This version of the CCD42 family of CCD sensors has fullframe architecture. Back illumination technology, in combination with extremely low noise amplifiers, makes the device well suited to the most demanding applications requiring a high dynamic range.
| Space Agency | Mission | Instrument |
| ESA | Rosetta | Optical Spectrograph and InfraRed Imager System (OSIRIS) |
| JAXA / NASA | Solar-B/Hinode | X-Ray Telescope (EIT) |
| NASA / PSU | SWIFT | Ultraviolet/Optical Telescope (UVOT) |
| NASA | STEREO A | SECCHI |
| NASA | STEREO B | Extreme Ultraviolet Imager (EUVI) |
| Part Number | CCD42-40 |
|---|---|
| Sensor Type | CCD |
| Resolution | 2048 x 2048 |
| Pixel Size | 13.5 x 13.5 µm |
| Image Area | 27.6 x 27.6 mm |
| Output Amp | 2x VLN |
| Package | Compact Ceramic, 37.0 x 51.7 |
| Total Pixels | 4.19 MP |
| Wavelength Category |
X-Ray (0.01-10 nm) Ultraviolet (193-400 nm) |
| Document | Type |
|---|---|
| High TRL Space Imaging Detectors Catalogue |
| Document | Type |
|---|---|
| CCD42 40 (BI, AIMO) Datasheet | |
| CCD42 40 (BI, NIMO) Datasheet | |
| CCD42 40 (FI, AIMO) (Datasheet) | |
| CCD42 40 (FI, NIMO) (Datasheet) |
| Document | Type |
|---|---|
| 2014 CCD And CMOS Technology For Astronomical Sensors | |
| 2014 Presentation CCD And CMOS Technolody Developments For Astronomical Sensors |
