Abstract
COMPTEL, the imaging telescope on board CGRO, uses Compton scatter kinematics to reconstruct the direction of the incident photon. On the basis of the gammaray detection principle, it can also be used as a gamma-ray polarimeter. A series of Monte Carlo (M-C) simulations have been carried out using a simplified geometrical model of COMPTEL. The aim is to investigate COMPTEL’s response to polarized gamma-rays. including the dependence on incident photon energy and incident angle. M-C simulations show that COMPTEL can detect the polarization of Crab pulsar (if it is 100% polarized) at a marginal level and determine the polarization angle to within a few degrees.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
References
Schonfelder V. et al.: 1993. Ap.J Suppl., 86, p657–692.
Swinyard B.M. et al.: 1991. Proc. SPIE ,1548, 94.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1995 Springer Science+Business Media Dordrecht
About this paper
Cite this paper
Lei, F., Dean, A.J., Hills, G.L., Swinyard, B.M. (1995). Comptel as A Gamma-Ray Polarimeter. In: Bassani, L., Di Cocco, G. (eds) Imaging in High Energy Astronomy. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0407-4_44
Download citation
DOI: https://doi.org/10.1007/978-94-011-0407-4_44
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4182-9
Online ISBN: 978-94-011-0407-4
eBook Packages: Springer Book Archive