H.E.S.S and Fermi-LAT discovery of gamma rays from the blazar 1ES 1312-423
Langue
en
Article de revue
Ce document a été publié dans
Monthly Notices of the Royal Astronomical Society. 2013-09-21, vol. 434, p. 1889-1901
Oxford University Press (OUP): Policy P - Oxford Open Option A
Résumé en anglais
A deep observation campaign carried out by the High Energy Stereoscopic System (H.E.S.S.) on Centaurus A enabled the discovery of gamma rays from the blazar 1ES 1312-423, two degrees away from the radio galaxy. With a ...Lire la suite >
A deep observation campaign carried out by the High Energy Stereoscopic System (H.E.S.S.) on Centaurus A enabled the discovery of gamma rays from the blazar 1ES 1312-423, two degrees away from the radio galaxy. With a differential flux at 1 TeV of (1.9 +/-0.6(stat) +/-0.4(sys)) x 10^{-13} /cm^2 /s /TeV corresponding to 0.5% of the Crab nebula differential flux and a spectral index of 2.9 +/- 0.5 (stat) +/- 0.2 (sys), 1ES 1312-423 is one of the faintest sources ever detected in the very high energy (E>100 GeV) extragalactic sky. A careful analysis using three and a half years of Fermi-LAT data allows the discovery at high energies (E>100 MeV) of a hard spectrum (index of 1.4 +/- 0.4 (stat) +/- 0.2 (sys)) source coincident with 1ES 1312-423. Radio, optical, UV and X-ray observations complete the spectral energy distribution of this blazar, now covering 16 decades in energy. The emission is successfully fitted with a synchrotron self Compton model for the non-thermal component, combined with a black-body spectrum for the optical emission from the host galaxy.< Réduire
Mots clés en anglais
BL Lacertae objects: individual: 1ES 1312-423
galaxies: jets
gamma-rays: galaxies
radiation mechanisms: non-thermal
galaxies: active
Origine
Importé de halUnités de recherche