Pregled bibliografske jedinice broj: 1006277
The Unprecedented VHE Gamma-ray Outburst of PKS 1510-089 in May 2016
The Unprecedented VHE Gamma-ray Outburst of PKS 1510-089 in May 2016 // Fifteenth Marcel Grossmann Meeting - MG15
Rim, Italija, 2018. (predavanje, međunarodna recenzija, neobjavljeni rad, znanstveni)
CROSBI ID: 1006277 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
The Unprecedented VHE Gamma-ray Outburst of PKS 1510-089 in May 2016
Autori
Terzić, Tomislav ; Zacharias, Michael ; Sitarek, Julian ; Dominis Prester, Dijana ; Jankowsky, Felix ; Lindfors, Elina ; Mohamed, Mahmoud ; Sanchez, David ; for the H.E.S.S. and MAGIC Collaborations
Kolaboracija
MAGIC Collaboration ; H.E.S.S. Collaboration
Vrsta, podvrsta i kategorija rada
Sažeci sa skupova, neobjavljeni rad, znanstveni
Skup
Fifteenth Marcel Grossmann Meeting - MG15
Mjesto i datum
Rim, Italija, 01.07.2018. - 07.07.2018
Vrsta sudjelovanja
Predavanje
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
Blazars, Relativistic jets, VHE gamma-rays, PKS1510-089
Sažetak
PKS 1510-089 (z=0.361), one of only a handful of flat spectrum radio quasars (FSRQ) detected in the very high energy (VHE, E > 100 GeV) gamma-rays, is known for its flux variability and complex multiwavelength behaviour. VHE observations by H.E.S.S. and MAGIC in May 2016 detected an unprecedented flare, both in intensity and in the shortness of its variability timescale. The flare lasted less than 48 hours, during which time the flux reached about 80 per cent of the Crab Nebula flux above 200 GeV. In addition, the intranight variability of this source was detected for the first time. Simultaneous observations in high energy (HE, E > 100 MeV) gamma-rays performed with Fermi-LAT and optical R-band performed with ATOM show behaviour not consistent with simple simultaneous brightening in all bands. While a significant hardening of the spectrum is visible in HE, the flux increased only moderately. A simultaneous rise in daily-averaged optical flux was seen in the R-band. However, the intranight flux evolution shows two prominent peaks, while only one is visible in the VHE range. These intriguing features of the flare will be presented in detail. We will also discuss possible explanations for the observed emission.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
HRZZ-IP-2016-06-9782 - Visokoenergijska astronomija gama-zraka teleskopima MAGIC i CTA (MAGIC-CTA) (Godinović, Nikola, HRZZ - 2016-06) ( CroRIS)
Ustanove:
Sveučilište u Rijeci - Odjel za fiziku