Abstract
The application of CCDs to X-ray imaging and spectroscopy for astronomy is described. The requirements which differ markedly from those of traditional optical applications are highlighted. Results of recent research programs to optimize CCD X-ray response are presented. It is shown that very high quantum efficiencies and Fano noise limited energy resolutions can be obtained. A number of issues related to the practical implementation of future instruments are reviewed.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 179-201 |
| Number of pages | 23 |
| Journal | Experimental Astronomy |
| Volume | 2 |
| Issue number | 3 |
| DOIs | |
| State | Published - May 1991 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science