Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/1170
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dc.contributor.authorKnežević, Zoranen_US
dc.contributor.authorMilani, Andreaen_US
dc.contributor.authorCellino, Albertoen_US
dc.contributor.authorNovaković, Bojanen_US
dc.contributor.authorSpoto, Federicaen_US
dc.contributor.authorPaolicchi, Paoloen_US
dc.date.accessioned2022-09-23T17:57:44Z-
dc.date.available2022-09-23T17:57:44Z-
dc.date.issued2014-01-01-
dc.identifier.issn17439213en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/1170-
dc.description.abstractWe have recently proposed a new approach to the asteroid family classification by combining the classical HCM method with an automated procedure to add newly discovered members to existing families. This approach is specifically intended to cope with ever increasing asteroid data sets, and consists of several steps to segment the problem and handle the very large amount of data in an efficient and accurate manner. We briefly present all these steps and show the results from three subsequent updates making use of only the automated step of attributing the newly numbered asteroids to the known families. We describe the changes of the individual families membership, as well as the evolution of the classification due to the newly added intersections between the families, resolved candidate family mergers, and emergence of the new candidates for the mergers. We thus demonstrate how by the new approach the asteroid family classification becomes stable in general terms (converging towards a permanent list of confirmed families), and in the same time evolving in details (to account for the newly discovered asteroids) at each update.en
dc.relation.ispartofProceedings of the International Astronomical Unionen_US
dc.subjectasteroid familiesen
dc.subjectasteroidsen
dc.subjectautomated classificationen
dc.titleAutomated Classification of Asteroids into Families at Worken_US
dc.typeConference Paperen_US
dc.identifier.doi10.1017/S1743921314008035-
dc.identifier.scopus2-s2.0-84930647713-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84930647713-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage130en_US
dc.relation.lastpage133en_US
dc.relation.volume9en_US
dc.relation.issueS310en_US
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.grantfulltextnone-
item.openairetypeConference Paper-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-6349-6881-
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