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Home > Astronomy > Detectors > EEV10a |
Operational Characteristics
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Noise (ADU) |
3.5 |
2.2 |
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All binning modes up to 4 x 2 have been tested in both speeds with no increase in noise.
Linearity
Vertical CTE | >0.999999 |
Horizontal CTE | >0.999999 |
Pixel Scale | 0.4 arcsecs/pixel on IDS235 0.19 arcsecs/pixel on ISIS Blue |
X Pixel size | 13.5 microns |
Y Pixel size | 13.5 microns |
X size in pixels of digitised area | 2148 |
Y size in pixels of digitised area | 4200 |
X size of useful imaging area | 2048 |
Y size of useful imaging area | 4100 |
X start of useful imaging area | 51 |
Y start of useful imaging area | 0 |
LN2 capacity of cryostat | 2.5 litres |
Cryostat window thickness | 4 mm |
Distance from window to CCD | 10 mm |
Cryostat window size | 36 x 66 mm |
Operating temperature | 153K |
Preferred amplifier | L( R provides the same performance ) |
Anti-blooming available | no |
Quantum Efficiency
Full QE curve for EEV4280 in tabulated form,
measured at ATC March 99
Dark current | 4 e/hour @ -120 degrees C |
Full well bloom limit | ~150000 electrons |
Chip flatness | Profile scan shows centre section to be flat to < 1 micron |
Cosmetics | There are about 2ish pixel/column defects plus a cluster of single pixel defects. See dark frame. |
Cosmic Ray count | ~2000 events/chip/hour |
Fringing. See below a graph of fringe amplitude vs wavelength for EEV10 and Red+2
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Fringing. Flat field showing fringing, EEV10 on the left Red+2 on the right. |
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