VIOTTO, VALENTINA
 Distribuzione geografica
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Continente #
NA - Nord America 3.593
EU - Europa 379
AS - Asia 189
OC - Oceania 2
SA - Sud America 2
Continente sconosciuto - Info sul continente non disponibili 1
Totale 4.166
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Nazione #
US - Stati Uniti d'America 3.591
CN - Cina 152
IT - Italia 137
FI - Finlandia 74
UA - Ucraina 42
SE - Svezia 36
GB - Regno Unito 24
VN - Vietnam 24
FR - Francia 17
DE - Germania 16
PL - Polonia 13
IE - Irlanda 8
AT - Austria 4
HK - Hong Kong 4
IN - India 4
NL - Olanda 3
BR - Brasile 2
CA - Canada 2
IR - Iran 2
JP - Giappone 2
RO - Romania 2
AU - Australia 1
CH - Svizzera 1
EU - Europa 1
LU - Lussemburgo 1
NO - Norvegia 1
NZ - Nuova Zelanda 1
TR - Turchia 1
Totale 4.166
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Città #
Fairfield 600
Chandler 453
Woodbridge 398
Ashburn 301
Ann Arbor 263
Houston 261
Cambridge 228
Seattle 226
Wilmington 174
Beijing 112
Princeton 55
Medford 54
Helsinki 47
San Diego 47
Des Moines 43
New York 39
Ogden 29
Padova 28
Dong Ket 24
Selvazzano Dentro 19
Boardman 18
Nanjing 13
Jacksonville 12
Zielona Góra 10
London 9
Dublin 8
Voghera 7
Bologna 6
Cagliari 6
Paris 6
Dearborn 5
Haikou 5
Nanchang 5
Orange 5
Orsay 5
Brescia 4
Hong Kong 4
Jiaxing 4
Roxbury 4
Washington 4
Amsterdam 3
Arosio 3
Chicago 3
Hebei 3
Kilburn 3
Norwalk 3
Rome 3
Tianjin 3
Vienna 3
Acton 2
Berlin 2
Brentino Belluno 2
Catania 2
Dayton 2
Inverigo 2
Kharkiv 2
Los Angeles 2
Milan 2
Prescot 2
Pune 2
Strasbourg 2
Trani 2
Valdagno 2
Viterbo 2
Americana 1
Ardabil 1
Arzano 1
Atlanta 1
Auckland 1
Bacoli 1
Borgo Valsugana 1
Borås 1
Erzurum 1
Esslingen am Neckar 1
Florence 1
Garching 1
Greenwich 1
Hendon 1
Isola Vicentina 1
Lappeenranta 1
Las Vegas 1
Leawood 1
Martignacco 1
Miami 1
New Hyde Park 1
Nürnberg 1
Oslo 1
Palmer 1
Pesaro 1
Phoenix 1
Rockville 1
Santa Clara 1
Sendai 1
Southwark 1
Stockholm 1
São Paulo 1
Tappahannock 1
Tokyo 1
Valbonne 1
Venice 1
Totale 3.634
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Nome #
A testing facility at the Asiago Copernico telescope in the framework of the ADaptive Optics National laboratory of Italy: ADONI 119
Manufacturing and alignment tolerance analysis through Montecarlo approach for PLATO 115
A comparison between the opto-thermo-mechanical model and lab measurements for CHEOPS 113
Radiation, thermal gradient and weight: A threefold dilemma for PLATO 112
A display model for the TOU of PLATO: Just a cool toy or a benchmark of opportunities? 110
Shaping the PSF to nearly top-hat profile: CHEOPS laboratory resultsSpace Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave 108
PLATO: A multiple telescope spacecraft for exo-planets hunting 104
From a demonstration model to the flight model: AIV procedures and results for CHEOPS telescope 103
The AIV concept of SHARK-NIR, a new coronagraph for the Large Binocular Telescope 102
A comparison between different coronagraphic data reduction techniques 101
Aligning the demonstration model of CHEOPS 95
Modelling global multi-conjugated adaptive optics 94
Dealing with the cigar: Preliminary performance estimation of an INGOT WFS 94
PLATO: The ESA mission for exo-planets discovery 92
Extending the pyramid WFS to LGSs: The INGOT WFS 92
SHARK-NIR: The coronagraphic camera for LBT in the AIV phase at INAF-Padova 91
High order dark wavefront sensing simulations 90
SHARK-NIR system design analysis overview 88
Thermal effects on PLATO point spread function 86
The Copernico Telescope testing facility for AO on-sky demonstrations 86
High-z galaxies simulations: A benchmark for Global-MCAO 85
The NIR arm of SHARK: System for coronagraphy with High-order Adaptive optics from R to K bands 84
Exploring the performance of a GMCAO-equipped ELT within the deep field surveys strategy 84
Multiple Spatial Frequencies Pyramid WaveFront Sensing 83
Revisiting static modulation in pyramid wavefront sensing 83
SHARK (System for coronagraphy with High order Adaptive optics from R to K band): A proposal for the LBT 2nd generation instrumentation 82
SHARK-NIR: From K-band to a key instrument, a status update 82
Multiple spatial frequencies wavefront sensing 82
An extensive coronagraphic simulation applied to LBT 80
The telescope optical unit prototype AIV in the framework of the PLATO ESA mission 78
Validating the phase diversity approach for sensing NCPA in SHARK-NIR, the second-generation high-contrast imager for the Large Binocular Telescope 77
SHARK-NIR coronagraphic simulations: Performance dependence on the Strehl ratio 72
PWFSs on GMCAO: A different approach to the non-linearity issue 68
Data processing on simulated data for SHARK-NIR 67
SHARK-NIR, the coronagraphic camera for LBT, moving toward construction 67
A Holographic Diffuser Generalised Optical Differentiation Wavefront Sensor 66
SHARK-NIR Channel: A high contrast imager with coronagraphic capabilities for the Large Binocular Telescope 65
Avoiding to trade sensitivity for linearity in a real world WFS 62
Global Multi Conjugated Adaptive Optics (GMCAO) aiming to the (whole) sky 62
Ingot Laser Guide Stars Wavefront Sensing 62
From 3D view to 3D print 61
The Chandra Deep Field South as a test case for Global Multi Conjugate Adaptive Optics 60
A testing facility for AO on-sky demonstrations at the Copernico’s Telescope within the ADONI framework 60
Hierarchichal-segmented AO in order to attain wide field compensation in the visible on an 8m class telescope 56
GMCAO simulation tool development 55
Prospects of Deep Field Surveys with Global-MCAO on an ELT 48
null 45
GMCAO for E-ELT: A feasibility study 44
From 8(m) to 8(mm): wavefront sensing from cosmological to human scales 41
Statistical and morphological analysis of mock galactic fields in the Global-MCAO perspective 40
CHEOPS observations of the HD 108236 planetary system: a fifth planet, improved ephemerides, and planetary radii 40
The CHEOPS mission 38
Simulations of ELT-GMCAO performance for deep field observations 30
The telescope optical units prototype and AIV in the framework of the PLATO ESA mission 28
Rad-hard properties of the optical glass adopted for the PLATO space telescope refractive components 27
A virtual coronagraphic test bench for SHARK-NIR, the second-generation high contrast imager for the Large Binocular Telescope 26
A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS 25
A search for transiting planets around hot subdwarfs I. Methods and performance tests on light curves from Kepler, K2, TESS, and CHEOPS 23
A CHEOPS-enhanced view of the HD 3167 system, 16
Totale 4.249
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Categoria #
all - tutte 16.571
article - articoli 2.585
book - libri 0
conference - conferenze 0
curatela - curatele 0
other - altro 0
patent - brevetti 0
selected - selezionate 0
volume - volumi 0
Totale 19.156
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Totale Lug Ago Sett Ott Nov Dic Gen Feb Mar Apr Mag Giu
2018/2019303 0 0 0 0 0 0 0 0 0 0 167 136
2019/2020978 111 62 10 60 128 69 100 111 113 89 96 29
2020/2021450 29 39 11 26 16 28 19 43 88 25 77 49
2021/2022706 11 75 100 39 20 24 27 86 38 8 71 207
2022/2023796 131 97 54 126 97 89 2 60 99 3 30 8
2023/2024419 44 46 53 40 21 84 35 23 72 1 0 0
Totale 4.249