plt_stablity_ratio_ - BS04

REVISION DATE: 15-Dec-2017 21:17:39

This is looking at the spectal stability of the lamp data Mike is collecting in Hawaii over a number of days. I took the first day first data set and divided all the following data sets but this one data set (for each track)

The table shows the Ratio of the 5 net lights and there percent standard deviation for each day and track. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. The Ratio is calculated but dividing each of the days 5 net lights by the very fist net light on day 1 (not a mean of the day 1s 5 net lights)


Track Day CPIX 360
Mean / %std
CPIX 600
Mean / %std
CPIX 940
Mean / %std
1 1 1.00082 / 0.1197 1.00213 / 0.1261 1.00086 / 0.0709
1 2 1.00236 / 0.0894 1.00261 / 0.0695 1.00152 / 0.0619
1 3 1.00173 / 0.1314 1.00151 / 0.0785 1.00091 / 0.0466
1 4 1.00213 / 0.1674 1.00174 / 0.0591 1.00083 / 0.0408
1 5 1.00192 / 0.1085 1.00193 / 0.0826 1.00073 / 0.0305
2 1 1.00107 / 0.1772 1.00092 / 0.0729 1.00089 / 0.0617
2 2 1.00161 / 0.0819 1.00201 / 0.0730 1.00147 / 0.0487
2 3 1.00183 / 0.0676 1.00134 / 0.0626 1.00115 / 0.0468
2 4 1.00150 / 0.0956 1.00126 / 0.1065 1.00076 / 0.0576
2 5 1.00272 / 0.0996 1.00119 / 0.0914 1.00124 / 0.0784
3 1 0.99998 / 0.1655 1.00156 / 0.0883 1.00067 / 0.0673
3 2 1.00010 / 0.2001 1.00126 / 0.1207 1.00110 / 0.0505
3 3 1.00047 / 0.1128 1.00130 / 0.0526 1.00061 / 0.0481
3 4 1.00060 / 0.1117 1.00097 / 0.1156 1.00023 / 0.0616
3 5 1.00036 / 0.0513 1.00079 / 0.0520 1.00014 / 0.0387
4 1 1.00173 / 0.1749 1.00105 / 0.0849 1.00097 / 0.0655
4 2 1.00255 / 0.1449 1.00095 / 0.0966 1.00086 / 0.0486
4 3 1.00288 / 0.0549 1.00142 / 0.1041 1.00101 / 0.0379
4 4 1.00305 / 0.1494 1.00036 / 0.0590 1.00018 / 0.0326
4 5 1.00337 / 0.0834 1.00088 / 0.1079 1.00050 / 0.0385
5 1 1.00078 / 0.0516 1.00091 / 0.0552 1.00118 / 0.0672
5 2 1.00223 / 0.1743 1.00082 / 0.0773 1.00076 / 0.0263
5 3 1.00399 / 0.1474 1.00149 / 0.0873 1.00147 / 0.0247
5 4 1.00174 / 0.1044 1.00045 / 0.0656 1.00034 / 0.0449
5 5 1.00312 / 0.0968 1.00090 / 0.0545 1.00083 / 0.0731
6 1 1.00262 / 0.1776 1.00141 / 0.0883 1.00036 / 0.0283
6 2 1.00423 / 0.1845 1.00201 / 0.0985 1.00053 / 0.0372
6 3 1.00435 / 0.0824 1.00226 / 0.0624 1.00090 / 0.0167
6 4 1.00418 / 0.1007 1.00128 / 0.0243 1.00001 / 0.0349
6 5 1.00414 / 0.1080 1.00209 / 0.0906 1.00009 / 0.0143
7 1 1.00068 / 0.1655 1.00180 / 0.1106 1.00070 / 0.0630
7 2 1.00189 / 0.1623 1.00202 / 0.0772 1.00086 / 0.0868
7 3 1.00113 / 0.1215 1.00158 / 0.1094 0.99983 / 0.0526
7 4 1.00131 / 0.1779 1.00112 / 0.0825 0.99967 / 0.0901
7 5 1.00225 / 0.1434 1.00054 / 0.0954 0.99933 / 0.0751
8 1 1.00191 / 0.1437 1.00140 / 0.0944 1.00086 / 0.0894
8 2 1.00190 / 0.1641 1.00199 / 0.1148 1.00115 / 0.0761
8 3 1.00304 / 0.0779 1.00175 / 0.0715 1.00044 / 0.0307
8 4 1.00239 / 0.1116 1.00127 / 0.1112 1.00026 / 0.0536
8 5 1.00311 / 0.1287 1.00154 / 0.0754 1.00018 / 0.0531
9 1 1.00138 / 0.1228 1.00191 / 0.1304 1.00085 / 0.0575
9 2 1.00213 / 0.0754 1.00198 / 0.0903 1.00061 / 0.0373
9 3 1.00253 / 0.1632 1.00226 / 0.0698 1.00107 / 0.0482
9 4 1.00268 / 0.1950 1.00128 / 0.0398 1.00042 / 0.0481
9 5 1.00324 / 0.0851 1.00149 / 0.0414 1.00075 / 0.0745
10 1 1.00033 / 0.1019 1.00071 / 0.0532 1.00082 / 0.0607
10 2 1.00020 / 0.1450 1.00047 / 0.0686 1.00088 / 0.0461
10 3 1.00102 / 0.1313 1.00115 / 0.0844 1.00134 / 0.0516
10 4 1.00018 / 0.1336 1.00009 / 0.0974 1.00018 / 0.0454
10 5 1.00111 / 0.0904 1.00016 / 0.0602 1.00082 / 0.0578
11 1 1.00121 / 0.0819 1.00119 / 0.0832 1.00152 / 0.0980
11 2 1.00134 / 0.1311 1.00131 / 0.0762 1.00233 / 0.0341
11 3 1.00246 / 0.0727 1.00176 / 0.0365 1.00187 / 0.0440
11 4 1.00181 / 0.1500 1.00114 / 0.0511 1.00167 / 0.0604
11 5 1.00240 / 0.0961 1.00139 / 0.0458 1.00199 / 0.0330
12 1 1.00166 / 0.1326 1.00184 / 0.1138 1.00047 / 0.0442
12 2 1.00346 / 0.1541 1.00241 / 0.1431 1.00122 / 0.0636
12 3 1.00236 / 0.1400 1.00168 / 0.0992 1.00038 / 0.0492
12 4 1.00279 / 0.0911 1.00137 / 0.0766 1.00020 / 0.0408
12 5 1.00236 / 0.1214 1.00205 / 0.0486 1.00034 / 0.0458
13 1 1.00089 / 0.1010 1.00099 / 0.0780 1.00069 / 0.0552
13 2 1.00104 / 0.1395 1.00082 / 0.0756 1.00054 / 0.0338
13 3 1.00217 / 0.1198 1.00173 / 0.0559 1.00078 / 0.0428
13 4 1.00151 / 0.1697 1.00073 / 0.0812 1.00006 / 0.0532
13 5 1.00205 / 0.1132 1.00086 / 0.0822 1.00061 / 0.0209
14 1 1.00115 / 0.1547 1.00166 / 0.0950 1.00024 / 0.0430
14 2 1.00233 / 0.1370 1.00214 / 0.0772 1.00038 / 0.0616
14 3 1.00242 / 0.1308 1.00223 / 0.0686 1.00028 / 0.0386
14 4 1.00161 / 0.1520 1.00118 / 0.0442 0.99948 / 0.0425
14 5 1.00221 / 0.0805 1.00209 / 0.0563 1.00012 / 0.0473

Track 1: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 1

image

Track 2: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 2

image

Track 3: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 3

image

Track 4: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 4

image

Track 5: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 5

image

Track 6: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 6

image

Track 7: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 7

image

Track 8: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 8

image

Track 9: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 9

image

Track 10: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 10

image

Track 11: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 11

image

Track 12: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 12

image

Track 13: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 13

image

Track 14: showing each of the 5 net light scans ratio (to the day 1 net 1 light) for each days data. Nets are lite-dark divided by int time so units are ADU/pix/sec. The data are normalized to the ol455 monitor data by dividing the net signal by the ol455 data/2.391e-08. 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. The red line is the standard deviation of the 5 points from each day.

Figure 14

image

Figure 15

image

pwd: E:\zflora\mldata\mobyrefresh\characterizations\intial\MOBY-L267\bs4cal
Date: 15-Dec-2017 21:17:39
Created from plt_stablity_ratio_(1)