FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1925792681> ?p ?o ?g. }

• W1925792681 endingPage "1088" @default.
• W1925792681 startingPage "1073" @default.
• W1925792681 abstract "(Abridged) We quantify the bias and scatter in galaxy cluster masses and concentrations derived from an idealised mock weak gravitational lensing (WL) survey, and their effect on the cluster mass-concentration relation. For this, we simulate WL distortions on a population of background galaxies due to a large (~3000) sample of galaxy cluster haloes extracted from the Millennium Simulation at z~0.2. This study takes into account the influence of shape noise, cluster substructure and asphericity as well as correlated large-scale structure, but not uncorrelated large-scale structure along the line of sight and observational effects. We find a small, but non-negligble, negative median bias in both mass and concentration at a level of ~5%, the exact value depending both on cluster mass and radial survey range. Both the mass and concentration derived from WL show considerable scatter about their true values. This scatter has, even for the highest mass clusters of M200 > 10^14.8 M_sun, a level of ~30% and ~20% for concentration and mass respectively and increases strongly with decreasing cluster mass. For a typical survey analysing 30 galaxies per arcmin^2 over a radial range from 30 to 15' from the cluster centre, the derived M200-c relation has a slope and normalisation too low compared to the underlying true (3D) relation by ~40% and ~15% respectively. The scatter and bias in mass are shown to reflect a departure at large radii of the true WL shear/matter distribution of the simulated clusters from the NFW profile adopted in modelling the mock observations. Orientation of the triaxial cluster haloes dominates the concentration scatter (except at low masses, where galaxy shape noise becomes dominant), while the bias in c is mostly due to substructure within the virial radius." @default.
• W1925792681 created "2016-06-24" @default.
• W1925792681 creator A5016823102 @default.
• W1925792681 creator A5033973593 @default.
• W1925792681 creator A5035122637 @default.
• W1925792681 date "2012-01-23" @default.
• W1925792681 modified "2023-09-25" @default.
• W1925792681 title "Mock weak lensing analysis of simulated galaxy clusters: bias and scatter in mass and concentration" @default.
• W1925792681 cites W1672666614 @default.
• W1925792681 cites W1897873612 @default.
• W1925792681 cites W1921097980 @default.
• W1925792681 cites W1968752888 @default.
• W1925792681 cites W1974542762 @default.
• W1925792681 cites W1977282636 @default.
• W1925792681 cites W1997235862 @default.
• W1925792681 cites W1997254864 @default.
• W1925792681 cites W2007559135 @default.
• W1925792681 cites W2015904699 @default.
• W1925792681 cites W2026261559 @default.
• W1925792681 cites W2026341740 @default.
• W1925792681 cites W2031430331 @default.
• W1925792681 cites W2032627363 @default.
• W1925792681 cites W2039490501 @default.
• W1925792681 cites W2039971612 @default.
• W1925792681 cites W2045821305 @default.
• W1925792681 cites W2063150651 @default.
• W1925792681 cites W2064289393 @default.
• W1925792681 cites W2070998352 @default.
• W1925792681 cites W2082153469 @default.
• W1925792681 cites W2084868634 @default.
• W1925792681 cites W2096186332 @default.
• W1925792681 cites W2100143236 @default.
• W1925792681 cites W2100382624 @default.
• W1925792681 cites W2105539567 @default.
• W1925792681 cites W2110563485 @default.
• W1925792681 cites W2123353468 @default.
• W1925792681 cites W2125856726 @default.
• W1925792681 cites W2133270107 @default.
• W1925792681 cites W2140466930 @default.
• W1925792681 cites W2141449818 @default.
• W1925792681 cites W2141709306 @default.
• W1925792681 cites W2141968105 @default.
• W1925792681 cites W2147875900 @default.
• W1925792681 cites W2156048499 @default.
• W1925792681 cites W2158236716 @default.
• W1925792681 cites W2166616205 @default.
• W1925792681 cites W2167335950 @default.
• W1925792681 cites W2953228579 @default.
• W1925792681 cites W3099027360 @default.
• W1925792681 cites W3100110286 @default.
• W1925792681 cites W3100437165 @default.
• W1925792681 cites W3101256601 @default.
• W1925792681 cites W3103266369 @default.
• W1925792681 cites W3103850807 @default.
• W1925792681 cites W3103877238 @default.
• W1925792681 cites W3104625974 @default.
• W1925792681 cites W3104882445 @default.
• W1925792681 cites W3105489959 @default.
• W1925792681 cites W3105595725 @default.
• W1925792681 cites W3106262625 @default.
• W1925792681 cites W3123302290 @default.
• W1925792681 cites W3125319234 @default.
• W1925792681 cites W4250548444 @default.
• W1925792681 doi "https://doi.org/10.1111/j.1365-2966.2011.20364.x" @default.
• W1925792681 hasPublicationYear "2012" @default.
• W1925792681 type Work @default.
• W1925792681 sameAs 1925792681 @default.
• W1925792681 citedByCount "79" @default.
• W1925792681 countsByYear W19257926812012 @default.
• W1925792681 countsByYear W19257926812013 @default.
• W1925792681 countsByYear W19257926812014 @default.
• W1925792681 countsByYear W19257926812015 @default.
• W1925792681 countsByYear W19257926812016 @default.
• W1925792681 countsByYear W19257926812017 @default.
• W1925792681 countsByYear W19257926812018 @default.
• W1925792681 countsByYear W19257926812019 @default.
• W1925792681 countsByYear W19257926812020 @default.
• W1925792681 countsByYear W19257926812021 @default.
• W1925792681 countsByYear W19257926812022 @default.
• W1925792681 countsByYear W19257926812023 @default.
• W1925792681 crossrefType "journal-article" @default.
• W1925792681 hasAuthorship W1925792681A5016823102 @default.
• W1925792681 hasAuthorship W1925792681A5033973593 @default.
• W1925792681 hasAuthorship W1925792681A5035122637 @default.
• W1925792681 hasBestOaLocation W19257926811 @default.
• W1925792681 hasConcept C121332964 @default.
• W1925792681 hasConcept C127413603 @default.
• W1925792681 hasConcept C134222618 @default.
• W1925792681 hasConcept C144024400 @default.
• W1925792681 hasConcept C149923435 @default.
• W1925792681 hasConcept C156055797 @default.
• W1925792681 hasConcept C159249277 @default.
• W1925792681 hasConcept C159985019 @default.
• W1925792681 hasConcept C164866538 @default.
• W1925792681 hasConcept C190670322 @default.
• W1925792681 hasConcept C192562407 @default.
• W1925792681 hasConcept C199360897 @default.
• W1925792681 hasConcept C204323151 @default.

• next