Pregled bibliografske jedinice broj: 1018222
The VHE γ-Ray View of the FSRQ PKS 1510-089
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)
CROSBI ID: 1018222 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
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 ; Terzić, 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
Citiraj ovu publikaciju:
Časopis indeksira:
- Web of Science Core Collection (WoSCC)
- Emerging Sources Citation Index (ESCI)
- Scopus