Contact Stansberry - "; echo " there is a problem w/ your write-up.\n"; return ; } $row = mysql_fetch_array($result); $title = $row["title"]; $princ = $row["principal"]; $deputy= $row["deputy"]; $campn0 = $row["campn0"]; $aorkeys = $row["aorkeys"]; // get real name of principal, deputies //echo "retrieving name for principal code $princ
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Task Outcome Summary


Abstract

This task is intended to monitor background counts for each array, tracking the cooling of the telescope. A set of darks were obtained at 24, 70, and 160 microns in the standard fashion. All the expected data were received and are nominal. In this campaign, the telescope primary mirror temperature was about 128 K, and the resulting thermal background saturated all three arrays, even when they were pointed to the internal dark positions using the CSMM. However, some pixels in the 70 micron array were on-scale in the first read after the reset, and some preliminary information has been derived from those images.

Analysis

All data were processed with the DAT in order to derive calibrated images. Images would normally be combined with mips_enhancer, but as all the data in this case are saturated, this step was neglected. Unprocessed ramps for the Ge arrays were inspected for unsaturated reads at the beginning of each ramp.


Results

24 µm Data

24 micron SUR slopes and first differences (Figures 1 and 2) are all zero, with the exception of two typically bad pixels. Thus, the array was saturated in less than 0.5 seconds. One exposure of raw-mode data was taken for mips-915, CE State Validation and Functional Test. In those data the first read after the 2 bias boost frames (the reset-read frame) showed the normal patterns and DN levels for such data, confirming that the 24 µm array is alive.


Figure 1. 24 µm slope image. All values are zero except for two bad (low-response) pixels.


Figure 2. 24 µm first difference image. All values are zero except for one bad (low-response) pixel.


70 µm Data

Data ramps on the 70 µm array saturate at the first read for most pixels, but are unsaturated on the first read for a few. Figure 3 shows two 70µm images which indicate the degree of saturation of each pixel at the first read after the reset at the beginning of the DCE. Because all pixels on the the array are reset simultaneously, but pixels are read-out sequentially thereafter, the effective integration time for the first read depends on the order in which the pixels are read-out, and ranges from 1/8th to 1/4 of a MIPS second.


Figure 3. 70 µm slope images derived from the difference between the first and second reads on the data ramps, displayed with an inverted greyscale (i.e. dark is high slope, light is 0 slope). The two frames were acquired while the CSMM was deflected to the 70 µm "Dark A" position (left), and the 160 µm Dark position (right), which places the 70 µm array in almost exactly the nominal SED mode position. Saturated pixels show zero slope and are white; unsaturated pixels appear dark, with the darkest pixels being those that were least saturated at the first read. The readout order of the pixels is indicated by the labels on the right-hand image.

Based on the above supposition that some of the pixels were not saturated on the first read after the reset, several interesting features are apparent in Figure 3:

Figures 4 and 5 show raw images of the DN at the first read for the 70µm array, and correspond to the left and right panels in Figure 3. Saturated pixels are white, unsaturated ones are darker. Visible in this representation are readout [4,7] (medium grey 4x8 block, DN = 48k, at lower left), which developed a short to chasis ground during ATLO testing, and readout [4,4] (black 4x8 block, DN = 0, bottom middle), which has developed a short, probably on its output line, after launch.


Figure 4. 70 µm first-read DN image for an exposure taken at the 70 µm Dark A position.


Figure 5. 70 µm first-read DN image for an exposure taken at the 70 µm SED position (CSMM was configured for 160 µm dark, which is almost identical to SED nominal for the 70 µm array).

The figure below summarizes out preliminary conclusions about the 70 µm array. It should be straight-forward to confirm or discount the more preliminary of them by comparing with Scatttered Background Monitor data from Campaign B.



160 µm Data

Figure 6 shows the DN at the first read, and uses unaltered MIPL output such that high saturation occurs at -1DN, rather than at 65k DN. In the particular case of the 160 µm array the unaltered MIPL DN show readouts 3 and 5 more clearly, because readout 3 rails at about +18k DN, and readout 5 rails at about -600 DN. The 16 engineering pixels occupy the center row in the image, with pixels 3, 8, 13, and 18 being empty.


Figure 6. 160 µm first-read image. All DN values are -1 except for the two shorted readouts in the bottom row. Readout 3 DN are about +18k, reflecting a DC offset of the data ramp by -48k; Readout 5 DN are about -600 DN, reflecting a tiny DC offset. Both offsets are caused by thermally activated shorts on the ground-sense lines for these readouts.


Conclusions

The Campaign A1 data for this task were badly saturated, as expected. The 70 µm data were not entirely saturated, and suggest that overall the array is healthy, that the ground data system is ordering the data appropriately, and that the orientation of the array is as expected from pre-flight predictions and Code 5 modeling. No useful measurement of scattered background can be made from these data, but by comparing them to data to be taken in later campaigns it should be possible to derive the rate at which the background is declining, at least at 70 µm.

Output and Deliverable Products

None.

Actions Following Analysis

None.