CESCUTTI, GABRIELE
 Distribuzione geografica
Continente #
NA - Nord America 3.828
AS - Asia 3.199
EU - Europa 1.977
SA - Sud America 391
AF - Africa 185
OC - Oceania 4
Continente sconosciuto - Info sul continente non disponibili 3
Totale 9.587
Nazione #
US - Stati Uniti d'America 3.729
SG - Singapore 1.279
CN - Cina 622
IT - Italia 366
HK - Hong Kong 365
BR - Brasile 315
SE - Svezia 283
PL - Polonia 281
VN - Vietnam 277
KR - Corea 220
DE - Germania 172
FR - Francia 158
BD - Bangladesh 155
UA - Ucraina 116
RU - Federazione Russa 105
MA - Marocco 102
GB - Regno Unito 87
FI - Finlandia 77
BG - Bulgaria 66
IE - Irlanda 64
NL - Olanda 58
IN - India 55
CA - Canada 50
TR - Turchia 38
AR - Argentina 31
CH - Svizzera 27
BE - Belgio 26
MX - Messico 24
AT - Austria 23
IQ - Iraq 23
ZA - Sudafrica 22
ES - Italia 19
IR - Iran 16
JP - Giappone 16
SA - Arabia Saudita 16
SN - Senegal 15
ID - Indonesia 11
IL - Israele 11
PK - Pakistan 11
DZ - Algeria 10
EC - Ecuador 10
AZ - Azerbaigian 9
LT - Lituania 9
UZ - Uzbekistan 9
AE - Emirati Arabi Uniti 8
CO - Colombia 8
JO - Giordania 8
KE - Kenya 8
JM - Giamaica 7
UY - Uruguay 7
CL - Cile 6
MY - Malesia 6
SK - Slovacchia (Repubblica Slovacca) 6
TH - Thailandia 6
VE - Venezuela 6
ET - Etiopia 5
KG - Kirghizistan 5
PH - Filippine 5
PT - Portogallo 5
TN - Tunisia 5
AU - Australia 4
CZ - Repubblica Ceca 4
GE - Georgia 4
LB - Libano 4
NP - Nepal 4
BB - Barbados 3
DK - Danimarca 3
GR - Grecia 3
HN - Honduras 3
HU - Ungheria 3
KZ - Kazakistan 3
NG - Nigeria 3
RS - Serbia 3
BH - Bahrain 2
BY - Bielorussia 2
CR - Costa Rica 2
DO - Repubblica Dominicana 2
EG - Egitto 2
EU - Europa 2
GT - Guatemala 2
KH - Cambogia 2
LU - Lussemburgo 2
LV - Lettonia 2
LY - Libia 2
OM - Oman 2
PE - Perù 2
PR - Porto Rico 2
PY - Paraguay 2
QA - Qatar 2
RO - Romania 2
SY - Repubblica araba siriana 2
AL - Albania 1
BF - Burkina Faso 1
BO - Bolivia 1
BW - Botswana 1
CI - Costa d'Avorio 1
EE - Estonia 1
GF - Guiana Francese 1
GY - Guiana 1
HR - Croazia 1
Totale 9.568
Città #
Singapore 755
Ashburn 463
Hong Kong 357
San Jose 344
Ann Arbor 225
Seoul 220
Warsaw 199
Fairfield 198
Woodbridge 198
Hefei 181
Chandler 180
Houston 157
Beijing 156
Wilmington 127
Santa Clara 119
Princeton 114
Boardman 104
Chicago 102
Jacksonville 97
Casablanca 92
Lauterbourg 83
Columbus 78
Los Angeles 78
Zgierz 78
Ho Chi Minh City 75
Trieste 69
Hanoi 66
Sofia 66
Dublin 65
Seattle 64
Cambridge 63
The Dalles 54
Moscow 52
Milan 51
Dallas 44
Munich 38
New York 37
Council Bluffs 36
Düsseldorf 36
Buffalo 35
Frankfurt am Main 32
London 30
São Paulo 27
Bremen 22
Brussels 22
Da Nang 21
Paris 21
Bern 20
Turku 20
Helsinki 18
Miano 18
Vienna 18
Izmir 17
Montreal 16
Rome 16
Tehran 16
Dakar 15
Guangzhou 14
Chennai 13
Johannesburg 13
Rio de Janeiro 13
Boston 12
Haiphong 12
Tokyo 12
Toronto 12
Norwalk 11
Orem 11
San Francisco 11
Nuremberg 10
Portsmouth 10
San Diego 10
Atlanta 9
Baku 9
Belo Horizonte 9
Brooklyn 9
Denver 9
Mexico City 9
Charlotte 8
Dong Ket 8
Redondo Beach 8
Shanghai 8
Tashkent 8
Washington 8
Baghdad 7
Colmenar Viejo 7
Curitiba 7
Dhaka 7
Kocaeli 7
Montevideo 7
Nairobi 7
Naples 7
Phoenix 7
Stockholm 7
Amman 6
Brasília 6
Campinas 6
Florence 6
Heidelberg 6
Jeddah 6
Kingston 6
Totale 6.283
Nome #
The role of neutron star mergers in the chemical evolution of the Galactic halo 353
Effects of galactic fountains and delayed mixing in the chemical evolution of the Milky Way 243
An inhomogeneous model for the Galactic halo: a possible explanation for the spread observed in s- and r-process elements 233
A comparison of the s- and r-process element evolution in local dwarf spheroidal galaxies and in the Milky Way 231
Abundance gradients in the Milky Way for alpha-elements, iron peak elements, barium, lanthanum and europium 226
Chemical evolution of the Galactic bulge: different stellar populations and possible gradients 226
Chemical evolution of the Milky Way: the origin of phosphorus 215
Manganese evolution in Omega Centauri: a clue to the cluster formation mechanisms? 212
Galactic astroarchaeology: reconstructing the bulge history by means of the newest data 205
The origin of abundance gradients in the Milky Way: the predictions of different models 201
The evolution of carbon and oxygen in the bulge and disk of the Milky Way 169
The Evolution of Oxygen and Magnesium in the Bulge and Disk of the Milky Way 164
Silicon depletion in damped Ly α systems. The S/Zn method 163
The evolution of barium and europium in local dwarf spheroidal galaxies 154
Detailed chemical evolution of Carina and Sagittarius dwarf spheroidal galaxies 149
Evolution of neutron capture elements in dwarf galaxies 138
Constraints on stellar rotation from the evolution of Sr and Ba in the Galactic halo 135
Chemical clocks and their time zones: understanding the [s/Mg]–age relation with birth radii 131
MINCE: II. Neutron capture elements 127
The contribution from rotating massive stars to the enrichment in Sr and Ba of the Milky Way 127
Barium lines in high-quality spectra of two metal-poor giants in the Galactic halo 123
4MOST: 4-metre Multi-Object Spectroscopic Telescope 123
A new delay time distribution for merging neutron stars tested against Galactic and cosmic data 122
2D chemical evolution models 121
7Be in the outburst of the ONe nova V6595 Sgr 121
(Re)mind the gap: A hiatus in star formation history unveiled by APOGEE DR17 119
The chemical evolution of manganese in different stellar systems 119
7Be detection in the 2021 outburst of RS Oph 118
Origin of neutron-capture elements with the Gaia-ESO survey: the evolution of s- and r-process elements across the Milky Way 117
Modelling the chemical evolution of Zr, La, Ce, and Eu in the Galactic discs and bulge 115
The Fall of a Giant. Chemical evolution of Enceladus, alias the Gaia Sausage 115
Abundances of carbon-enhanced metal-poor stars as constraints on their formation 115
7Li evolution in the thin and thick discs of the Milky Way 111
MINCE: I. Presentation of the project and of the first year sample 108
The cerium content of the Milky Way as revealed by Gaia DR3 GSP-Spec abundances 108
Time evolution of Ce as traced by APOGEE using giant stars observed with the Kepler, TESS and K2 missions 105
An inefficient dwarf: chemical abundances and the evolution of the Ursa Minor dwarf spheroidal galaxy 104
Chromium: NTLE abundances in metal-poor stars and nucleosynthesis in the Galaxy 103
Chemical evolution models for local group dwarf spheroidal galaxies: the evolution of Fe-peak elements 102
Chemical evolution of neutron capture elements in our Galaxy and in the dwarf spheroidal galaxies of the Local Group 101
Young giants of intermediate mass. Evidence of rotation and mixing 99
Classical novae with CUBES 98
Detection of 7Be II in the Small Magellanic Cloud 96
Neutron stars mergers in a stochastic chemical evolution model: Impact of time delay distributions 95
The CEMP star SDSS J0222-0313: the first evidence of proton ingestion in very low-metallicity AGB stars? 94
r-Process Nucleosynthesis from Compact Binary Mergers 94
Neutron star binary orbits in their host potential: Effect on early R-process enrichment 88
There is no place like home – finding birth radii of stars in the Milky Way 88
Chemical evolution of heavy elements in the Local Group 88
Impact of AGB Stars on the Chemical Evolution of Neutron-Capture Elements 87
Metal Mixing in the r-process Enhanced Ultrafaint Dwarf Galaxy Reticulum II* 87
Magnetic-buoyancy-induced mixing in AGB stars: A theoretical explanation of the non-universal relation of [Y/Mg] to age 86
Observational constraints on the origin of the elements: VIII. Constraining the barium, strontium, and yttrium chemical evolution in metal-poor stars 83
UVES analysis of red giants in the bulge globular cluster NGC 6522 81
The Gaia-ESO survey: placing constraints on the origin of r-process elements 81
Stellar population astrophysics (SPA) with the TNG. GIANO-B spectroscopy of red supergiants in Alicante 7 and Alicante 10 81
Uncertainties in s-process nucleosynthesis in low-mass stars determined from Monte Carlo variations 79
Uncertainties in νp-process nucleosynthesis from Monte Carlo variation of reaction rates 78
Explaining the Ba, Y, Sr, and Eu abundance scatter in metal-poor halo stars: constraints to the r-process 76
INHOMOGENEOUS GALACTIC HALO: A POSSIBLE EXPLANATION FOR THE SPREAD OBSERVED IN S- AND R- PROCESS ELEMENTS 73
Phosphorus Abundances in the Hyades and Galactic Disk 71
Mass and metallicity distribution of parent AGB stars of presolar SiC 71
Estimating stellar birth radii and the time evolution of Milky Way's ISM metallicity gradient 70
Lithium and beryllium in the Gaia-Enceladus galaxy 70
High-resolution abundance analysis of red giants in the globular cluster NGC 6522 68
Impacts of Nuclear-Physics Uncertainty in Stellar Temperatures on the s-Process Nucleosynthesis 67
Does the chemical signature of TYC 844210361 originate from a rotating massive star that died in a faint explosion? 67
Heavy element abundances in galactic globular clusters 66
New eyes on the first stars: the old bulge component and the important role of PNe in this context 66
Galactic chemical evolution: The role of the first stars 65
Lithium in the closest satellite of our Milky Way 63
Europium enrichment and hierarchical formation of the Galactic halo 63
Uncertainties in s-process nucleosynthesis in massive stars determined by Monte Carlo variations 63
Phosphorus Abundances in FGK Stars 62
The chemical evolution of Barium and Europium in the Milky Way 60
LTE or non-LTE, that is the question. The NLTE chemical evolution of strontium in extremely metal-poor stars 60
Production Uncertainties of p-Nuclei in the γ-Process in Massive Stars Using a Monte Carlo Approach 60
Manganese in dwarf spheroidal galaxies 59
Uncertainties in the production of p nuclei in massive stars obtained from Monte Carlo variations 57
The effects of stellar winds of fast-rotating stars in the earliest phases of chemical enrichment of the Galaxy 55
Solar abundance of manganese: a case for near Chandrasekhar-mass Type Ia supernova progenitors 54
The chemical evolution of barium and Europium in the Milky Way 54
The s-process in the Galactic halo: the fifth signature of spinstars in the early Universe? 54
The Evolution of Heavy Elements in Dwarf Spheroidal Galaxies 51
The oldest stars of the bulge: new information on the ancient Galaxy 50
The Chemical Evolution in the Solar Vicinity and the Nucleosynthesis of Neutron Capture Elements 49
Manganese spread in Ursa Minor as a proof of sub-classes of type Ia supernovae 47
The neutron-capture and α-elements abundance ratios scatter in old stellar populations: cosmological simulations of the stellar halo 47
The Chemical Evolution of Phosphorus 46
The nature of the First Stars: the role of the isotopic ratios of barium 44
The CUBES science case 43
CUBES phase a design overview: The Cassegrain U-Band efficient spectrograph for the very large telescope 37
Observational constraints on the origin of the elements: III. Evidence for the dominant role of sub-Chandrasekhar SN Ia in the chemical evolution of Mn and Fe in the Galaxy 37
CUBES, the Cassegrain U-Band Efficient Spectrograph for the VLT 31
CUBES: a UV spectrograph for the future 29
High N/O ratio at high redshift as a result of a strong burst of star formation and differential galactic winds 8
Chemical Evolution of R-process Elements in Stars (CERES): III. Chemical abundances of neutron capture elements from Ba to Eu 8
Explaining the 12C/13C ratio in the Galactic halo: The contribution from shell mergers in primordial massive stars 7
A Sequoia stellar candidate with very high 7Li and 9Be 7
Unlocking the mystery of strontium synthesis in the early Galaxy through analysis of barium isotopes in very metal-poor stars 6
Totale 9.796
Categoria #
all - tutte 35.341
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 35.341


Totale Lug Ago Sett Ott Nov Dic Gen Feb Mar Apr Mag Giu
2021/2022512 10 41 24 37 5 62 19 26 78 42 20 148
2022/2023724 84 91 72 40 75 108 29 88 58 8 53 18
2023/2024630 31 32 25 24 51 54 67 184 7 8 80 67
2024/20251.942 8 276 274 102 117 207 105 108 146 170 168 261
2025/20264.387 434 306 281 347 327 336 601 128 383 725 274 245
2026/202740 40 0 0 0 0 0 0 0 0 0 0 0
Totale 9.845