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dc.contributor.authorGraham, P.
dc.contributor.authorTingay, Steven
dc.date.accessioned2017-01-30T12:54:15Z
dc.date.available2017-01-30T12:54:15Z
dc.date.created2014-04-10T20:00:52Z
dc.date.issued2014
dc.identifier.citationGraham, P. J. and Tingay, S. J. 2014. The importance of jet bending in gamma-ray AGNs- revisited. The Astrophysical Journal. 784 (2):159.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/26588
dc.identifier.doi10.1088/0004-637X/784/2/159
dc.description.abstract

We investigate the hypothesis that γ-ray-quiet active galactic nuclei (AGNs) have a greater tendency for jet bending than γ-ray-loud AGNs, revisiting the analysis of Tingay et al. We perform a statistical analysis using a large sample of 351 radio-loud AGNs along with γ-ray identifications from the Fermi Large Area Telescope (LAT). Our results show no statistically significant differences in jet-bending properties between γ-ray-loud and γ-ray-quiet populations, indicating that jet bending is not a significant factor for γ-ray detection in AGNs.

dc.publisherIOP Publishing Ltd.
dc.subjectOnline-only material: machine-readable tables
dc.subjectquasars: general
dc.subjectgalaxies: active - galaxies: jets - gamma rays: general
dc.titleThe importance of jet bending in gamma-ray AGNs - revisited
dc.typeJournal Article
dcterms.source.volume784
dcterms.source.number159
dcterms.source.startPage1
dcterms.source.endPage6
dcterms.source.issn0004-637X
dcterms.source.titleThe Astrophysical Journal
curtin.note

© 2014. The American Astronomical Society. All rights reserved.

curtin.department
curtin.accessStatusOpen access


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