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NOT CCD #4 test report.

Data collected 99 08 21.

Test circumstances.

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

Summary of Results

Bias level406ADU
Bias std. dev.5.50ADU
Conversion factor1.180electrons/ADU
Readout Noise6.50electrons/pixel
Nonlinearity<0.2%
Shutter error~ 0.0sec

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)
1.000003718.843720.503267.80
2.000007395.337400.516461.94
3.0000011167.311166.39914.24
4.0000014823.114832.412997.1
5.0000018631.118631.316254.4
6.0000022278.622290.919494.8
7.0000026107.026108.622588.3
8.0000029760.129772.125850.2
9.0000033592.833592.328858.2
10.000037255.637268.132382.9
11.000041086.141090.235323.9
12.000044763.244776.638520.5
13.000048589.548591.741769.0
14.000052275.152288.044767.7
15.000056078.956083.347525.4
16.000059778.359790.150815.1
17.000063543.663547.249409.5
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 12 bias frames is available here (2.3 MByte, gzipped).

A median stacked image of 19 short exposures (0.1 sec each) is available here (4.1 MByte, gzipped). This image may be useful for exploring the blemish structure of CCD#4. The many spots and regions with reduced sensitivity are artefacts of the thinning/coating process. There is a great deal of structure in this CCD's flat field and it is possible that it was not properly oxygen soaked on the occasion of this test.

Back to top Last modified: May 31 2023