The 6dF Fisch Camera Performance
Contents
4. SDSU2 Controller Performance
Tables
Table 3: Controller Performance
Table 4: VCTE and HCTE measurements at various counts
Table 5: Data sheet Quantum Efficiency values
Table 6: Relative QE measurements
This document contains a summary of the specifications and the testing of the 6dF Flair Spectrograph camera. This document is available online at http://www.mso.anu.edu.au/observing/. Follow the links: Computing and other resources, Detector Lab, CCD Detector Controllers and Instruments, CCD Systems, CCD102.
A list of images contained in the data pack is given in Chapter 9.
|
Serial Number |
8492-14-11 |
|
|
Engineering chip Description |
CCD47-10-1 Marconi 1024x1024 Thinned Back illum. Grade 1, astronomy BB coating, AIMO |
|
|
Science Chip Description |
CCD47-10-1 Marconi 1024x1024 Thinned Back illum. Grade 0, astronomy BB coating, AIMO |
|
|
Pixel Size(micron) |
13umx13um |
|
|
Chip size |
1056x1027 |
|
|
Preflash, e- |
None |
|
|
Readout Mode |
MPP |
NON-MPP |
|
Dark Current (e/px/s @ 20 Deg C) |
250 |
|
|
Full Well Capacity [e/px] |
90000 |
|
More detailed information can be viewed in the Manufacturer’s Data Sheet .
|
Dark Signal non-uniformity defects |
Bright columns |
0 |
|
Point Defects |
3 |
|
|
Photon Response non-uniformity defects |
Total columns |
0 |
|
Dark point defects |
31 |
|
|
Traps |
0 |
Left Amplifier
|
Characteristic |
Amplifier Left |
||
|
Readout Speed |
slow |
medium |
fast |
|
Noise (e-/RMS) |
2.7 |
2.75 |
3.9 |
|
Gain (e-/ADU) |
0.33 |
0.64 |
1.3 |
|
Full Frame READOUT TIME [secs] |
42 |
24 |
11 |
|
Linearity 0.5% [ke] |
|
42 |
|
|
Saturation [ke] |
|
42 |
|
|
Control Temperature [K] |
170.0 |
||
|
Dark Current [e/px/hr] at 170K |
0.79 |
||
Table 3: Controller Performance
The measured charge transfer efficiency values are shown in the table below.
|
No of counts |
HCTE % |
VCTE % |
Images |
|
|
|
|
|
|
1000 |
100.0002 |
99.99994 |
cte1thou0001red |
|
10000 |
99.99979 |
99.99998 |
cte10thou0001red |
|
50000 |
99.99981 |
99.99996 |
cte50thou0001red |
Table 4: VCTE and HCTE measurements at various counts
|
Wavelength |
Quantum Efficiency |
|
350nm |
39.5% |
|
400nm |
74.9% |
|
500nm |
80.1% |
|
650nm |
75.4% |
|
900nm |
33.2% |
Table 5: Data sheet Quantum Efficiency values
The following measurements show that the QE doesn’t vary over 150-184 K at 690nm.
|
Temp (K) |
Wavelength Nm |
Average Signal ADU |
Date taken |
Image names |
|
|
|
|
|
|
|
170 |
690 |
8860 |
22/11 |
qe0001_170K, qe0002_170K |
|
178.8 |
690 |
8875 |
22/11 |
qe0001_180K, qe0002_180K |
|
184 |
690 |
8870 |
22/11 |
qe0001_184K, qe0002_184K |
|
170 |
690 |
8850 |
22/11 |
qe0003_170K, qe0004_170K |
|
150 |
690 |
8740 |
23/11 |
qe0001_150K, qe0002_150K |
|
160 |
690 |
8770 |
23/11 |
qe_0001_160K,qe0002_160k |
|
170 |
690 |
8770 |
23/11 |
qe0005_170K, qe0006_170K |
Table 6: Relative QE measurements
The average signal is stable enough (on a given day) to conclude that the QE has no significant temperature dependence at 690nm over the above range. This is bearing in mind that the shot noise of the signals is the square root of the average signal, ~95 ADU’s.
The non- linearity was determined to < 0.1%. Plots are presented below for linearity, non-linearity, and variance versus mean signal at low and high levels.
The images were analyzed to obtain mean signal level and variance. The plots show that the non linearity is < 0.1%. The definition used for non-linearity is:

Where the mean is the unbiased signal level.

Figure 1: Linearity - low level

Figure 2: Linearity – high level

Figure 3: Non-linearity - low-level

Figure 4: Non-linearity - high level

Figure 5: Variance vs Mean signal - low level

Figure 6: Variance vs Mean signal - high level
The following documents contain the detailed testing procedures and results.
The following table lists the images in the delivered dataset. They are a subset of the images used for the analysis shown in this document (and the linked documents).
|
Directory |
Image |
Type |
Comment |
|
noiseexps |
noise0001.fits |
Bias |
These four exposures were used to measure noise and gain at medium readout speed. |
|
noise0002.fits |
Bias |
||
|
noise0003.fits |
Flat |
||
|
noise0004.fits |
Flat |
||
|
|
|
|
|
|
noise0005.fits |
Bias |
These four exposures were used to measure noise and gain at fast readout speed. |
|
|
noise0006.fits |
Bias |
||
|
noise0007.fits |
Flat |
||
|
noise0008.fits |
Flat |
||
|
|
|
|
|
|
darkexps |
bias0005-0010 |
Bias |
Bias taken prior to the following darks for dark current tests, and bias stability tests. |
|
dark0007-0011 |
Dark, 2 hour exposure |
|
|
|
bias0011-0015 |
Bias |
Bias taken after to the above darks for dark current tests, and bias stability tests. |
|
|
|
|
|
|
|
darkcurrent0007 |
text |
Results file from dark current algorithm |
|
|
darkcurrent0007.fits |
Dark current |
dark0007 with overscan and bias subtraction |
|
|
darkcurrent0008 |
text |
Results file from dark current algorithm |
|
|
darkcurrent0008.fits |
|
dark0008 with overscan and bias subtraction |
|
|
|
|
|
|
|
coude |
focus0004.fits |
|
|
|
focus0006.fits |
|
|
|
|
focus0007.fits |
|
|
|
|
|
|
|
|
|
spectra0052.fits |
|
|
|
|
spectra0053.fits |
|
|
|
|
spectra0055.fits |
|
|
|
|
|
|
|
|
|
cteexps |
cte1thou0001red |
Flat, 1000 counts |
|
|
cte10thou0001red |
Flat, 10 000 counts |
|
|
|
cte50thou0001red |
Flat 50 000 counts |
|
|
|
|
|
|
|
|
quanteffexps |
qe0001_170K, |
|
|
|
qe0002_170K |
|
|
|
|
qe0001_180K |
|
|
|
|
qe0002_180K |
|
|
|
|
qe0001_184K |
|
|
|
|
qe0002_184K |
|
|
|
|
qe0003_170K |
|
|
|
|
qe0004_170K |
|
|
|
|
qe0001_150K |
|
|
|
|
qe0002_150K |
|
|
|
|
qe_0001_160K |
|
|
|
|
qe0002_160k |
|
|
|
|
qe0005_170K |
|
|
|
|
qe0006_170K |
|
|
|
|
|
|
|
|
|
linearityexps |
linlow0001 |
0 |
The flats taken and their corresponding exposure time in seconds for low-level linearity measurements. |
|
linlow0002 |
0 |
||
|
linlow0003 |
.100 |
||
|
linlow0004 |
.100 |
||
|
linlow0005 |
.500 |
||
|
linlow0006 |
.500 |
||
|
linlow0007 |
.200 |
||
|
linlow0008 |
.200 |
||
|
linlow0009 |
.500 |
||
|
linlow0010 |
.500 |
||
|
linlow0011 |
.300 |
||
|
linlow0012 |
.300 |
||
|
linlow0013 |
.500 |
||
|
linlow0014 |
.500 |
||
|
linlow0015 |
.400 |
||
|
linlow0016 |
.400 |
||
|
linlow0017 |
.500 |
||
|
linlow0018 |
.500 |
||
|
|
|
|
|
|
linhigh0001 |
0 |
The flats taken and their corresponding exposure time in seconds for high-level linearity measurements. |
|
|
linhigh0002 |
0 |
||
|
linhigh0003 |
1 |
||
|
linhigh0004 |
1 |
||
|
linhigh0005 |
10 |
||
|
linhigh0006 |
10 |
||
|
linhigh0007 |
7 |
||
|
linhigh0008 |
7 |
||
|
linhigh0009 |
10 |
||
|
linhigh0010 |
10 |
||
|
linhigh0011 |
13 |
||
|
linhigh0012 |
13 |
||
|
linhigh0013 |
10 |
||
|
linhigh0014 |
10 |
||
|
linhigh0015 |
19 |
||
|
linhigh0016 |
19 |
||
|
linhigh0017 |
10 |
||
|
linhigh0018 |
10 |
||
|
linhigh0019 |
25 |
||
|
linhigh0020 |
25 |
||
|
linhigh0021 |
10 |
||
|
linhigh0022 |
10 |
||
|
linhigh0023 |
31 |
||
|
linhigh0024 |
31 |
||
|
linhigh0025 |
10 |
||
|
linhigh0026 |
10 |
||
|
linhigh0027 |
37 |
||
|
linhigh0028 |
37 |
||
|
linhigh0029 |
10 |
||
|
linhigh0030 |
10 |
||
|
linhigh0031 |
43 |
||
|
linhigh0032 |
43 |
||
|
linhigh0033 |
10 |
||
|
linhigh0034 |
10 |
||
|
linhigh0035 |
49 |
||
|
linhigh0036 |
49 |
||
|
linhigh0037 |
10 |
||
|
linhigh0038 |
10 |
||
|
linhigh0039 |
55 |
||
|
linhigh0040 |
55 |
||
|
linhigh0041 |
10 |
||
|
linhigh0042 |
10 |
||
|
linhigh0043 |
61 |
||
|
linhigh0044 |
61 |
||
|
linhigh0045 |
10 |
||
|
linhigh0046 |
10 |