Abstract is: Richard Massey (born 14 October 1977) is a physicist currently working as Royal Society Research Fellow in the Institute for Computational Cosmology at Durham University. Previously he was a senior research fellow in astrophysics at the California Institute of Technology and STFC Advanced Fellow at the Institute for Astronomy of the University of Edinburgh. Massey graduated in Maths and Physics from the University of Durham in 2000 and was a member of Castle. He completed his Ph.D. at Cambridge (Clare College) in 2003, with a thesis entitled Weighing the Universe with weak gravitational lensing. Massey is most well known for his studies of dark matter, including the first 3D map of its large-scale distribution and its behaviour during collisions. He was awarded the 2011 Philip Leverhulme Prize in Astronomy and Astrophysics.He has featured in several TV documentaries, including BBC's Horizon documentary "How Big is the Universe?" in 2013 and online.
| human | Q5 |
| P8880 | AstroGen ID | 14980 |
| P646 | Freebase ID | /m/027kz1j |
| P1960 | Google Scholar author ID | 6TubcLQAAAAJ |
| P345 | IMDb ID | nm3758317 |
| P496 | ORCID iD | 0000-0002-6085-3780 |
| P1053 | ResearcherID | D-1300-2016 |
| P184 | doctoral advisor | Alexandre Réfrégier | Q114437843 |
| P69 | educated at | University of Cambridge | Q35794 |
| Durham University | Q458393 | ||
| Clare College | Q760967 | ||
| P108 | employer | Durham University | Q458393 |
| P734 | family name | Massey | Q21484684 |
| Massey | Q21484684 | ||
| Massey | Q21484684 | ||
| P735 | given name | Richard | Q1249148 |
| Richard | Q1249148 | ||
| James | Q677191 | ||
| James | Q677191 | ||
| P106 | occupation | cosmologist | Q2998308 |
| P21 | sex or gender | male | Q6581097 |
| Q58908658 | A detection of weak-lensing magnification using galaxy sizes and magnitudes |
| Q112108736 | A forward-modelling method to infer the dark matter particle mass from strong gravitational lenses |
| Q59962981 | A gravitationally-boosted MUSE survey for emission-line galaxies at z ≳ 5 behind the massive cluster RCS 0224 |
| Q58489726 | A weak lensing mass reconstruction of the large-scale filament feeding the massive galaxy cluster MACS J0717.5+3745 |
| Q58489776 | A weak lensing study of X-ray groups in the COSMOS survey: form and evolution of the mass-luminosity relation |
| Q123693838 | Abell 1201: detection of an ultramassive black hole in a strong gravitational lens |
| Q59320361 | Abell 2744: too much substructure for ΛCDM? |
| Q58908903 | Active galactic nucleus host galaxy morphologies in COSMOS |
| Q59846249 | An integral field spectrograph for SNAP |
| Q58489780 | Bars in early- and late-type discs in COSMOS |
| Q123698885 | Beyond the bulge–halo conspiracy? Density profiles of early-type galaxies from extended-source strong lensing |
| Q57686471 | CLASH: the concentration-mass relation of galaxy clusters |
| Q58489880 | COSMOS Morphological Classification with the Zurich Estimator of Structural Types (ZEST) and the Evolution Sincez= 1 of the Luminosity Function of Early, Disk, and Irregular Galaxies |
| Q56567288 | COSMOS: Hubble Space Telescope Observations |
| Q58489879 | COSMOS: Three‐dimensional Weak Lensing and the Growth of Structure |
| Q58489727 | COSMOS: stochastic bias from measurements of weak lensing and galaxy clustering |
| Q57630801 | Color, 3D simulated images with shapelets |
| Q47098810 | Cosmology and Fundamental Physics with the Euclid Satellite |
| Q53822180 | Cosmology and fundamental physics with the Euclid satellite. |
| Q84667338 | Cosmology: Dark is the new black |
| Q58474380 | Creation of cosmic structure in the complex galaxy cluster merger Abell 2744 |
| Q58489707 | Dark matter astrometry: accuracy of subhalo positions for the measurement of self-interaction cross-sections |
| Q58915446 | Dark matter dynamics in Abell 3827: new data consistent with standard cold dark matter |
| Q55042909 | Dark matter maps reveal cosmic scaffolding. |
| Q58489845 | Erratum: “First Catalog of Strong Lens Candidates in the COSMOS Field” (ApJS, 176, 19 [2008]) |
| Q112965681 | Euclid : Forecasts from redshift-space distortions and the Alcock–Paczynski test with cosmic voids |
| Q112953856 | Euclid : the selection of quiescent and star-forming galaxies using observed colours |
| Q109931203 | Euclid Preparation. XIV. The Complete Calibration of the Color–Redshift Relation (C3R2) Survey: Data Release 3 |
| Q125445752 | Euclid preparation |
| Q112945342 | Euclid preparation: IX. EuclidEmulator2 – power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations |
| Q106359227 | Euclid preparation: V. Predicted yield of redshift 7 < z < 9 quasars from the wide survey |
| Q112945393 | Euclid preparation: VI. Verifying the Performance of Cosmic Shear Experiments (Corrigendum) |
| Q106359232 | Euclid preparation: VI. Verifying the performance of cosmic shear experiments |
| Q106369680 | Euclid preparation: VII. Forecast validation for Euclid cosmological probes |
| Q106369685 | Euclid preparation: VIII. The Complete Calibration of the Colour–Redshift Relation survey: VLT/KMOS observations and data release |
| Q106369634 | Euclid preparation: X. The Euclid photometric-redshift challenge |
| Q109745185 | Euclid preparation: XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography |
| Q112945491 | Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses |
| Q112945517 | Euclid preparation: XIII. Forecasts for galaxy morphology with the Euclid Survey using deep generative models |
| Q112945983 | Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering |
| Q112945525 | Euclid preparation: XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis |
| Q112945530 | Euclid preparation: XVI. Exploring the ultra-low surface brightness Universe with Euclid/VIS |
| Q112946183 | Euclid preparation: XVII. Cosmic Dawn Survey: Spitzer Space Telescope observations of the Euclid deep fields and calibration fields |
| Q112945994 | Euclid preparation: XVIII. The NISP photometric system |
| Q57617376 | Euclid space mission: a cosmological challenge for the next 15 years |
| Q112945331 | Euclid: Constraining dark energy coupled to electromagnetism using astrophysical and laboratory data |
| Q112953782 | Euclid: Estimation of the Impact of Correlated Readout Noise for Flux Measurements with the Euclid NISP Instrument |
| Q106369640 | Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes |
| Q112945556 | Euclid: Forecasts for k-cut 3×2 Point Statistics |
| Q106369643 | Euclid: Identification of asteroid streaks in simulated images using StreakDet software |
| Q110205383 | Euclid: Impact of non-linear and baryonic feedback prescriptions on cosmological parameter estimation from weak lensing cosmic shear |
| Q106369717 | Euclid: Reconstruction of weak-lensing mass maps for non-Gaussianity studies |
| Q106369656 | Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey |
| Q106359243 | Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments |
| Q58915941 | Evolution of galaxies and their environments at z = 0.1-3 in COSMOS |
| Q59733261 | Evolution of the stellar-to-dark matter relation: separating star-forming and passive galaxies from z = 1 to 0 |
| Q63376036 | Exponential shapelets: basis functions for data analysis of isolated features |
| Q58489848 | First Catalog of Strong Lens Candidates in the COSMOS Field |
| Q58919308 | First lensing measurements of SZ-detected clusters |
| Q58492576 | Flexion measurement in simulations of Hubble Space Telescope data |
| Q59782742 | Frontier Fields: Subaru weak-lensing analysis of the merging galaxy cluster A2744 |
| Q59733327 | Galaxies in X-ray groups. II. A weak lensing study of halo centering |
| Q57340956 | Gravitational Lensing Accuracy Testing 2010 (GREAT10) Challenge Handbook |
| Q58489822 | Handbook for the GREAT08 Challenge: An image analysis competition for cosmological lensing |
| Q58489686 | Hubble Frontier Fields: a high-precision strong-lensing analysis of galaxy cluster MACSJ0416.1-2403 using ∼200 multiple images |
| Q59739493 | Hubble Frontier Fields: a high-precision strong-lensing analysis of the massive galaxy cluster Abell 2744 using ∼180 multiple images |
| Q58489673 | Hubble Frontier Fields: the geometry and dynamics of the massive galaxy cluster merger MACSJ0416.1-2403 |
| Q60909558 | Image analysis for cosmology: results from the GREAT10 star challenge |
| Q58910152 | Image simulation with shapelets |
| Q58916068 | Large Structures and Galaxy Evolution in COSMOS at z < 1.1 |
| Q58489741 | New constraints on the evolution of the stellar-to-dark matter connection: a combined analysis of galaxy-galaxy lensing, clustering, and stellar mass functions from z = 0.2 to z =1 |
| Q57308642 | On dark peaks and missing mass: a weak-lensing mass reconstruction of the merging cluster system A520 |
| Q58908896 | On the contribution of large-scale structure to strong gravitational lensing |
| Q59747039 | Origins of weak lensing systematics, and requirements on future instrumentation (or knowledge of instrumentation) |
| Q59285144 | Overview of the SuperNova/Acceleration Probe (SNAP) |
| Q58908835 | Pixel-based correction for Charge Transfer Inefficiency in the Hubble Space Telescope Advanced Camera for Surveys |
| Q112108948 | PyAutoLens: Open-Source Strong Gravitational Lensing |
| Q58908018 | Quantifying the abundance of faint, low-redshift satellite galaxies in the COSMOS survey |
| Q121287366 | RXJ0437+00: constraining dark matter with exotic gravitational lenses |
| Q58908802 | Radio galaxy feedback in x-ray-selected groups from COSMOS: the effect on the intracluster medium |
| Q58490107 | Results of the GREAT08 Challenge: an image analysis competition for cosmological lensing |
| Q91666602 | Robust diffraction-limited near-infrared-to-near-ultraviolet wide-field imaging from stratospheric balloon-borne platforms-Super-pressure Balloon-borne Imaging Telescope performance |
| Q59846386 | SNAP NIR detectors |
| Q59846257 | SNAP Telescope |
| Q59846433 | SNAP Telescope |
| Q59846408 | SNAP focal plane |
| Q59846390 | SNAP: an integral field spectrograph for supernova identification |
| Q57497257 | Scientific Synergy between LSST and Euclid |
| Q58923211 | Self-interacting dark matter scattering rates through cosmic time |
| Q56908323 | Space-quality data from balloon-borne telescopes: The High Altitude Lensing Observatory (HALO) |
| Q58908862 | Stellar and total baryon mass fractions in groups and clusters since redshift 1 |
| Q58908933 | The Angular Correlations of Galaxies in the COSMOS Field |
| Q58489894 | The COSMOS Survey: Hubble Space Telescope Advanced Camera for Surveys Observations and Data Processing |
| Q58035509 | The COSMOS density field: a reconstruction using both weak lensing and galaxy distributions |
| Q58489901 | The Cosmic Evolution Survey (COSMOS): A Large‐Scale Structure atz = 0.73 and the Relation of Galaxy Morphologies to Local Environment |
| Q58489903 | The Evolution of the Number Density of Large Disk Galaxies in COSMOS |
| Q58489905 | The First Release COSMOS Optical and Near‐IR Data and Catalog |
| Q58489869 | The Hα Luminosity Function and Star Formation Rate at z ≈ 0.24 in the COSMOS 2 Square Degree Field |
| Q58489906 | The Redshift Evolution of Early‐Type Galaxies in COSMOS: Do Massive Early‐Type Galaxies Form by Dry Mergers? |
| Q58490116 | The Shear Testing Programme 2: Factors affecting high-precision weak-lensing analyses |
| Q59699985 | The Shear Testing Programme – I. Weak lensing analysis of simulated ground-based observations |
| Q58489897 | The XMM‐Newton Wide‐Field Survey in the COSMOS Field. III. Optical Identification and Multiwavelength Properties of a Large Sample of X‐Ray–Selected Sources |
| Q29028333 | The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827 |
| Q58489801 | The buildup of the Hubble sequence in the cosmos field |
| Q63377289 | The core of the massive cluster merger MACS J0417.5−1154 as seen by VLT/MUSE |
| Q59733332 | The correlated formation histories of massive galaxies and their dark matter halos |
| Q114823773 | The distribution of dark matter and gas spanning 6 Mpc around the post-merger galaxy cluster MS 0451−03 |
| Q58923108 | The diverse density profiles of galaxy clusters with self-interacting dark matter plus baryons |
| Q59868930 | The extraordinary amount of substructure in theHubble Frontier Fieldscluster Abell 2744 |
| Q68481638 | The nongravitational interactions of dark matter in colliding galaxy clusters |
| Q58923214 | The offsets between galaxies and their dark matter in Λ cold dark matter |
| Q58489804 | The opacity of galactic disks at z ~ 0.7 |
| Q112108631 | The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles |
| Q58490085 | The third gravitational lensing accuracy testing (GREAT3) challenge handbook |
| Q58035406 | The zCOSMOS redshift survey: evolution of the light in bulges and discs since z ~ 0.8 |
| Q58489899 | TheXMM‐NewtonWide‐Field Survey in the COSMOS Field: Statistical Properties of Clusters of Galaxies |
| Q36972702 | Warm-hot baryons comprise 5-10 per cent of filaments in the cosmic web |
| Q58489912 | Weak Gravitational Lensing with COSMOS: Galaxy Selection and Shape Measurements |
| Q58908471 | Weak lensing calibrated M-T scaling relation of galaxy groups in the COSMOS field^{sstarf}^ |
| Q59285137 | Weak lensing from space I: instrumentation and survey strategy |
| Q58489747 | Weak lensing measurement of galaxy clusters in the CFHTLS-wide survey |
| Q59452007 | What if LIGO’s gravitational wave detections are strongly lensed by massive galaxy clusters? |
| Q59285142 | Wide-Field Surveys from the SNAP Mission |
| Q114437843 | Alexandre Réfrégier | doctoral student | P185 |
| Richard Massey | wikipedia | |
| ta | இரிச்சர்டு மாசே | wikipedia |
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