Abstract
The use of focusing telescopes in hard X-ray (E > 10 keV) astronomy will provide better flux sensitivity and imaging performances with respect to the direct-viewing detectors, utilized until now. We present recent results obtained from our group regarding the possible use of Bragg-diffraction technique to design hard X-ray focusing telescopes.
| Original language | English |
|---|---|
| Journal | Nuovo Cimento Della Societa Italiana Di Fisica C-geophysics and Space Physics |
| Volume | 20 |
| Issue number | 5 |
| Pages (from-to) | 843-849 |
| ISSN | 0390-5551 |
| Publication status | Published - 1997 |