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000601582 1001_ $$0P:(DE-HGF)0$$aEppel, F.$$b0$$eCorresponding author
000601582 245__ $$aTELAMON: Effelsberg monitoring of AGN jets with very-high-energy astroparticle emission -- I. Program description and sample characterization
000601582 260__ $$aLes Ulis$$bEDP Sciences$$c2024
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000601582 500__ $$a16 pages, 11 figures, 4 tables, accepted for publication in A&A
000601582 520__ $$aAims. 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, specifically TeV blazars and candidate neutrino-associated AGN. Here, we present and characterize our main sample of TeV-detected blazars. Methods. We analyze the data sample from the first ~2.5 years of observations between August 2020 and February 2023 in the range from 14 GHz to 45 GHz. During this pilot phase, we have observed all 59 TeV-detected blazars in the Northern Hemisphere (i.e., Dec. >0{\deg}) known at the time of observation. We discuss the basic data reduction and calibration procedures used for all TELAMON data and introduce a sub-band averaging method used to calculate average light curves for the sources in our sample. Results. The TeV-selected sources in our sample exhibit a median flux density of 0.12 Jy at 20 mm, 0.20 Jy at 14 mm and 0.60 Jy at 7 mm. The spectrum for most of the sources is consistent with a flat radio spectrum and we find a median spectral index ($S(\nu)\propto\nu^\alpha$) of $\alpha=-0.11$. Our results on flux density and spectral index are consistent with previous studies of TeV-selected blazars. Compared to the GeV-selected F-GAMMA sample, TELAMON sources are significantly fainter in the radio band. This is consistent with the double-humped spectrum of blazars being shifted towards higher frequencies for TeV-emitters (in particular for high-synchrotron peaked BL Lac type objects), which results in a lower radio flux density. The spectral index distribution of our TeV-selected blazar sample is not significantly different from the GeV-selected F-GAMMA sample. Moreover, we present a strategy to track the light curve evolution of sources in our sample for future variability and correlation analysis.
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000601582 536__ $$0G:(GEPRIS)447572188$$aDFG project 447572188 - VLBA Beobachtungen von Neutrino-Kandidaten Blazaren (447572188)$$c447572188$$x1
000601582 536__ $$0G:(GEPRIS)434448349$$aDFG project G:(GEPRIS)434448349 - TANAMI 2 – VLBI und Multiwellenlängen-Beobachtungen von AGN Jets des Südlichen Himmels (434448349)$$c434448349$$x2
000601582 536__ $$0G:(GEPRIS)465409577$$aDFG project G:(GEPRIS)465409577 - Radioüberwachung und hochauflösende Bildgebung von extremen Blazaren und anderen TeV-detektierten aktiven Galaxien mit dem Effelsberg 100-m Teleskop und dem Global Millimetre VLBI Array (465409577)$$c465409577$$x3
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000601582 7001_ $$aHeßdörfer, J.$$b2
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000601582 7001_ $$00009-0003-8342-4561$$aDebbrecht, L.$$b4
000601582 7001_ $$aEich, J.$$b5
000601582 7001_ $$00000-0002-5726-5216$$aGokus, A.$$b6
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000601582 7001_ $$aKirchner, D.$$b8
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000601582 7001_ $$aWeber, P.$$b13
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000601582 7001_ $$aDorner, D.$$b15
000601582 7001_ $$aEdwards, P. G.$$b16
000601582 7001_ $$aGiroletti, M.$$b17
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000601582 7001_ $$00000-0003-3878-1677$$aHervet, O.$$b19
000601582 7001_ $$00000-0002-3723-3372$$aKoyama, S.$$b20
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000601582 7001_ $$aZacharias, M.$$b24
000601582 7001_ $$00000-0001-7470-3321$$aZensus, J. A.$$b25
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