Home > Publications database > TeV flaring activity of the AGN PKS 0625-354 in November 2018 |
Preprint | PUBDB-2024-00633 |
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2024
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Report No.: arXiv:2401.07071
Abstract: Most $\gamma$-ray detected active galactic nuclei are blazars with one of their relativistic jets pointing towards the Earth. Only a few objects belong to the class of radio galaxies or misaligned blazars. Here, we investigate the nature of the object PKS 0625-354, its $\gamma$-ray flux and spectral variability and its broad-band spectral emission with observations from H.E.S.S., Fermi-LAT, Swift-XRT, and UVOT taken in November 2018. The H.E.S.S. light curve above 200 GeV shows an outburst in the first night of observations followed by a declining flux with a halving time scale of 5.9h. The $\gamma\gamma$-opacity constrains the upper limit of the angle between the jet and the line of sight to $\sim10^\circ$. The broad-band spectral energy distribution shows two humps and can be well fitted with a single-zone synchrotron self Compton emission model. We conclude that PKS 0625-354, as an object showing clear features of both blazars and radio galaxies, can be classified as an intermediate active galactic nuclei. Multi-wavelength studies of such intermediate objects exhibiting features of both blazars and radio galaxies are sparse but crucial for the understanding of the broad-band emission of $\gamma$-ray detected active galactic nuclei in general.
Keyword(s): galaxy, radio wave ; jet, relativistic ; emission, model ; AGN ; blazar ; spectral ; flux ; HESS ; GeV ; variability ; spectral energy distribution ; GLAST ; synchrotron ; TeV
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Journal Article
TeV flaring activity of the AGN PKS 0625–354 in November 2018
Astronomy and astrophysics 683, A70 (2024) [10.1051/0004-6361/202348063]
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