Compacting frequent star patterns in RDF graphs

dc.bibliographicCitation.firstPage561eng
dc.bibliographicCitation.lastPage585eng
dc.bibliographicCitation.volume55eng
dc.contributor.authorKarim, Farah
dc.contributor.authorVidal, Maria-Esther
dc.contributor.authorAuer, Sören
dc.date.accessioned2021-05-07T06:29:40Z
dc.date.available2021-05-07T06:29:40Z
dc.date.issued2020
dc.description.abstractKnowledge graphs have become a popular formalism for representing entities and their properties using a graph data model, e.g., the Resource Description Framework (RDF). An RDF graph comprises entities of the same type connected to objects or other entities using labeled edges annotated with properties. RDF graphs usually contain entities that share the same objects in a certain group of properties, i.e., they match star patterns composed of these properties and objects. In case the number of these entities or properties in these star patterns is large, the size of the RDF graph and query processing are negatively impacted; we refer these star patterns as frequent star patterns. We address the problem of identifying frequent star patterns in RDF graphs and devise the concept of factorized RDF graphs, which denote compact representations of RDF graphs where the number of frequent star patterns is minimized. We also develop computational methods to identify frequent star patterns and generate a factorized RDF graph, where compact RDF molecules replace frequent star patterns. A compact RDF molecule of a frequent star pattern denotes an RDF subgraph that instantiates the corresponding star pattern. Instead of having all the entities matching the original frequent star pattern, a surrogate entity is added and related to the properties of the frequent star pattern; it is linked to the entities that originally match the frequent star pattern. Since the edges between the entities and the objects in the frequent star pattern are replaced by edges between these entities and the surrogate entity of the compact RDF molecule, the size of the RDF graph is reduced. We evaluate the performance of our factorization techniques on several RDF graph benchmarks and compare with a baseline built on top gSpan, a state-of-the-art algorithm to detect frequent patterns. The outcomes evidence the efficiency of proposed approach and show that our techniques are able to reduce execution time of the baseline approach in at least three orders of magnitude. Additionally, RDF graph size can be reduced by up to 66.56% while data represented in the original RDF graph is preserved.eng
dc.description.versionacceptedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/6168
dc.identifier.urihttps://doi.org/10.34657/5215
dc.language.isoengeng
dc.publisherDordrecht : Springer Science + Business Media B.Veng
dc.relation.doihttps://doi.org/10.1007/s10844-020-00595-9
dc.relation.essn1573-7675
dc.relation.ispartofseriesJournal of Intelligent Information Systems 55 (2020)eng
dc.rights.licenseEs gilt deutsches Urheberrecht. Das Dokument darf zum eigenen Gebrauch kostenfrei genutzt, aber nicht im Internet bereitgestellt oder an Außenstehende weitergegeben werden.eng
dc.subjectSemantic Webger
dc.subjectRDF compactionger
dc.subjectLinked datager
dc.subjectKnowledge graphger
dc.subject.ddc020eng
dc.titleCompacting frequent star patterns in RDF graphseng
dc.typearticleeng
dc.typeTexteng
dcterms.bibliographicCitation.journalTitleJournal of Intelligent Information Systemseng
tib.accessRightsopenAccesseng
wgl.contributorTIBeng
wgl.subjectInformatikeng
wgl.typeZeitschriftenartikeleng
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