Wierzcholska A, Glawion D (2022)
Publication Type: Journal article
Publication year: 2022
Book Volume: 15
Article Number: 3-A10
Journal Issue: 3
DOI: 10.5506/APhysPolBSupp.15.3-A10
The catalogue of TeV gamma-ray emitting objects includes about 90 extragalactic sources, among which only a few belong to the class of radio galaxies or misaligned blazars. This smaller class includes PKS 0625-354, a source detected as a TeV gamma-ray emitter already in 2012. Here, we report on H.E.S.S. observations of this active galaxy performed in November 2018. The classification of the object is still a matter of debate in the context of blazar and radio-galaxy scenarios. With the recent H.E.S.S. observations, supported with multi-wavelength observations collected with Fermi-LAT, Swift-XRT, and Swift-UVOT, we report on the detection of TeV gamma-ray variability of the sources. Ten days of H.E.S.S. observations revealed an outburst observed on November 1 followed by a decrease in the gamma-ray flux. We report on the result of H.E.S.S. and multiwavelength observations of PKS 0625-354. We also discuss the possible interpretation of the broadband spectral energy distribution of the source and the implication of the TeV gamma-ray variability detected.
APA:
Wierzcholska, A., & Glawion, D. (2022). IT’S A BLAZAR. . . IT’S A RADIO GALAXY. . . IT’S PKS 0625-354! Acta Physica Polonica B, Proceedings Supplement, 15(3). https://doi.org/10.5506/APhysPolBSupp.15.3-A10
MLA:
Wierzcholska, Alicja, and Dorit Glawion. "IT’S A BLAZAR. . . IT’S A RADIO GALAXY. . . IT’S PKS 0625-354!" Acta Physica Polonica B, Proceedings Supplement 15.3 (2022).
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