TELAMON: Effelsberg Monitoring of AGN Jets with Very-High-Energy Astroparticle Emissions

dc.contributor.authorKadler M.
dc.contributor.authorBach U.
dc.contributor.authorBerge D.
dc.contributor.authorBuson S.
dc.contributor.authorDorner D.
dc.contributor.authorEdwards P.G.
dc.contributor.authorEppel F.
dc.contributor.authorGiroletti M.
dc.contributor.authorGokus A.
dc.contributor.authorHervet O.
dc.contributor.authorHeßdörfer J.
dc.contributor.authorKoyama S.
dc.contributor.authorKraus A.
dc.contributor.authorKrichbaum T.P.
dc.contributor.authorLindfors E.
dc.contributor.authorMannheim K.
dc.contributor.authorde Menezes R.
dc.contributor.authorOjha R.
dc.contributor.authorParaschos G.F.
dc.contributor.authorPueschel E.
dc.contributor.authorRösch F.
dc.contributor.authorRos E.
dc.contributor.authorSchleicher B.
dc.contributor.authorSinapius J.
dc.contributor.authorSitarek J.
dc.contributor.authorWilms J.
dc.contributor.authorZacharias M.
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-id178548321
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/178548321
dc.date.accessioned2025-08-27T23:53:04Z
dc.date.available2025-08-27T23:53:04Z
dc.description.abstract<p>We introduce the TELAMON program, which is using the Effelsberg 100-m telescope to monitor the radio spectra of active galactic nuclei (AGN) under scrutiny in astroparticle physics, namely TeV blazars and candidate neutrino-associated AGN. Thanks to its large dish aperture and sensitive instrumentation, the Effelsberg telescope can yield superior radio data over other programs in the low flux-density regime down to several 10 mJy. This is a particular strength in the case of TeV-emitting blazars, which are often comparatively faint radio sources of the high-synchrotron peaked type.</p><p>We perform high-cadence high-frequency observations every 2-4 weeks at multiple frequencies up to 44 GHz. This setup is well suited to trace dynamical processes in the compact parsec-scale jets of blazars related to high-energy flares or neutrino detections. Our sample currently covers about 40 sources and puts its focus on AGN with very-high-energy astroparticle emission, i.e., TeV blazars and neutrino-associated AGN. Here, we introduce the TELAMON program characteristics and present first results obtained since fall 2020.</p>
dc.format.pagerange974
dc.identifier.issn1824-8039
dc.identifier.jour-issn1824-8039
dc.identifier.olddbid204794
dc.identifier.oldhandle10024/187821
dc.identifier.urihttps://www.utupub.fi/handle/11111/53511
dc.identifier.urlhttps://pos.sissa.it/395/974
dc.identifier.urnURN:NBN:fi-fe2023021627483
dc.language.isoen
dc.okm.affiliatedauthorLindfors, Elina
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.typeA4 Conference Article
dc.publisher.countryItalyen_GB
dc.publisher.countryItaliafi_FI
dc.publisher.country-codeIT
dc.relation.conferenceInternational Cosmic Ray Conference
dc.relation.doi10.22323/1.395.0974
dc.relation.ispartofjournalPOS Proceedings of Science
dc.relation.ispartofseriesPOS Proceedings of Science
dc.relation.volume395
dc.source.identifierhttps://www.utupub.fi/handle/10024/187821
dc.titleTELAMON: Effelsberg Monitoring of AGN Jets with Very-High-Energy Astroparticle Emissions
dc.title.book37th International Cosmic Ray Conference (ICRC2021)
dc.year.issued2022

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