1 |
gvacanti |
1.1 |
om-badpix |
2 |
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========= |
3 |
calsci |
1.7 |
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4 |
atalaver |
1.9 |
Version 2.0 -2017-11-09 (AT) |
5 |
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+ Version 2.0 Issue 6 |
6 |
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+ Adding low sensitivity Depletion patch produced by accidental |
7 |
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Jupiter observation with V filter |
8 |
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9 |
calsci |
1.8 |
Version 1.2 -2009-06-05 (AT) |
10 |
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+ Version 1.2 Issue 5 |
11 |
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+ New bad pixel map based on inflight high resolution flat field |
12 |
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observations (revs. 400 - 1700) and images of extended sources |
13 |
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as M31 and some comets. |
14 |
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+ Issue 5 is resubmitted to restore coherence in the system. |
15 |
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Since V. 0.5 Changelog entries were not properly handled because |
16 |
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of a typo. |
17 |
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18 |
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Version 1.1 -2009-06-04 (AT) |
19 |
calsci |
1.7 |
+ Resubmission because of CVS problem. |
20 |
calsci |
1.8 |
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21 |
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Version 1.0 -2009-06-01 (AT) |
22 |
calsci |
1.7 |
+ version 1.0 Issue 5 |
23 |
calsci |
1.6 |
+ New bad pixel map based on inflight high resolution flat field |
24 |
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observations (revs. 400 - 1700) and images of extended sources |
25 |
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as M31 and some comets. |
26 |
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Old list of bad pixels (BADPIX_0004) is completetely replaced. |
27 |
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28 |
calsci |
1.8 |
Version 0.5 -2003-04-16 (CB) |
29 |
calsci |
1.7 |
+ version 0.5 Issue 5 ---> never uploaded: overwritten (AT 2009-06-01) |
30 |
bchen |
1.5 |
+ New bad pixel map based on inflight high resolution flat field |
31 |
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observations |
32 |
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33 |
bchen |
1.4 |
Version 0.4 - 2002-01-16 (CB) |
34 |
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+ Version 0.4 Issue 4 |
35 |
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+ The origin for OM badpixel coordinates is (1,1) and was incorrectly |
36 |
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designed in the previous version (version 3) as (0,0). This new |
37 |
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CCF corrects this bug. Others unchanged. |
38 |
bchen |
1.3 |
Version 0.3 - 2001-11-02 (CB) |
39 |
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----------- |
40 |
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41 |
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+ Version 0.3 Issue 3 |
42 |
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+ Include new bad pixels based on inflight flatfields between |
43 |
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Rev 130 and Rev 340. The sensitivity values are suitable |
44 |
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for a rough quality flag, not for correction. |
45 |
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46 |
rmuch |
1.2 |
Version 0.2 - 2000-06-16 (RM) |
47 |
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----------- |
48 |
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+ Version 0.2 Issue 2 |
49 |
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+ add the 6 m spots identified by Bob Shirey. |
50 |
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the values for the sensitivity reduction are preliminary. Flatfields |
51 |
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with a better statistics are needed to get a correct quantification. |
52 |
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53 |
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54 |
gvacanti |
1.1 |
Version 0.1 - 1999-09-17 (GV) |
55 |
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----------- |
56 |
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+ in CVS |
57 |
rmuch |
1.2 |
+ realistic numbers from Rudi based on CSL analysis: |
58 |
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first estimate of edge emission included |