BAT AGN spectroscopic survey – XV: the high frequency radio cores of ultra-hard X-ray selected AGN

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dc.contributor.authorSmith, K. L.
dc.contributor.authorMushotzky, R. F.
dc.contributor.authorKoss, M.
dc.contributor.authorTrakhtenbrot, B.
dc.contributor.authorRicci, Claudio
dc.contributor.authorWong, O. I.
dc.contributor.authorBauer, F. E.
dc.contributor.authorRicci, F.
dc.contributor.authorVogel, S.
dc.contributor.authorStern, D.
dc.contributor.authorPowell, M. C.
dc.contributor.authorUrry, C. M.
dc.contributor.authorHarrison, F.
dc.contributor.authorMejia-Restrepo, J.
dc.contributor.authorOh, K.
dc.contributor.authorBaek, J.
dc.contributor.authorChun, A.
dc.date.accessioned2022-05-20T14:30:38Z
dc.date.available2022-05-20T14:30:38Z
dc.date.issued2019
dc.description.abstractWe have conducted 22 GHz radio imaging at 1 arcsec resolution of 100 low-redshift AGN selected at 14–195 keV by the Swift-BAT. We find a radio core detection fraction of 96 per cent, much higher than lower frequency radio surveys. Of the 96 radio-detected AGN, 55 have compact morphologies, 30 have morphologies consistent with nuclear star formation, and 11 have sub-kpc to kpc-scale jets. We find that the total radio power does not distinguish between nuclear star formation and jets as the origin of the radio emission. For 87 objects, we use optical spectroscopy to test whether AGN physical parameters are distinct between radio morphological types. We find that X-ray luminosities tend to be higher if the 22 GHz morphology is jet-like, but find no significant difference in other physical parameters. We find that the relationship between the X-ray and core radio luminosities is consistent with the LR/LX ∼ 10−5 of coronally active stars. We further find that the canonical fundamental planes of black hole activity systematically overpredict our radio luminosities, particularly for objects with star formation morphologies.
dc.fuente.origenOUP
dc.identifier.doi10.1093/mnras/stz3608
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://ieeexplore.ieee.org/stamp/stamp.jsp?arnumber=9114176
dc.identifier.urihttps://doi.org/10.1093/mnras/stz3608
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/64248
dc.information.autorucInstituto de astrofísica ; Ricci, Claudio ; S/I ; 1015217
dc.information.autorucInstituto de astrofísica ; Bauer, Franz Erik ; S/I ; 1007961
dc.issue.numero3
dc.language.isoen
dc.nota.accesoContenido parcial
dc.pagina.final4234
dc.pagina.inicio4216
dc.publisherOUP
dc.revistaMonthly Notices of the Royal Astronomical Society
dc.rightsacceso restringido
dc.titleBAT AGN spectroscopic survey – XV: the high frequency radio cores of ultra-hard X-ray selected AGNes_ES
dc.typeartículo
dc.volumen492
sipa.codpersvinculados1015217
sipa.codpersvinculados1007961
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