10 November 1998 Bragg telescopes in lobster-eye configuration
Author Affiliations +
In this paper will be investigated the possibility to exploit the Bragg diffraction from mosaic crystals as a reflection technique for the realization of lobster-eye telescopes for hard x-rays. In particular for our study we will assume the particular lobster-eye configuration also known as Schmidt imager. This geometry is particularly interesting not only why it can allow a 1D focusing over large fields of view but also because it is relatively easy to be realized, being based on flat reflectors. Until now lobster-eye telescopes have been mostly studied for applications in the classical x-ray band, making use of total external reflection at grazing angles mirrors. However, due to the much larger reflection angles typical of Bragg diffraction it is possible to extend the use of the Schmidt geometry also to the hard x-ray energy band. Here, in addition to a general description of the behavior of Schmidt telescopes based on the Bragg diffraction technique, we will report also some theoretical evaluations about the performances achievable with these devices.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Giovanni Pareschi, Filippo Frontera, G. Pasqualini, and Andrea Stevoli "Bragg telescopes in lobster-eye configuration", Proc. SPIE 3445, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, (10 November 1998); doi: 10.1117/12.330278; https://doi.org/10.1117/12.330278


The current status of ASTRO-H/HXT development facility
Proceedings of SPIE (August 31 2009)
Instrumentation of the hard x-ray telescope mission
Proceedings of SPIE (October 17 1996)
Hard x-ray telescope mission
Proceedings of SPIE (October 11 1996)

Back to Top