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MIPS IOC Task Summary |
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Duration |
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IOC |
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IOC-MIPS_ |
Name |
T (K) |
(hrs) - Est |
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Critical |
Notes |
SI Science Requirements |
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1 |
005a |
Electronics live tests |
Any |
1.00 |
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Y |
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10120C |
2 |
010a |
Detector aliveness check |
Any |
1.00 |
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Y |
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10170C |
3 |
015a |
CE state validation |
Any |
1.00 |
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Y |
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10510C, 10130C, 10500C |
4 |
020a |
Command and data paths |
Any |
1.00 |
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Y |
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10130C |
5 |
025a |
Scan mirror operational test |
Any |
0.02 |
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Y |
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10260C |
6 |
030a |
Heaters, temp sensors |
Any |
0.08 |
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Y |
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10210C |
7 |
035a |
CE EEPROM test |
Any |
0.25 |
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Y |
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10030C |
8 |
040a |
Engineering and data acquistion |
Any |
0.08 |
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Y |
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10150C |
9 |
050a |
Scattered backgrd monitor #1 |
90 |
1.00 |
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Y |
Must be near this temp |
10630C |
10 |
055a |
Scattered backgrd monitor #2 |
60 |
1.00 |
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Y |
Must be near this temp |
10630C |
11 |
100a |
First light 24 um |
45 |
0.11 |
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Y |
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10290C |
12 |
105a |
On-board S/W: Command expansion and data manipulation |
45 |
0.25 |
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Y |
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10140C |
13 |
110a |
Confirmation of on-board data processing algorithms |
45 |
1.00 |
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Y |
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10160C |
14 |
120a |
Calibration of Stims against celestial standards 24 um |
43 |
0.50 |
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Y |
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10190C, 10590C |
15 |
150a |
Determination of radiometric throughput 24 um |
38 |
1.00 |
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Y |
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10560C, 10700C |
16 |
115a |
Detector response to Stims -- 24 um |
35 |
0.33 |
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Y |
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10180C |
17 |
155a |
Latent images and saturation behavior 24 um |
31 |
0.33 |
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Y |
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10530C |
18 |
060a |
Scattered backgrd monitor #3 |
30 |
1.00 |
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Y |
Must be near this temp |
10630C |
19 |
065a |
Scattered backgrd monitor #4 |
23 |
1.00 |
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Y |
Must be near this temp |
10630C |
20 |
101a |
First light 70 um |
17 |
0.11 |
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Y |
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10290C |
21 |
130a |
24 um and 70 um array geometries and scan mirror vectors |
16 |
1.50 |
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Y |
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10450C, 10460C |
22 |
070a |
Scattered backgrd monitor #5 |
12 |
1.00 |
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Y |
Must be near this temp |
10630C |
23 |
135a |
SED of CSE |
12 |
0.33 |
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Y |
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10750C |
24 |
140a |
SED slit profile |
12 |
0.67 |
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N |
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new |
25 |
145a |
SED wavelength cal |
12 |
0.25 |
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N |
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new |
26 |
300a |
SED AOT validation |
12 |
1.50 |
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Y |
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10750C, 10830C, 10840C, 10850C, 10860C, 10870C, 10770C |
27 |
102a |
First light 160 um |
8.5 |
0.11 |
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Y |
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10290C |
28 |
045a |
Bias level commanding |
8.5 |
--- |
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Y |
Done with sensitivity |
10200C |
29 |
160a |
Ge:Ga anneal frequency |
8.5 |
3.30 |
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Y |
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10490C, 10220C |
30 |
225a |
Instrument stability |
8.5 |
3.30 |
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Y |
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10510C, 10550C |
31 |
230a |
Effect of bias and integration times on sensitivity |
8.5 |
1.42 |
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Y |
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10470C |
32 |
355a |
Cluster option validation |
8.5 |
0.75 |
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Y |
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10740C |
33 |
350a |
Calib of Stims against celestial standards 70 & 160 um |
7.4 |
1.50 |
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Y |
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10190C, 10590C |
34 |
235a |
160 um array geometry |
7 |
0.17 |
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Y |
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10450C |
35 |
270a |
Total power at Ecliptic Pole |
7 |
0.67 |
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Y |
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10750C |
36 |
275a |
Photometry of a CSE |
7 |
0.75 |
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N |
ERO |
10870C, 10760C |
37 |
280a |
Super Res of SVS-13 |
7 |
1.00 |
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N |
ERO |
10870C, 10760C, 10700C, 10530C |
38 |
285a |
Scan map of a PN or SNR |
7 |
2.50 |
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N |
ERO |
10870C, 10760C |
39 |
290a |
Scan map of HH 7-11 region |
7 |
3.00 |
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N |
ERO |
10870C, 10760C, 10770C, 10530C |
40 |
295a |
Scan map of M31 or M33 |
7 |
8.50 |
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N |
ERO |
10870C, 10760C, 10770C |
41 |
315a |
Behavior as a function of sky background |
7 |
3.00 |
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Y |
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10540C |
42 |
210a |
Latent images and saturation behavior 70 & 160 um |
6.5 |
0.67 |
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Y |
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10530C |
43 |
345a |
Opt temp for 24 um array |
6.5 |
1.50 |
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Y |
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10470C |
44 |
220a |
Slew state validation |
6 |
0.50 |
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Y |
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10130C |
45 |
247a |
Detector response to Stims -- 70 and 160 um |
6 |
0.67 |
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Y |
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10180C |
46 |
250a |
Cosmic ray limits on integration times |
6 |
0.37 |
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N |
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10240C, 10230C |
47 |
320a |
Phot/SR AOT validation |
6 |
2.00 |
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Y |
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10740C, 10830C, 10840C, 10850C, 10860C |
48 |
325a |
Scan AOT validation |
6 |
9.50 |
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Y |
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10740C, 10830C, 10840C, 10850C, 10860C |
49 |
330a |
Total power AOT validation |
6 |
0.70 |
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Y |
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10750C, 10830C, 10840C, 10850C, 10860C, 10870C, 10770C |
50 |
125a |
Transfer function test |
5.5 |
3.00 |
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Y |
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10150C |
51 |
205a |
Determination of radiometric throughput 70 & 160 um |
5.5 |
2.00 |
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Y |
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10560C, 10700C |
52 |
240a |
Spectral leak checks |
5.5 |
1.13 |
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N |
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10690C |
53 |
245a |
Optimum bias setting |
5.5 |
3.00 |
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Y |
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10470C |
54 |
255a |
Radiometry tests |
5.5 |
12.00 |
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Y |
6 x 2 hour sessions |
10520C, 10600C, 10700C |
55 |
260a |
Read noise and dark current and stability #1 |
5.5 |
9.00 |
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Y |
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10520C, 10540C, 10570C |
56 |
261a |
Read noise and dark current and stability #2 |
5.5 |
9.00 |
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Y |
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10520C, 10540C, 10570C |
57 |
262a |
Read noise and dark current and stability #3 |
5.5 |
9.00 |
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Y |
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10520C, 10540C, 10570C |
58 |
265a |
Scan to determine confusion limits |
5.5 |
2.00 |
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N |
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10720C |
59 |
305a |
Pipeline quality flatfields |
5.5 |
3.50 |
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N |
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10870C |
60 |
310a |
Off-axis glints |
5.5 |
15.00 |
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Y |
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10630C |
61 |
335a |
Point spread functions |
5.5 |
3.50 |
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N |
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10650C |
62 |
340a |
Ultimate scattered light levels |
5.5 |
10.00 |
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Y |
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10630C |
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Total = |
145.32 |
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118.15 |
hours |
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6.06 |
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4.92 |
days |
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William B. Latter |
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SSC/MIPS Instrument Scientist |
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Total < 9 K = |
128.01 |
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101.76 |
hours |
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16-Sep-99 |
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5.33 |
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4.24 |
days |
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