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TELAMON: Effelsberg monitoring of AGN jets with very-high-energy astroparticle emission -- I. Program description and sample characterization

Authors :
Eppel, F.
Kadler, M.
Heßdörfer, J.
Benke, P.
Debbrecht, L.
Eich, J.
Gokus, A.
Hämmerich, S.
Kirchner, D.
Paraschos, G. F.
Rösch, F.
Schulga, W.
Sinapius, J.
Weber, P.
Bach, U.
Dorner, D.
Edwards, P. G.
Giroletti, M.
Kraus, A.
Hervet, O.
Koyama, S.
Krichbaum, T. P.
Mannheim, K.
Ros, E.
Zacharias, M.
Zensus, J. A.
Publication Year :
2024

Abstract

Aims. 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.<br />Comment: 16 pages, 11 figures, 4 tables, accepted for publication in A&A

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2401.06296
Document Type :
Working Paper