Abstract
Astronomers are increasingly using thick (c. 100 micron) CCDs due to their superior red response (e.g. the PanSTARRS, DES, HSC, and LSST cameras). I introduce the signatures of diffusion and both permanent and induced electric fields on the data, and discuss the consequences for the PSF, astrometry, and photometry.
| Original language | English (US) |
|---|---|
| Article number | C04023 |
| Journal | Journal of Instrumentation |
| Volume | 9 |
| Issue number | 4 |
| DOIs | |
| State | Published - Apr 2014 |
All Science Journal Classification (ASJC) codes
- Mathematical Physics
- Instrumentation
Keywords
- Detectors for UV
- Image processing
- Photon detectors for UV
- visible and IR photons
- visible and IR photons (solid-state) (PIN diodes, APDs, Si-PMTs, G-APDs, CCDs, EBCCDs, EMCCDs etc)