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NOT CCD #7 test report.

Data collected 2000 01 20.

Test circumstances.

LocationIn ALFOSC, on telescope.
Light sourceBlue light in filter wheel.

Summary of Results

Bias level370ADU
Bias std. dev.5.285ADU
Conversion factor1.056electrons/ADU
Readout Noise5.58electrons/pixel
Nonlinearity<0.5%
Shutter error-0.01sec

Data

Window used: (896:1152,896:1152) (pixel, of full field, unbinned).

Exposure time (s)Mean Counts 1 (ADU)Mean Counts 2 (ADU)(Photon Noise)2 (ADU2)
2.000002204.002208.492213.0
2.000002238.522238.512213.7
4.000004378.554385.994309.8
8.000008820.978820.578612.3
12.000013090.413107.912573.
16.000017601.517601.917258.
20.000021848.321870.121040.
24.000026386.126387.225059.
28.000030638.330662.929388.
32.000035174.235177.733622.
36.000039449.239471.537776.
40.000043961.343968.642051.
44.000048273.048294.545960.
48.000052750.752764.850019.
52.000057105.257125.154074.
This table as ASCII

Plots

Linearity GIF PostScript
Linearity as count rate GIF PostScript
Photon transfer curve GIF PostScript
BitStat GIF PostScript

Images

A median stacked image of 21 bias frames is available here (2.2 MByte, gzipped).

A median stacked image of 20 short exposures (0.1 sec each) is available here (4.0 MByte, gzipped). This image may be useful for exploring the blemish structure of CCD#7. There are several traps and a couple of bad columns. The many spots with reduced sensitivity are artefacts of the thinning/coating process.

Back to top Last modified: May 31 2023