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The effective exposure times for the 1983-1985 Epoch ITFs were derived
by Imhoff (1984b and 1986), by De La Peña and Coulter (1996) for the
1992 Epoch LWP ITF, and by De La Peña for the LWR ITFs. During the
creation of the 1983-1985 ITFs in their own geometric space for the
NEWSIPS system, if additional images were deemed usable in contrast to
those originally chosen by Imhoff, the effective exposure times were
modified to reflect the use of additional images.
Table 6.1 lists the effective exposure times (FN exposure
values) for each level of the ITFs used in the Final Archive. These
exposure values have been normalized to an arbitrary scale such that the
FN associated with the lowest level of an ITF is 0.0.
Table 6.1:
ITF Effective Exposure Times (seconds)
ITF |
SWP |
LWP |
LWR ITFA |
LWR ITFB |
Level |
Epoch 1985 |
Epoch 1992 |
Epoch 1983 |
Epoch 1983 |
1 |
0.000 |
0.000 |
0.000 |
0.000 |
2 |
32.919 |
38.750 |
35.880 |
35.607 |
3 |
67.946 |
78.737 |
72.974 |
72.425 |
4 |
104.147 |
121.868 |
91.067 |
89.708 |
5 |
131.397 |
168.958 |
125.213 |
125.621 |
6 |
166.296 |
200.756 |
156.510 |
162.627 |
7 |
223.034 |
237.941 |
193.275 |
198.780 |
8 |
269.680 |
278.107 |
245.053 |
254.362 |
9 |
340.471 |
341.073 |
283.705 |
288.706 |
10 |
408.490 |
396.582 |
320.355 |
325.599 |
11 |
473.749 |
483.497 |
385.554 |
401.720 |
12 |
575.995 |
561.518 |
471.557 |
490.480 |
Next: 6.3 Description of the
Up: 6 Photometric Correction (PHOTOM)
Previous: 6.1.4 Periodic Noise
Karen Levay
12/4/1997