SESANA, ALBERTO
 Distribuzione geografica
Continente #
NA - Nord America 11.138
AS - Asia 10.682
EU - Europa 5.377
SA - Sud America 1.355
AF - Africa 242
OC - Oceania 12
Continente sconosciuto - Info sul continente non disponibili 3
Totale 28.809
Nazione #
US - Stati Uniti d'America 10.879
SG - Singapore 3.654
VN - Vietnam 2.440
CN - Cina 1.653
HK - Hong Kong 1.408
RU - Federazione Russa 1.183
IT - Italia 1.087
BR - Brasile 1.015
DE - Germania 908
SE - Svezia 485
IE - Irlanda 483
FR - Francia 315
IN - India 255
FI - Finlandia 213
GB - Regno Unito 202
ID - Indonesia 188
KR - Corea 187
BD - Bangladesh 162
CA - Canada 147
AR - Argentina 130
IQ - Iraq 120
UA - Ucraina 119
ZA - Sudafrica 94
JP - Giappone 76
PK - Pakistan 73
TR - Turchia 73
MX - Messico 71
PH - Filippine 71
SA - Arabia Saudita 70
EC - Ecuador 57
NL - Olanda 54
AT - Austria 50
ES - Italia 50
PL - Polonia 49
CO - Colombia 39
VE - Venezuela 34
MY - Malesia 33
UZ - Uzbekistan 27
LT - Lituania 26
CH - Svizzera 25
CL - Cile 25
EG - Egitto 25
MA - Marocco 24
BE - Belgio 23
DK - Danimarca 23
TN - Tunisia 22
KE - Kenya 21
IL - Israele 20
JO - Giordania 17
PE - Perù 17
PY - Paraguay 17
TH - Thailandia 16
AZ - Azerbaigian 14
LB - Libano 14
NP - Nepal 14
AE - Emirati Arabi Uniti 13
UY - Uruguay 13
DZ - Algeria 12
ET - Etiopia 12
PS - Palestinian Territory 12
IR - Iran 11
PT - Portogallo 11
OM - Oman 10
GR - Grecia 9
HU - Ungheria 8
AU - Australia 7
DO - Repubblica Dominicana 7
KZ - Kazakistan 7
SY - Repubblica araba siriana 7
CR - Costa Rica 6
CZ - Repubblica Ceca 6
GE - Georgia 6
JM - Giamaica 6
KG - Kirghizistan 6
PA - Panama 6
AL - Albania 5
BO - Bolivia 5
RO - Romania 5
RS - Serbia 5
SN - Senegal 5
BG - Bulgaria 4
BH - Bahrain 4
HN - Honduras 4
NI - Nicaragua 4
NZ - Nuova Zelanda 4
SV - El Salvador 4
AO - Angola 3
BY - Bielorussia 3
CI - Costa d'Avorio 3
HR - Croazia 3
LK - Sri Lanka 3
LV - Lettonia 3
MD - Moldavia 3
NO - Norvegia 3
QA - Qatar 3
TW - Taiwan 3
AM - Armenia 2
BA - Bosnia-Erzegovina 2
CG - Congo 2
CU - Cuba 2
Totale 28.759
Città #
Singapore 2.232
Ann Arbor 1.406
Hong Kong 1.387
San Jose 1.220
Ashburn 901
Ho Chi Minh City 755
Hanoi 648
Fairfield 521
Chandler 489
Dublin 466
Frankfurt am Main 432
New York 422
Santa Clara 389
Hefei 373
Milan 328
Wilmington 325
Woodbridge 293
Munich 266
Houston 261
Chicago 256
Princeton 221
Los Angeles 219
The Dalles 213
Seattle 205
Dallas 203
Moscow 190
Seoul 184
Cambridge 180
Beijing 175
Lauterbourg 160
Jakarta 141
Helsinki 123
Shanghai 117
Council Bluffs 113
Lawrence 110
Altamura 96
Buffalo 95
São Paulo 94
Da Nang 78
Dearborn 67
San Diego 65
Tokyo 62
Guangzhou 56
Haiphong 56
Rome 56
Jacksonville 55
Biên Hòa 54
Orem 54
Montreal 51
Columbus 49
Andover 46
Baghdad 45
Ha Long 45
Hải Dương 43
London 43
Boardman 42
Sacramento 42
Toronto 42
Can Tho 38
Nuremberg 38
Chennai 36
Thái Nguyên 35
Brooklyn 34
Johannesburg 34
Lappeenranta 34
Warsaw 34
Quận Bình Thạnh 33
Rio de Janeiro 33
Denver 32
Falls Church 31
Dhaka 29
Turku 27
Belo Horizonte 26
Phoenix 26
Quận Một 25
Riyadh 25
Vaxjo 25
Bắc Ninh 24
Nanjing 24
Poplar 24
Stockholm 24
Tashkent 24
Amsterdam 23
Atlanta 23
Jeddah 23
Mexico City 23
Ninh Bình 23
Norwalk 23
Brasília 22
Bologna 21
Brussels 21
Erbil 21
Ankara 20
Boston 20
Bắc Giang 20
Lahore 20
Phủ Lý 20
Quito 20
Vienna 20
Vũng Tàu 20
Totale 18.358
Nome #
REPEATING PARTIAL DISRUPTIONS AND TWO-BODY RELAXATION 497
Stellar hardening of massive black hole binaries: The impact of the host rotation 486
Detectability of gravitational waves from primordial black holes orbiting Sgr A∗ 417
The second data release from the European Pulsar Timing Array: V. Implications for massive black holes, dark matter and the early Universe 388
Black holes, gravitational waves and fundamental physics: A roadmap 335
Constraining stellar binary black hole formation scenarios with eLISA eccentricity measurements 319
Testing strengths, limitations, and biases of current pulsar timing arrays'detection analyses on realistic data 309
Observing the inspiral of coalescing massive black hole binaries with LISA in the era of multimessenger astrophysics 303
Post-Newtonian phase accuracy requirements for stellar black hole binaries with LISA 298
Merger Rate of Stellar Black Hole Binaries above the Pair-instability Mass Gap 296
On the search of electromagnetic cosmological counterparts to coalescences of massive black hole binaries 288
Unveiling early black hole growth with multifrequency gravitational wave observations 282
On the eccentricity evolution of massive black hole binaries in stellar backgrounds 279
Mass-redshift dependency of supermassive black hole binaries for the gravitational wave background 274
The lifetime of binary black holes in Sérsic galaxy models 273
Low-frequency gravitational-wave science with eLISA/NGO 267
Post-Newtonian evolution of massive black hole triplets in galactic nuclei-IV. Implications for LISA 265
Multimessenger astronomy with pulsar timing and X-ray observations of massive black hole binaries 264
Second Data Release from the European Pulsar Timing Array: Challenging the Ultralight Dark Matter Paradigm 253
Massive black hole binary eccentricity in rotating stellar systems 253
Detectability of Modulated X-Rays from LISA's Supermassive Black Hole Mergers 252
Optical follow-up of the tick-tock massive black hole binary candidate 250
Limiting eccentricity of subparsec massive black hole binaries surrounded by self-gravitating gas discs 249
The second data release from the European Pulsar Timing Array IV. Search for continuous gravitational wave signals 248
Properties and merger signatures of galaxies hosting LISA coalescing massive black hole binaries 245
Extreme mass ratio inspirals and tidal disruption events in nuclear clusters. I. Time dependent rates 242
Gravitational wave sources in the era of multi-band gravitational wave astronomy 241
Massive black hole binary plane reorientation in rotating stellar systems 240
Linking the spin evolution of massive black holes to galaxy kinematics 239
From galactic nuclei to the halo outskirts: Tracing supermassive black holes across cosmic history and environments 231
The role of bars on the dynamical-friction-driven inspiral of massive objects 230
Gravitational waves from an eccentric population of primordial black holes orbiting Sgr A∗ 229
The second data release from the European Pulsar Timing Array. II. Customised pulsar noise models for spatially correlated gravitational waves 218
Comparing Recent Pulsar Timing Array Results on the Nanohertz Stochastic Gravitational-wave Background 218
The second data release from the European Pulsar Timing Array 218
Chasing supermassive black hole merging events with Athena and LISA 215
Massive black hole binaries: dynamical evolution and observational signatures 215
Circumbinary disc self-gravity governing supermassive black hole binary mergers 215
Practical approaches to analyzing PTA data: Cosmic strings with six pulsars 212
Evolution of binary black holes in self gravitating discs: Dissecting the torques 212
Gravitational wave cosmology and astrophysics with large spectroscopic galaxy surveys 212
The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter, and the early Universe 209
Resolving the nano-hertz gravitational wave sky: The detectability of eccentric binaries with PTA experiments 209
Searching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array 206
Unveiling the hosts of parsec-scale massive black hole binaries: morphology and electromagnetic signatures 205
Quasi-periodic eruptions from impacts between the secondary and a rigidly precessing accretion disc in an extreme mass-ratio inspiral system 204
Hanging on the cliff: Extreme mass ratio inspiral formation with local two-body relaxation and post-Newtonian dynamics 203
Eccentricity evolution of PTA sources from cosmological initial conditions 202
The effect of mission duration on LISA science objectives 201
Linking gravitational waves and X-ray phenomena with joint LISA and Athena observations 198
Resolving Massive Black Hole Binary Evolution via Adaptive Particle Splitting 198
Connecting low-redshift LISA massive black hole mergers to the nHz stochastic gravitational wave background 190
From bright binaries to bumpy backgrounds: Mapping realistic gravitational wave skies with pulsar-timing arrays 188
Emission signatures from sub-parsec post-Newtonian binaries embedded in circumbinary discs 184
The second data release from the European Pulsar Timing Array. III. Search for gravitational wave signals 183
Eppur si muove: Evidence of disc precession or a sub-milliparsec SMBH binary in the QPE-emitting galaxy GSN 069 181
Neural networks unveiling the properties of gravitational wave background from supermassive black hole binaries 181
About gravitational-wave generation by a three-body system 181
European Pulsar Timing Array limits on an isotropic stochastic gravitational-wave background 181
The second data release from the European Pulsar Timing Array: I. The dataset and timing analysis 180
Eccentricity evolution of massive black hole binaries from formation to coalescence 180
The quest for dual and binary supermassive black holes: A multi-messenger view 179
Extreme mass ratio inspirals triggered by massive black hole binaries: from relativistic dynamics to cosmological rates 178
Post-Newtonian evolution of massive black hole triplets in galactic nuclei – II. Survey of the parameter space 178
Unveiling the gravitational universe at μ-Hz frequencies 178
Ticking away: The long-term X-ray timing and spectral evolution of eRO-QPE2 176
Test for LISA foreground Gaussianity and stationarity: Extreme mass-ratio inspirals 173
The International Pulsar Timing Array second data release: Search for an isotropic gravitational wave background 173
Gravitational wave background from extreme mass ratio inspirals 171
Noise analysis in the European Pulsar Timing Array data release 2 and its implications on the gravitational-wave background search 171
Post-Newtonian evolution of massive black hole triplets in galactic nuclei - I. Numerical implementation and tests 168
Post-Newtonian evolution of massive black hole triplets in galactic nuclei – III. A robust lower limit to the nHz stochastic background of gravitational waves 167
Massive BH binaries as periodically variable AGN 166
Identifying heavy stellar black holes at cosmological distances with next-generation gravitational-wave observatories 164
European Pulsar Timing Array limits on continuous gravitational waves from individual supermassive black hole binaries 163
Stellar-mass black-hole binaries in LISA: characteristics and complementarity with current-generation interferometers 163
Science with the TianQin observatory: Preliminary results on testing the no-hair theorem with ringdown signals 161
The Competing Effect of Gas and Stars in the Evolution of Massive Black Hole Binaries 161
Galaxy fields of LISA massive black hole mergers in a simulated universe 160
Exploring the Local Black Hole Mass Function below 106 Solar Masses 160
Cosmology with the Laser Interferometer Space Antenna 158
Science with the space-based interferometer eLISA: Supermassive black hole binaries 155
THE NANOGRAV NINE-YEAR DATA SET: LIMITS ON THE ISOTROPIC STOCHASTIC GRAVITATIONAL WAVE BACKGROUND 153
Lecture notes on black hole binary astrophysics 153
Science with the TianQin observatory: Preliminary results on massive black hole binaries 152
Science with the TianQin observatory: Preliminary result on extreme-mass-ratio inspirals 151
Constraining astrophysical observables of galaxy and supermassive black hole binary mergers using pulsar timing arrays 151
Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature 151
Observing GW190521-like binary black holes and their environment with LISA 149
Hypervelocity Stars from a Supermassive Black Hole-Intermediate-mass Black Hole Binary 148
The importance of live binary evolution in numerical simulations of binaries embedded in circumbinary discs 147
Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background 147
Gravitational-wave physics and astronomy in the 2020s and 2030s 145
Detecting double neutron stars with LISA 145
Hypervelocity binaries from close encounters with a SMBH-IMBH binary: Orbital properties and diagnostics 145
Single sources in the low-frequency gravitational wave sky: Properties and time to detection by pulsar timing arrays 144
Prospects for Multiband Gravitational-Wave Astronomy after GW150914 144
Robust parameter estimation from pulsar timing data 143
Expected properties of the first gravitational wave signal detected with pulsar timing arrays 143
Weakly parametric approach to stochastic background inference in LISA 142
Totale 21.217
Categoria #
all - tutte 102.291
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 102.291


Totale Lug Ago Sett Ott Nov Dic Gen Feb Mar Apr Mag Giu
2020/2021198 0 0 0 0 0 0 0 0 0 0 96 102
2021/20221.413 200 61 127 103 36 145 41 53 136 142 92 277
2022/20232.179 287 546 215 169 210 334 14 121 150 33 65 35
2023/20242.031 66 61 50 174 240 472 290 92 212 41 49 284
2024/20256.866 315 795 514 279 405 347 386 258 647 931 622 1.367
2025/202613.399 2.026 1.441 821 1.414 1.271 676 2.216 720 1.099 1.565 150 0
Totale 29.570