PoS - Proceedings of Science
Volume 395 - 37th International Cosmic Ray Conference (ICRC2021) - MM - Multi-Messenger
TELAMON: Monitoring of AGN with the Effelsberg 100-m Telescope in the Context of Astroparticle Physics
M. Kadler*, U. Bach, D. Berge, S. Buson, D. Dorner, P.G. Edwards, F. Eppel, M. Giroletti, A. Gokus, O. Hervet, J. Hessdoerfer, S. Koyama, A. Kraus, T. Krichbaum, E. Lindfors, K. Mannheim, R. de Menezes, R. Ojha, G. Paraschos, E. Pueschel, F. Rösch, E. Ros, B. Schleicher, J.L. Sinapius, J. Sitarek, J. Wilms and M. Zachariaset al. (click to show)
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Pre-published on: July 31, 2021
Published on: March 18, 2022
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.
DOI: https://doi.org/10.22323/1.395.0974
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