Abstract
We present a comparison of the spectroscopic capabilities of a front side-illuminated thin-gate CCD and the AXAF CCD Imaging Spectrometer back side-illuminated CCD for two simulated astrophysical observations below 1 keV. The thin-gate CCD has superior energy resolution but inferior (although nonnegligible) quantum efficiency over this bandpass. We show that the low-noise, thin-gate CCD design provides superior determination of confidence intervals for spectroscopy below 1 keV.
| Original language | English (US) |
|---|---|
| Pages (from-to) | L51-L54 |
| Journal | Astrophysical Journal |
| Volume | 466 |
| Issue number | 1 PART II |
| DOIs | |
| State | Published - 1996 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
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