Observations of very high energy gamma-ray galactic sources with H.E.S.S.

Due to changing environment with orbital phase (magnetic field strength, stellar photon field, relative position of compact object and star with respect to observer,. ), the VHE

We also compared the simple and model weight results to that obtained with the original Kerr ( 2011 ) method, which sim- ply corresponds to the model weight method with the

DISCOVERY OF VERY HIGH ENERGY GAMMA-RAY EMISSION FROM THE DISTANT BL LAC OBJECT H2356-309 WITH THE H.E.S.S.. Superina for the H.E.S.S

The interaction of the relativistic wind from a young pulsar with the stellar wind of the companion provides a common scenario to explain the emission from these sources.. They

To search for VHE γ-ray emission from each GC we per- formed two different kinds of analyses where the size of the emission region was assumed to be either a) point-like (0. ◦ 1

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

SUZAKU X-RAY FOLLOW-UP OBSERVATIONS OF SEVEN UNASSOCIATED FERMI-LAT GAMMA-RAY SOURCES AT HIGH GALACTIC LATITUDES..

exposure of individual observation periods (as represented on Fig. SN 2016adj was observed every night from day 3 till day 10 after the discovery date, and the average time