Is PKS 0625-354 another variable TeV active galactic nucleus?
Dorit Glawion, Alicja Wierzcholska (for the H.E.S.S. Collaboration)

TL;DR
This paper reports the detection of gamma-ray variability in the active galaxy PKS 0625-354 using H.E.S.S. telescopes, providing new insights into gamma-ray emission mechanisms in non-blazar AGN.
Contribution
It presents the first detailed gamma-ray variability study of PKS 0625-354, challenging its classification and expanding understanding of non-blazar AGN emission.
Findings
Detected gamma-ray variability with >5sigma significance
Observed flux decrease over nine nights
Constructed multi-band spectral energy distribution
Abstract
The majority of the active galactic nuclei (AGN) detected at very-high-energies above 100 GeV belong to the class of blazars with a small angle between the jet-axis and the line-of-sight. Only about 10 percent of the gamma-ray AGN are objects with a larger viewing angle resulting in a smaller Doppler boosting of the emission. Originally, it was believed that gamma-ray emission can only be observed from blazars and those are variable in its brightness. Instead, the last years have shown that non-blazar active galaxies also show a fascinating variability behaviour which provide important new insights into the physical processes responsible for the gamma-ray production and especially for flaring events. Here, we report on the observation of gamma-ray variability of the active galaxy PKS 0625-354 detected with the H.E.S.S. telescopes in November 2018. The classification of PKS 0625-354 is a…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Dark Matter and Cosmic Phenomena
