About: Simona Mei

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An Entity of Type : foaf:Person, within Data Space : data.idref.fr associated with source document(s)

Attributes	Values
type	Person
sameAs	Mei, Simona (19..-....) Mei, Simona (19..-....)
Life Event	http://www.idref.fr/161266487/birth
preferred label	Mei, Simona (19..-....)
name	Simona Mei
dbpedia-owl:citizenship	http://sws.geonames.org/3017382/
Language	http://lexvo.org/id/iso639-3/fra
Given name	Simona
familyName	Mei
has biographical i...tion (Deprecated)	Enseignant chercheur à l'université de Paris Diderot-Paris 7 (U.F.R. Physique ). Professeur d'Astrophysique à Université de Paris (en 2021)
gender	female
ORCID iD	0000-0002-2849-559X
Scopus ID	7102846243
is sameAs of	Mei, Simona (19..-....) Mei, Simona (19..-....)
is Thesis advisor of	http://www.sudoc.fr/177405716/id Galaxy cluster detection with optical and infrared imaging Evolution des propriétés structurelles des galaxies de type précoce dans différents environnements http://www.sudoc.fr/161266436/id http://www.sudoc.fr/184297834/id Propriétés et évolution des galaxies de type précoce à z ~1.3, Super-amas du lynx http://www.sudoc.fr/169784509/id L'assemblage de masse dans des galaxies à redshift intermédiaire http://www.sudoc.fr/25948718X/id http://www.sudoc.fr/234669950/id Scaling relations and stellar populations of galaxy clusters from their first epochs of assembly to the present http://www.sudoc.fr/202929981/id http://www.sudoc.fr/235456187/id http://www.sudoc.fr/236139762/id http://www.sudoc.fr/250012758/id http://www.sudoc.fr/271582758/id http://www.sudoc.fr/202926990/id http://www.sudoc.fr/256373787/id
is Praeses of	Régime non-linéaire de formation des structures cosmiques, empreintes sur la covariance du spectre de puissance et dynamique des inhomogénéités d'énergie noire http://www.sudoc.fr/190696753/id http://www.sudoc.fr/276035887/id http://www.sudoc.fr/234637498/id http://www.sudoc.fr/23589138X/id http://www.sudoc.fr/249359219/id http://www.sudoc.fr/274947048/id http://www.sudoc.fr/256418853/id http://www.sudoc.fr/268233675/id http://www.sudoc.fr/273645773/id http://www.sudoc.fr/264544110/id
is Author of	Euclid preparation. VIII. The Complete Calibration of the Colour–Redshift Relation survey: VLT/KMOS observations and data release THE NEXT GENERATION VIRGO CLUSTER SURVEY. IV. NGC 4216: A BOMBARDED SPIRAL IN THE VIRGO CLUSTER Euclid preparation. XVII. Cosmic Dawn Survey: Spitzer Space Telescope observations of the Euclid deep fields and calibration fields Spectroscopic Confirmation and Velocity Dispersions for 20 Planck Galaxy Clusters at 0.16 < z < 0.78 Science case and requirements for the MOSAIC concept for a multi-object spectrograph for the European Extremely Large Telescope Mass assembly and morphological transformations since z ∼ 3 from CANDELS An accurate cluster selection function for the J-PAS narrow-band wide-field survey Glimpsing the imprint of local environment on the galaxy stellar mass function The accelerated build-up of the red sequence in high-redshift galaxy clusters Chandra centres for COSMOS X-ray galaxy groups: differences in stellar properties between central dominant and offset brightest group galaxies Euclid: Forecasts for $k$-cut $3 \times 2$ Point Statistics The abundance and colours of galaxies in high-redshift clusters in the cold dark matter cosmology Properties of FIRBACK-ELAIS 175-μm sources in the ELAIS N2 region The Canada–France Imaging Survey: First Results from the u-Band Component The evolution of the mass-size relation for early-type galaxies from z ∼1 to the present: dependence on environment, mass range and detailed morphology Calibrating the Planck Cluster Mass Scale with Cluster Velocity Dispersions Euclid preparation Euclid preparation Euclid preparation. XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography Euclid preparation. XIII. Forecasts for galaxy morphology with the Euclid Survey using deep generative models HST Grism Confirmation of 16 Structures at 1.4 < z < 2.8 from the Clusters Around Radio-Loud AGN (CARLA) Survey Euclid: Cosmological forecasts from the void size function Euclid preparation. XXI. Intermediate-redshift contaminants in the search for $z>6$ galaxies within the Euclid Deep Survey Euclid preparation Planck intermediate results X. Physics of the hot gas in the Coma cluster Planck intermediate results. VI. The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusters Environmental dependence of bulge-dominated galaxy sizes in hierarchical models of galaxy formation. Comparison with the local Universe THE NEXT GENERATION VIRGO CLUSTER SURVEY. XX. RedGOLD BACKGROUND GALAXY CLUSTER DETECTIONS Euclid preparation. X. The Euclid photometric-redshift challenge Euclid: the selection of quiescent and star-forming galaxies using observed colours A catalog of polychromatic bulge-disc decompositions of ∼17.600 galaxies in CANDELS Erratum: “Virgo Redux: The Masses and Stellar Content of Nuclei in Early-type Galaxies from Multiband Photometry and Spectroscopy” (2017, ApJ, 849, 55) Massive molecular gas reservoir around the central AGN in the CARLA J1103 + 3449 cluster at z = 1.44★ Conditional quenching: a detailed look at the SFR−density relation at $z$ ∼ 0.9 from ORELSE Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments Euclid preparation. XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses The Next Generation Virgo Cluster Survey (NGVS). I. Introduction to the survey Euclid preparation. XXI. Intermediate-redshift contaminants in the search for z > 6 galaxies within the Euclid Deep Survey (Corrigendum) Euclid preparation Euclid preparation. VI. Verifying the performance of cosmic shear experiments Euclid preparation - VI. Verifying the Performance of Cosmic Shear Experiments (Corrigendum) Galaxy luminosities, stellar masses, sizes, velocity dispersions as a function of morphological type The structural properties of classical bulges and discs from z ∼ 2 The massive end of the luminosity and stellar mass functions: dependence on the fit to the light profile Euclid preparation. XIX. Impact of magnification on photometric galaxy clustering Euclid preparation Erratum: “The Next Generation Virgo Cluster Survey. X. Properties of Ultra-compact Dwarfs in the M87, M49, and M60 Regions” (2015, APJ, 812, 34) Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample Euclid preparation. III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selection THE NEXT GENERATION VIRGO CLUSTER SURVEY-INFRARED (NGVS-IR). I. A NEW NEAR-ULTRAVIOLET, OPTICAL, AND NEAR-INFRARED GLOBULAR CLUSTER SELECTION TOOL Euclid: Estimation of the Impact of Correlated Readout Noise for Flux Measurements with the Euclid NISP Instrument Euclid preparation. XXXV. Covariance model validation for the 2-point correlation function of galaxy clusters NO EVIDENCE FOR A DEPENDENCE OF THE MASS-SIZE RELATION OF EARLY-TYPE GALAXIES ON ENVIRONMENT IN THE LOCAL UNIVERSE THE NEXT GENERATION VIRGO CLUSTER SURVEY. V. MODELING THE DYNAMICS OF M87 WITH THE MADE-TO-MEASURE METHOD Systematic effects on the size–luminosity relations of early- and late-type galaxies: dependence on model fitting and morphology

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