FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100198162> ?p ?o ?g. }

• W3100198162 endingPage "20" @default.
• W3100198162 startingPage "10" @default.
• W3100198162 abstract "We present an estimation of the expected number of arcs and arclets in a survey of nearby (z < 0.1) clusters of galaxies, which takes into account the observational constraints. We show that strong lensing effects are not common, but also that they are not as rare as usually stated. Indeed, for a given cluster, the predicted number of arcs strongly depends on the magnitude limit of the survey and the actual value of the seeing. We also describe the procedures and results of a search for gravitational arcs and arclets in a sample of 33 galaxy clusters, representative of the local cluster distribution and spanning the redshift range of 0.014 < z < 0.076. Only one new arc candidate was discovered, located ~3 arcmin away from the center of the cluster Abell 3266 (z = 0.059), whose redshift was found to be z = 0.073. The assumption that a mass concentration around a bright cluster elliptical 166 away from the arc candidate could explain this arc as a gravitational image requires the presence of a very massive substructure in this cluster (M/LV ~ 163 M⊙/L⊙). Although such substructure cannot be completely discarded, the nature of the arc candidate most possibly corresponds to a disk galaxy belonging to A3266. Our simplified theoretical model predicts that the probability of finding at least one gravitational arc in the sample investigated is 25%, in good agreement with the actual number of arcs found, N = 1 or 0, either adopting the arc in A3266 as a gravitational image or not. We conclude that a deep survey of the central regions of low-z galaxy clusters, with very good image quality, should allow significant progress in the mapping of their central mass concentration." @default.
• W3100198162 created "2020-11-23" @default.
• W3100198162 creator A5004193106 @default.
• W3100198162 creator A5022523543 @default.
• W3100198162 creator A5024494537 @default.
• W3100198162 creator A5027207716 @default.
• W3100198162 creator A5034507379 @default.
• W3100198162 creator A5039473712 @default.
• W3100198162 creator A5077584906 @default.
• W3100198162 creator A5088474517 @default.
• W3100198162 date "2001-01-01" @default.
• W3100198162 modified "2023-10-17" @default.
• W3100198162 title "Gravitational Lensing by Nearby Clusters of Galaxies" @default.
• W3100198162 cites W142889368 @default.
• W3100198162 cites W1555895019 @default.
• W3100198162 cites W1583752947 @default.
• W3100198162 cites W1980290308 @default.
• W3100198162 cites W1997681753 @default.
• W3100198162 cites W2003230980 @default.
• W3100198162 cites W2008741599 @default.
• W3100198162 cites W2019119271 @default.
• W3100198162 cites W2019185840 @default.
• W3100198162 cites W2019511225 @default.
• W3100198162 cites W2027975819 @default.
• W3100198162 cites W2030326695 @default.
• W3100198162 cites W2038845640 @default.
• W3100198162 cites W2044476843 @default.
• W3100198162 cites W2056903171 @default.
• W3100198162 cites W2064895468 @default.
• W3100198162 cites W2066317414 @default.
• W3100198162 cites W2068095967 @default.
• W3100198162 cites W2071886800 @default.
• W3100198162 cites W2083432196 @default.
• W3100198162 cites W2087525524 @default.
• W3100198162 cites W2092916207 @default.
• W3100198162 cites W2106248946 @default.
• W3100198162 cites W2142238829 @default.
• W3100198162 cites W2144913687 @default.
• W3100198162 cites W2151876949 @default.
• W3100198162 cites W3098398738 @default.
• W3100198162 cites W3099001851 @default.
• W3100198162 cites W3099709479 @default.
• W3100198162 cites W3102075459 @default.
• W3100198162 cites W3103827746 @default.
• W3100198162 cites W4229934221 @default.
• W3100198162 cites W4301426066 @default.
• W3100198162 doi "https://doi.org/10.1086/318010" @default.
• W3100198162 hasPublicationYear "2001" @default.
• W3100198162 type Work @default.
• W3100198162 sameAs 3100198162 @default.
• W3100198162 citedByCount "14" @default.
• W3100198162 countsByYear W31001981622013 @default.
• W3100198162 countsByYear W31001981622016 @default.
• W3100198162 countsByYear W31001981622017 @default.
• W3100198162 countsByYear W31001981622020 @default.
• W3100198162 countsByYear W31001981622022 @default.
• W3100198162 crossrefType "journal-article" @default.
• W3100198162 hasAuthorship W3100198162A5004193106 @default.
• W3100198162 hasAuthorship W3100198162A5022523543 @default.
• W3100198162 hasAuthorship W3100198162A5024494537 @default.
• W3100198162 hasAuthorship W3100198162A5027207716 @default.
• W3100198162 hasAuthorship W3100198162A5034507379 @default.
• W3100198162 hasAuthorship W3100198162A5039473712 @default.
• W3100198162 hasAuthorship W3100198162A5077584906 @default.
• W3100198162 hasAuthorship W3100198162A5088474517 @default.
• W3100198162 hasBestOaLocation W31001981622 @default.
• W3100198162 hasConcept C121332964 @default.
• W3100198162 hasConcept C124017977 @default.
• W3100198162 hasConcept C1276947 @default.
• W3100198162 hasConcept C138125448 @default.
• W3100198162 hasConcept C156055797 @default.
• W3100198162 hasConcept C190670322 @default.
• W3100198162 hasConcept C33024259 @default.
• W3100198162 hasConcept C38437897 @default.
• W3100198162 hasConcept C44870925 @default.
• W3100198162 hasConcept C68498078 @default.
• W3100198162 hasConcept C98444146 @default.
• W3100198162 hasConceptScore W3100198162C121332964 @default.
• W3100198162 hasConceptScore W3100198162C124017977 @default.
• W3100198162 hasConceptScore W3100198162C1276947 @default.
• W3100198162 hasConceptScore W3100198162C138125448 @default.
• W3100198162 hasConceptScore W3100198162C156055797 @default.
• W3100198162 hasConceptScore W3100198162C190670322 @default.
• W3100198162 hasConceptScore W3100198162C33024259 @default.
• W3100198162 hasConceptScore W3100198162C38437897 @default.
• W3100198162 hasConceptScore W3100198162C44870925 @default.
• W3100198162 hasConceptScore W3100198162C68498078 @default.
• W3100198162 hasConceptScore W3100198162C98444146 @default.
• W3100198162 hasIssue "1" @default.
• W3100198162 hasLocation W31001981621 @default.
• W3100198162 hasLocation W31001981622 @default.
• W3100198162 hasOpenAccess W3100198162 @default.
• W3100198162 hasPrimaryLocation W31001981621 @default.
• W3100198162 hasRelatedWork W1588125547 @default.
• W3100198162 hasRelatedWork W1616562941 @default.
• W3100198162 hasRelatedWork W2002403941 @default.
• W3100198162 hasRelatedWork W2093330278 @default.
• W3100198162 hasRelatedWork W2137863141 @default.

• next