REVISION DATE: 05-Dec-2017 22:56:43
This is looking at the background stability of the lamp data Mike is collecting in Hawaii over a number of days.
The table shows the mean of 24 backgrounds scans minus the 10 darks scans for each day and track. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data.
| Track | Day | CPIX 360 Mean |
CPIX 600 Mean |
CPIX 940 Mean |
|---|---|---|---|---|
| 1 | 1 | -0.0978 | -0.6769 | 0.4538 |
| 1 | 2 | 0.4990 | -0.0083 | -0.3904 |
| 1 | 3 | 0.7250 | 0.8606 | 0.8471 |
| 1 | 4 | -0.7487 | -0.5391 | -0.4321 |
| 1 | 5 | 0.2494 | 0.6689 | 0.6500 |
| 2 | 1 | 0.4940 | 0.1627 | -1.1147 |
| 2 | 2 | 0.3600 | -0.0720 | -1.0313 |
| 2 | 3 | 0.5347 | 0.3370 | 0.5350 |
| 2 | 4 | -0.1513 | -1.2927 | -0.6527 |
| 2 | 5 | 0.4817 | 0.1083 | 0.0963 |
| 3 | 1 | 0.4787 | 0.0500 | -0.1868 |
| 3 | 2 | 0.4189 | 1.1919 | -0.5767 |
| 3 | 3 | 0.6301 | 0.7483 | 0.5277 |
| 3 | 4 | -0.2760 | -1.0449 | -1.3797 |
| 3 | 5 | 0.2267 | -0.0139 | 0.5639 |
| 4 | 1 | 0.5208 | -0.3608 | 0.5247 |
| 4 | 2 | 0.3274 | -0.0764 | -0.9257 |
| 4 | 3 | 0.7698 | 0.1819 | 0.2851 |
| 4 | 4 | -0.1233 | 0.2281 | -0.8878 |
| 4 | 5 | 0.6517 | 0.1271 | 0.0337 |
| 5 | 1 | -0.1808 | -0.2449 | 0.1185 |
| 5 | 2 | -0.1842 | -0.4870 | -0.0709 |
| 5 | 3 | -0.0356 | 0.7884 | -0.1579 |
| 5 | 4 | -0.0387 | -0.3658 | -1.6452 |
| 5 | 5 | -0.2551 | -0.0147 | -0.1510 |
| 6 | 1 | -1.2060 | -0.3937 | -0.6190 |
| 6 | 2 | -0.3433 | -0.3504 | -0.7461 |
| 6 | 3 | -0.2518 | -0.0912 | 0.3979 |
| 6 | 4 | -1.0173 | -0.8113 | -1.4387 |
| 6 | 5 | 0.6644 | -0.1743 | 0.3454 |
| 7 | 1 | 0.2312 | 0.1171 | -0.1298 |
| 7 | 2 | -0.6733 | -0.8661 | -0.4952 |
| 7 | 3 | -0.4363 | 0.0486 | 0.3192 |
| 7 | 4 | -0.9634 | -1.0003 | -1.0425 |
| 7 | 5 | -0.8110 | 0.1000 | -0.5445 |
| 8 | 1 | -0.6412 | -0.4602 | -1.1271 |
| 8 | 2 | -0.4042 | 0.3680 | -1.0937 |
| 8 | 3 | 0.3180 | 1.2616 | 0.2553 |
| 8 | 4 | -0.8176 | -0.2845 | -1.3940 |
| 8 | 5 | -0.1528 | -0.1063 | -1.0011 |
| 9 | 1 | -0.7583 | -0.8920 | -1.2764 |
| 9 | 2 | -0.0240 | -0.9080 | -1.0049 |
| 9 | 3 | 0.1649 | 1.0108 | 0.3861 |
| 9 | 4 | -0.8694 | -1.3288 | -1.2917 |
| 9 | 5 | 0.2000 | 0.3285 | 0.2316 |
| 10 | 1 | 0.1344 | -0.3104 | -0.7465 |
| 10 | 2 | -0.2535 | -1.1437 | -1.0844 |
| 10 | 3 | 0.5844 | 0.2319 | 0.1274 |
| 10 | 4 | -0.4573 | -0.6965 | -1.3264 |
| 10 | 5 | 0.8250 | 0.8628 | -0.2760 |
| 11 | 1 | -0.0740 | 0.5313 | 0.1955 |
| 11 | 2 | -0.3469 | -1.1059 | -0.9937 |
| 11 | 3 | 0.5215 | 0.6764 | 0.5187 |
| 11 | 4 | -1.7073 | -1.6153 | -0.7191 |
| 11 | 5 | -0.1736 | 0.3566 | -0.3639 |
| 12 | 1 | 0.1959 | 0.0113 | -0.4582 |
| 12 | 2 | -0.0860 | 0.1856 | -0.7353 |
| 12 | 3 | 0.1623 | 0.2384 | -0.6099 |
| 12 | 4 | -1.1812 | -1.2243 | -1.1640 |
| 12 | 5 | 0.2462 | 0.3575 | -0.3877 |
| 13 | 1 | -0.3456 | -0.4486 | -0.5020 |
| 13 | 2 | -0.5483 | 0.0530 | -0.7402 |
| 13 | 3 | 0.5351 | 0.3392 | 0.3666 |
| 13 | 4 | -0.6578 | -0.9953 | -0.8885 |
| 13 | 5 | -0.1628 | -0.5470 | -0.6959 |
| 14 | 1 | -0.7854 | 0.1448 | -0.3042 |
| 14 | 2 | -0.7142 | -0.7694 | -0.3375 |
| 14 | 3 | -0.5224 | 0.1389 | 0.3424 |
| 14 | 4 | -0.5760 | -0.5247 | -1.1229 |
| 14 | 5 | -0.1941 | -0.2437 | 0.2406 |
Track 1: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 1
Track 2: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 2
Track 3: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 3
Track 4: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 4
Track 5: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 5
Track 6: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 6
Track 7: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 7
Track 8: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 8
Track 9: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 9
Track 10: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 10
Track 11: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 11
Track 12: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 12
Track 13: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 13
Track 14: showing each of the 24 backgrounds scans minus the 10 darks scans for each days data. The Backgrounds and Darks have units of ADU/pix and so are not divided by integration time. The data are NOT normalized to the ol455 monitor data. The black dashed lines show the pixel locations of the data on the graphs to the right. The right 3 stacked panels shows a single pixel for each dark/day combo.
Figure 14
