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The VHE γ-Ray View of the FSRQ PKS 1510-089


(MAGIC Collaboration, H.E.S.S. Collaboration) Zacharias, Michael; Dominis Prester, Dijana; Jankowsky, Felix; Lindfors, Elina; Meyer, Manuel; Mohamed, Mahmoud; Prokoph, Heike; Sanchez, David; Sitarek, Julian; Terzic, Tomislav et al.
The VHE γ-Ray View of the FSRQ PKS 1510-089 // Galaxies, 7 (2019), 1; 41, 11 doi:10.3390/galaxies7010041 (međunarodna recenzija, članak, znanstveni)


Naslov
The VHE γ-Ray View of the FSRQ PKS 1510-089

Autori
Zacharias, Michael ; Dominis Prester, Dijana ; Jankowsky, Felix ; Lindfors, Elina ; Meyer, Manuel ; Mohamed, Mahmoud ; Prokoph, Heike ; Sanchez, David ; Sitarek, Julian ; Terzic, Tomislav ; Wagner, Stefan ; Wierzcholska, Alicja

Kolaboracija
MAGIC Collaboration, H.E.S.S. Collaboration

Izvornik
Galaxies (2075-4434) 7 (2019), 1; 41, 11

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

Ključne riječi
Active galactic nuclei ; blazar variability ; multi-wavelength ; correlation

Sažetak
The flat spectrum radio quasar PKS 1510-089 is a monitored target in many wavelength bands due to its high variability. It was detected as a very-high-energy (VHE) $\gamma$-ray emitter with H.E.S.S. in 2009, and has since been a regular target of VHE observations by the imaging Cherenkov observatories H.E.S.S. and MAGIC. In this paper, we summarize the current state of results focusing on the monitoring effort with H.E.S.S. and the discovery of a particularly strong VHE flare in 2016 with H.E.S.S. and MAGIC. While the source has now been established as a weak, but regular emitter at VHE, no correlation with other energy bands has been established. This is underlined by the 2016 VHE flare, where the detected optical and high-energy $\gamma$-ray counterparts evolve differently than the VHE flux.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Ustanove
Sveučilište u Rijeci - Odjel za fiziku

Časopis indeksira:


  • Web of Science Core Collection (WoSCC)
    • Emerging Sources Citation Index (ESCI)
  • Scopus


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