Compact Symmetric Objects. I. Toward a Comprehensive Bona Fide Catalog

dc.contributor.authorKiehlmann S
dc.contributor.authorLister M
dc.contributor.authorReadhead A
dc.contributor.authorLiodakis I
dc.contributor.authorO’Neill S
dc.contributor.authorPearson T
dc.contributor.authorSheldahl E
dc.contributor.authorSiemiginowska A
dc.contributor.authorTassis K
dc.contributor.authorTaylor G
dc.contributor.authorWilkinson P
dc.contributor.organizationfi=Suomen ESO-keskus|en=Finnish Centre for Astronomy with ESO|
dc.contributor.organization-code1.2.246.10.2458963.20.54954054844
dc.converis.publication-id386823989
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/386823989
dc.date.accessioned2025-08-28T03:24:14Z
dc.date.available2025-08-28T03:24:14Z
dc.description.abstract<p>Compact symmetric objects (CSOs) are jetted active galactic nuclei (AGN) with overall projected size <1 kpc. The classification was introduced to distinguish these objects from the majority of compact jetted AGN in centimeter-wavelength very long baseline interferometry observations, where the observed emission is relativistically boosted toward the observer. The original classification criteria for CSOs were (i) evidence of emission on both sides of the center of activity and (ii) overall size <1 kpc. However, some relativistically boosted objects with jet axes close to the line of sight appear symmetric and have been misclassified as CSOs, thereby undermining the CSO classification. This is because two essential CSO properties, pointed out in the original papers, have been neglected: (iii) low variability and (iv) low apparent speeds along the jets. As a first step toward creating a comprehensive catalog of “bona fide” CSOs, we identify 79 bona fide CSOs, including 15 objects claimed as confirmed CSOs here for the first time, that match the CSO selection criteria. This sample of bona fide CSOs can be used for astrophysical studies of CSOs without contamination by misclassified CSOs. We show that the fraction of CSOs in complete flux density limited AGN samples with S<sub>5GHz</sub> > 700 mJy is between (6.8 ± 1.6)% and (8.5 ± 1.8)%. © 2024. The Author(s). Published by the American Astronomical Society.<br></p>
dc.identifier.eissn1538-4357
dc.identifier.jour-issn0004-637X
dc.identifier.olddbid210626
dc.identifier.oldhandle10024/193653
dc.identifier.urihttps://www.utupub.fi/handle/11111/53822
dc.identifier.urlhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85184028418&doi=10.3847%2f1538-4357%2fad0c56&partnerID=40&md5=607fc6b49954614a05c7b3a817599efb
dc.identifier.urnURN:NBN:fi-fe2025082786707
dc.language.isoen
dc.okm.affiliatedauthorLiodakis, Yannis
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherInstitute of Physics
dc.publisher.countryUnited Statesen_GB
dc.publisher.countryYhdysvallat (USA)fi_FI
dc.publisher.country-codeUS
dc.relation.articlenumber240
dc.relation.doi10.3847/1538-4357/ad0c56
dc.relation.ispartofjournalAstrophysical Journal
dc.relation.issue2
dc.relation.volume961
dc.source.identifierhttps://www.utupub.fi/handle/10024/193653
dc.titleCompact Symmetric Objects. I. Toward a Comprehensive Bona Fide Catalog
dc.year.issued2024

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