Speaker
Michal Dyrda
(Institute of Nuclear Physics PAS)
Description
Most of the extragalactic objects detected so far in the very high energy (VHE) regime are blazars, but detected nearby radio galaxies: M87, Cen A and NGC 1275 of type FRI seem to constitute a new class of VHE emitters. The radio galaxy PKS 0625-354 was observed with the H.E.S.S. phase I telescopes in 2012, above the energy threshold of 250 GeV. The time-averaged TeV energy spectrum is well characterized by a power law model. The broad-band spectral energy distribution (SED), including the available multiwavelength data, as well as the VHE data gathered with H.E.S.S. will be presented.
| Registration number following "ICRC2015-I/" | 598 |
|---|---|
| Collaboration | H.E.S.S. |
Primary author
Michal Dyrda
(Institute of Nuclear Physics PAS)
Co-authors
Dr
Lukasz Stawarz
(Jagiellonian Univeristy)
Mr
Mateusz Janiak
(CAMK PAN)
Michal Ostrowski
(Jagiellonian University)
Mr
Olivier Hervet
(LUTH Obsevatory)
Rafal Moderski
(Nicolaus Copernicus Astronomical Center)
Dr
Wierzcholska Alicja
(Institute of Nuclear Physics PAS)
