Compton telescope with coded aperture mask: Imaging with the INTEGRAL/IBIS Compton mode

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

The angular error distribution is shown in figure 6 for (a) 511 keV and (b) 1275 keV estimated incident energy and for (c) all the coincidences showing a good agreement

Soulignons deux points : (1) les modèles théoriques d’émission prédisent une large émission γ en éventail et un fin faisceau radio, cette méthode favorise donc les pulsars avec

The source position should ideally be reconstructed from events (called true events thereafter) corresponding to one Compton scattering in each scatter detector without energy

The electric and magnetic polarizabilities αE and βM of Real Compton Scat- tering (RCS) 1 are a measure of the deformation of the nucleon structure under an applied EM field..

Virtual Compton Scattering has opened a new field of investigation of nucleon structure.. At low center-of-mass energies, the process γ ∗ p → γp allows the de- termination of

Abstract—We report the study of direct measurement of ion- ization charges in an innovative liquid xenon Compton camera of small animal imaging, named XEMIS2.. It was combined with

In the case where the Earth lies within the GRB emission cone (i.e. the direct light of the GRB could have been seen in the past), the Compton trail appears as a ring of