniti 5
BE - Belgio 5
CI - Costa d'Avorio 5
EG - Egitto 4
MY - Malesia 4
RS - Serbia 4
AL - Albania 3
AO - Angola 3
AU - Australia 3
AZ - Azerbaigian 3
BS - Bahamas 3
CR - Costa Rica 3
GE - Georgia 3
IR - Iran 3
KE - Kenya 3
LB - Libano 3
NG - Nigeria 3
RO - Romania 3
BO - Bolivia 2
DK - Danimarca 2
DZ - Algeria 2
GR - Grecia 2
GT - Guatemala 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
TT - Trinidad e Tobago 2
TW - Taiwan 2
UY - Uruguay 2
AF - Afghanistan, Repubblica islamica di 1
AQ - Antartide 1
BB - Barbados 1
BF - Burkina Faso 1
BH - Bahrain 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
GY - Guiana 1
HR - Croazia 1
HT - Haiti 1
Totale 12.978
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Città #
Moscow 1.213
Singapore 461
Ashburn 401
Chandler 346
San Jose 345
Boardman 339
Hong Kong 188
San Mateo 184
The Dalles 159
New York 148
Los Angeles 140
Beijing 109
Chicago 107
Dong Ket 100
Ho Chi Minh City 92
Lauterbourg 90
Shanghai 85
Seoul 84
Hefei 82
Milan 82
Kitzingen 73
Dallas 72
Hanoi 71
Istanbul 65
Dublin 60
Turin 53
Munich 46
Ogden 41
Orem 41
São Paulo 41
Brno 34
Montreal 32
Stockholm 31
Warsaw 31
Johannesburg 27
Tokyo 27
Santa Clara 26
Seattle 26
Poplar 25
Houston 23
Ann Arbor 22
Atlanta 22
Denver 22
Frankfurt am Main 22
Guangzhou 21
Mexico City 21
Amsterdam 20
West Jordan 20
Wilmington 20
Brooklyn 19
London 19
Helsinki 18
Da Nang 17
Strasbourg 17
Boston 16
Central 16
Manchester 16
Chennai 15
Phoenix 15
Rome 15
Toronto 14
L'aquila 13
Shenzhen 13
León 12
Council Bluffs 10
Dhaka 10
Mumbai 10
New Delhi 10
San Francisco 10
Tashkent 10
Asunción 9
Haiphong 9
Querétaro 9
Turku 9
Vancouver 9
Baghdad 8
Belo Horizonte 8
Berlin 8
Erbil 8
Hải Dương 8
Kyiv 8
Las Vegas 8
Wuxi 8
Amman 7
Columbus 7
Dongguan 7
Edinburgh 7
Jiaxing 7
Ankara 6
Buffalo 6
Jerusalem 6
L’Aquila 6
Porto Alegre 6
Pune 6
Quito 6
Bonndorf 5
Brasília 5
Goiânia 5
Milwaukee 5
Philadelphia 5
Totale 6.296
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Nome #
A consistent interpretation of recent CR nuclei and electron spectra 227
AMS-02 beryllium data and its implication for cosmic ray transport 215
A Combined Interpretation of CR Nuclei and Antiproton High Energy Measurements 209
Atmospheric neutrinos and the knee of the cosmic ray spectrum 203
A combined interpretation of cosmic ray light nuclei and antiproton measurements 203
Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation 189
Cosmic-ray antinuclei as messengers of new physics: status and outlook for the new decade 179
Demonstrating Agreement between Radio and Fluorescence Measurements of the Depth of Maximum of Extensive Air Showers at the Pierre Auger Observatory 172
Galactic factories of cosmic-ray electrons and positrons 170
Blazar VHE spectral alterations induced by photon-ALP oscillations 169
Constraints on dark matter annihilations from diffuse gamma-ray emission in the Galaxy 166
Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants 165
Antiprotons from dark matter annihilation in the Galaxy: Astrophysical uncertainties 162
An alternative solution to the gamma-ray Gradient problem 162
Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory 159
Galactic cosmic rays after the AMS-02 observations 159
A signature of anisotropic cosmic-ray transport in the gamma-ray sky 159
Radio measurements of the depth of air-shower maximum at the Pierre Auger Observatory 156
Expectations for high energy diffuse galactic neutrinos for different cosmic ray distributions 156
AugerPrime surface detector electronics 154
Constraining warm dark matter with high-z supernova lensing 153
Search for photons above 1018 eV by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory 152
Cosmic ray electrons, positrons and the synchrotron emission of the Galaxy: consistent analysis and implications 149
Origin of the Cosmic Ray Galactic Halo Driven by Advected Turbulence and Self-Generated Waves 148
Common Solution to the Cosmic Ray Anisotropy and Gradient Problems 148
Radial distribution of the diffuse gamma-ray emissivity in the Galactic disk 148
Cosmic microwave background constraints on light dark matter candidates 145
Simulating the Galactic multi-messenger emissions with HERMES 144
Cosmogenic neutrinos and gamma-rays and the redshift evolution of UHECR sources 143
Cosmic Ray Propagation in Galactic Turbulence 143
Cosmic ray nuclei, antiprotons and gamma rays in the galaxy: a new diffusion model 143
Signature of Energy Losses on the Cosmic Ray Electron Spectrum 143
Novel aspects of cosmic ray diffusion in synthetic magnetic turbulence 142
Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory 141
PAMELA and AMS-02 e+ and e- spectra are reproduced by three-dimensional cosmic-ray modeling 137
A unified solution to the anisotropy and gradient problems 137
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 136
Two phase galaxy formation: the gas content of normal galaxies 136
Cosmic-ray propagation with DRAGON2: II. Nuclear interactions with the interstellar gas 134
Intermediate-mass and heavy Galactic cosmic-ray nuclei: The case of new AMS-02 measurements 134
The HI content of local late-type galaxies 133
Dark Matter effects on high-redshift universe 132
Diffuse gamma emission of the Galaxy from cosmic rays 131
Self-generated cosmic-ray confinement in TeV halos: Implications for TeV γ -ray emission and the positron excess 130
Turbulence in the intergalactic medium 130
Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre 130
Two-phase galaxy formation: the evolutionary properties of galaxies 128
Cosmic-ray propagation with DRAGON2: I. numerical solver and astrophysical ingredients 128
The origin of Galactic cosmic rays: Challenges to the standard paradigm 128
Stochastic nature of Galactic cosmic-ray sources 128
Implications of the cosmic ray electron spectrum and anisotropy measured with Fermi-LAT 127
Do cosmic rays heat the early intergalactic medium? 127
Diffuse galactic gamma rays at intermediate and high latitudes. I. Constraints on the ISM properties 126
Unified interpretation of cosmic ray nuclei and antiproton recent measurements 126
Diffuse neutrino and gamma-ray emissions of the galaxy above the TeV 125
Gamma-ray and neutrino diffuse emission of the Galaxy above the TeV 124
Galactic electron and positron properties from cosmic ray and radio observations 124
TeV halos and the role of pulsar wind nebulae as sources of cosmic-ray positrons 124
Discovery of the supernova remnant G351.0-5.4 121
Energy deposition by weakly interacting massive particles: a comprehensive study 121
Three-Dimensional Model of Cosmic-Ray Lepton Propagation Reproduces Data from the Alpha Magnetic Spectrometer on the International Space Station 121
Diffuse Galactic Gamma Rays at Intermediate and High Latitudes, Constraints on ISM Properties 121
Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles 120
The puzzling origin of the Li-6 plateau 120
The Galactic Center GeV excess from a series of leptonic cosmic-ray outbursts 120
Unveiling the nature of dark matter with high redshift 21 cm line experiments 119
Impact of the magnetic horizon on the interpretation of the Pierre Auger Observatory spectrum and composition data 117
Testing hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory 117
Simulating intergalactic quasar scintillation 116
Cosmic ray propagation with CRPropa 3 114
CRPropa: A public framework to propagate UHECRs in the universe 111
Cosmic Ray propagation in the Galaxy and diffuse gamma-ray emission 111
AugerPrime surface detector electronics 110
Secondary antiprotons as a Galactic Dark Matter probe 110
Turbulent axion-photon conversions in the Milky Way 110
Galactic diffuse gamma rays meet the PeV frontier 109
Particle energy cascade in the intergalactic medium 109
Three dimensional modeling of CR propagation 108
Inference of the Mass Composition of Cosmic Rays with Energies from 1018.5 to 1020  eV Using the Pierre Auger Observatory and Deep Learning 106
The Pierre Auger Observatory: Contributions to the 39th International Cosmic Ray Conference (ICRC 2025) 104
The Distribution of Ultrahigh-energy Cosmic Rays along the Supergalactic Plane Measured at the Pierre Auger Observatory 104
Reionization during the dark ages from a cosmic axion background 104
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 103
Ground observations of a space laser for the assessment of its in-orbit performance 103
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 102
The scintillator surface detector of the Pierre Auger observatory 101
Quasi‐Constant Time Gap in Multiple Rings of Elves 100
Diffuse synchrotron emission from galactic cosmic ray electrons 100
Scaler Rates from the Pierre Auger Observatory: A New Proxy of Solar Activity 100
The Pierre Auger Observatory open data 99
The nature of dark matter from the global high-redshift H I 21 cm signal 99
CRPropa 3.0 - a Public Framework for Propagating UHE Cosmic Rays through Galactic and Extragalactic Space 97
Demonstrating Agreement between Radio and Fluorescence Measurements of the Depth of Maximum of Extensive Air Showers at the Pierre Auger Observatory 95
Prospects for γ-ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array 95
Search for a diffuse flux of photons with energies above tens of PeV at the Pierre Auger Observatory 94
Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory 94
Radio measurements of the depth of air-shower maximum at the Pierre Auger Observatory 94
Testing hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory 92
Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory 91
The origin of very high-energy diffuse γ-ray emission: The case for galactic source cocoons 71
Totale 13.144
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Categoria #
all - tutte 62.423
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 62.423
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Totale Lug Ago Sett Ott Nov Dic Gen Feb Mar Apr Mag Giu
2020/2021283 0 0 0 0 0 0 0 0 0 17 2 264
2021/2022447 10 7 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
2025/20268.998 510 309 141 741 834 5.017 712 238 315 181 0 0
Totale 13.144