Paper
18 October 1996 Use of Compton kinematics on the IBIS telescope
Guido Di Cocco, Giuseppe Malaguti, Ezio Caroli, Gianclaudio Ferro, D. Grassi, Claudio Labanti, A. Mauri, Elio Rossi, Filomena Schiavone, Aldo Spizzichino, Alessandro Traci
Author Affiliations +
Abstract
The multi-layer discrete structure of the IBIS telescope onboard the INTEGRAL gamma-ray satellite allows the application of the Compton kinematics for improving the signal to noise ratio of the images which are obtained by mens of a coded mask coupled to a position sensitive detector. Two steps of data selection based on Compton kinematics are envisaged: one to be operated aboard the satellite and the other one which will be applied on ground. The possible reduction of data volume to be transmitted to ground, background rejection, and signal to noise enhancement are shown.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Guido Di Cocco, Giuseppe Malaguti, Ezio Caroli, Gianclaudio Ferro, D. Grassi, Claudio Labanti, A. Mauri, Elio Rossi, Filomena Schiavone, Aldo Spizzichino, and Alessandro Traci "Use of Compton kinematics on the IBIS telescope", Proc. SPIE 2806, Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions, (18 October 1996); https://doi.org/10.1117/12.253987
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Compton scattering

Kinematics

Sensors

Scattering

Signal to noise ratio

Gamma radiation

RELATED CONTENT

The HERMES-TP/SP background and response simulations
Proceedings of SPIE (December 13 2020)
The GLAST burst monitor
Proceedings of SPIE (October 11 2004)
The DUAL mission concept
Proceedings of SPIE (September 13 2011)

Back to Top