Massimo Meneghetti
Meneghetti, Massimo, 1974-....
Meneghetti, Massimo
VIAF ID: 1298147553254753800009 (Personal)
Permalink: http://viaf.org/viaf/1298147553254753800009
Preferred Forms
- 100 0 _ ‡a Massimo Meneghetti
-
- 100 1 _ ‡a Meneghetti, Massimo ‡d 1974-
- 100 1 _ ‡a Meneghetti, Massimo, ‡d 1974-
- 100 1 _ ‡a Meneghetti, Massimo, ‡d 1974-....
4xx's: Alternate Name Forms (4)
5xx's: Related Names (3)
- 551 _ _ ‡a Bologna ‡4 ortw ‡4 https://d-nb.info/standards/elementset/gnd#placeOfActivity
- 510 2 _ ‡a Institut für Theoretische Astrophysik ‡g Heidelberg ‡4 affi ‡4 https://d-nb.info/standards/elementset/gnd#affiliation ‡e Affiliation
- 551 _ _ ‡a Padua ‡4 ortw ‡4 https://d-nb.info/standards/elementset/gnd#placeOfActivity
Works
Title | Sources |
---|---|
CLASH: A CENSUS OF MAGNIFIED STAR-FORMING GALAXIES ATz∼ 6-8 | |
CLASH: DISCOVERY OF A BRIGHTz≃ 6.2 DWARF GALAXY QUADRUPLY LENSED BY MACS J0329.6-0211 | |
The cluster lensing and supernova survey with Hubble (CLASH): strong-lensing analysis of A383 from 16-band HST/WFC3/ACS imaging | |
Cluster mass scaling relations through weak lensing measurements | |
Combining weak and strong lensing in cluster potential reconstruction | |
Constraints on dark energy models from galaxy clusters with multiple arcs | |
The contribution of halos with different mass ratios to the overall growth of cluster-sized halos | |
Dark matter–baryons separation at the lowest mass scale: the Bullet Group★ | |
Direct Lyman continuum and Ly α escape observed at redshift 4 | |
Disentangling dark sector models using weak lensing statistics | |
Do arcs require flat halo cusps? | |
Early structure formation in quintessence models and its implications for cosmic reionization from first stars | |
Effects of cluster galaxies on arc statistics | |
The effects of ellipticity and substructure on estimates of cluster density profiles based on lensing and kinematics | |
Effects of the halo concentration distribution on strong-lensing optical depth and X-ray emission | |
Euclid preparation: XVIII. The NISP photometric system | |
Euclid preparation: XXIX. Water ice in spacecraft Part I: The physics of ice formation and contamination | |
Euclid preparation: XXVII. A UV-NIR spectral atlas of compact planetary nebulae for wavelength calibration | |
Euclid preparation: XXX. Performance assessment of the NISP red grism through spectroscopic simulations for the wide and deep surveys | |
Euclid space mission: a cosmological challenge for the next 15 years | |
Euclidmission: building of a reference survey | |
Evidence for ubiquitous high-equivalent-width nebular emission in z ~ 7 galaxies: toward a clean measurement of the specific star-formation rate using a sample of bright, magnified galaxies | |
The Frontier Fields lens modelling comparison project | |
Giant cluster arcs as a constraint on the scattering cross-section of dark matter | |
Halo Concentrations and the Fundamental Plane of Galaxy Clusters | |
Hubble Space Telescope combined strong and weak lensing analysis of the CLASH sample: mass and magnification models and systematic uncertainties | |
Illuminating a dark lens : a type Ia supernova magnified by the frontier fields galaxy cluster Abell 2744 | |
The impact of gas physics on strong cluster lensing | |
Internal Cluster Structure | |
Intracluster light properties in the CLASH-VLT cluster MACS J1206.2-0847 | |
Introduction to gravitational lensing : with Python examples | |
Is the Number of Giant Arcs in ΛCDM Consistent with Observations? | |
KiDS and Euclid : Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography | |
The Lensed Arc Production Efficiency of Galaxy Clusters: A Comparison of Matched Observed and Simulated Samples | |
Magnifying the Early Episodes of Star Formation: Super Star Clusters at Cosmological Distances | |
Mass and concentration estimates from weak and strong gravitational lensing: a systematic study | |
Mass Distributions ofHubble Space TelescopeGalaxy Clusters from Gravitational Arcs | |
Mass profiles andc − MDMrelation in X-ray luminous galaxy clusters (Corrigendum) | |
Metallicity evolution, metallicity gradients, and gas fractions atz~ 3.4 | |
Méthodes numériques pour prédire le signal d'optique gravitationnelle comme outil pour sonder la matière dans l'Univers. | |
moka: a new tool for strong lensing studies | |
The MUSIC of CLASH: predictions on the concentration-mass relation | |
Next Generation Virgo Cluster Survey. XXI. The Weak Lensing Masses of the CFHTLS and NGVS RedGOLD Galaxy Clusters and Calibration of the Optical Richness | |
Numerical methods for the prediction of gravitational lensing signal as a probe of the mass content on the Universe | |
Numerical study of halo concentrations in dark-energy cosmologies | |
On the dissection of degenerate cosmologies with machine learning | |
Optimal filtering of optical and weak lensing data to search for galaxy clusters: application to the COSMOS field | |
Origins of weak lensing systematics, and requirements on future instrumentation (or knowledge of instrumentation) | |
Predicting the number of giant arcs expected in the next-generation wide-field surveys from space | |
Preface | |
Probing ionizing radiation of star-forming galaxies at with strong lensing | |
Realistic simulations of gravitational lensing by galaxy clusters: extracting arc parameters from mock DUNE images | |
Reconstructing the projected gravitational potential of galaxy clusters from galaxy kinematics | |
Relation d’échelle d'amas de galaxies à partir d'observations de lentilles gravitationnelles. | |
Reliable shapelet image analysis | |
Resolved [CII] emission in a lensed quasar atz= 4.4 | |
Scaling relation in two situations of extreme mergers | |
Searching dark-matter halos in the GaBoDS survey | |
Simulating the physical properties of dark matter and gas inside the cosmic web | |
Simulation-based marginal likelihood for cluster strong lensing cosmology | |
Statistical properties of SZ and X-ray cluster detections | |
Strong [CII] emission at high redshift | |
Strong lensing efficiency of galaxy clusters in dark energy cosmologies | |
Strong lensing in the MARENOSTRUM UNIVERSE | |
Strong lensing statistics and the power spectrum normalisation | |
The strongest gravitational lenses. III. The order statistics of the largest Einstein radii | |
Temperature dependence of the nonlinear optical response of smectic liquid crystals containing gold nanorods. | |
Testing the reliability of weak lensing cluster detections | |
Weak lensing by galaxies in groups and clusters – I. Theoretical expectations | |
Weak-lensing peaks in simulated light cones: investigating the coupling between dark matter and dark energy | |
Weighing simulated galaxy clusters using lensing and X-ray | |
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