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




TekijätKadler 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.

ToimittajaN/A

Konferenssin vakiintunut nimiInternational Cosmic Ray Conference

KustantajaSissa Medialab Srl

Julkaisuvuosi2022

JournalPOS Proceedings of Science

Kokoomateoksen nimi37th International Cosmic Ray Conference (ICRC2021)

Tietokannassa oleva lehden nimiProceedings of Science

Sarjan nimiPOS Proceedings of Science

Vuosikerta395

Aloitussivu974

ISSN1824-8039

DOIhttps://doi.org/10.22323/1.395.0974

Verkko-osoitehttps://pos.sissa.it/395/974

Rinnakkaistallenteen osoitehttps://research.utu.fi/converis/portal/detail/Publication/178548321


Tiivistelmä

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