A4 Vertaisarvioitu artikkeli konferenssijulkaisussa
TELAMON: Effelsberg Monitoring of AGN Jets with Very-High-Energy Astroparticle Emissions
Tekijät: Kadler 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.
Toimittaja: N/A
Konferenssin vakiintunut nimi: International Cosmic Ray Conference
Kustantaja: Sissa Medialab Srl
Julkaisuvuosi: 2022
Journal: POS Proceedings of Science
Kokoomateoksen nimi: 37th International Cosmic Ray Conference (ICRC2021)
Tietokannassa oleva lehden nimi: Proceedings of Science
Sarjan nimi: POS Proceedings of Science
Vuosikerta: 395
Aloitussivu: 974
ISSN: 1824-8039
DOI: https://doi.org/10.22323/1.395.0974
Verkko-osoite: https://pos.sissa.it/395/974
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/178548321
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.
Ladattava julkaisu This is an electronic reprint of the original article. |