A4 Refereed article in a conference publication

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




AuthorsKadler M., Bach U., Berge D., Buson S., Dorner D., Edwards P.G., Eppel F., Giroletti M., Gokus A., Hervet O., Heßdörfer J., Koyama S., Kraus A., Krichbaum T.P., Lindfors E., Mannheim K., de Menezes R., Ojha R., Paraschos G.F., Pueschel E., Rösch F., Ros E., Schleicher B., Sinapius J., Sitarek J., Wilms J., Zacharias M.

EditorsN/A

Conference nameInternational Cosmic Ray Conference

PublisherSissa Medialab Srl

Publication year2022

JournalPOS Proceedings of Science

Book title 37th International Cosmic Ray Conference (ICRC2021)

Journal name in sourceProceedings of Science

Series titlePOS Proceedings of Science

Volume395

First page 974

ISSN1824-8039

DOIhttps://doi.org/10.22323/1.395.0974

Web address https://pos.sissa.it/395/974

Self-archived copy’s web addresshttps://research.utu.fi/converis/portal/detail/Publication/178548321


Abstract

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.

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.


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Last updated on 2025-27-03 at 21:57