There is a problem w/ your write-up. Check that you have valied entries for \$CAID and \$Campn in your analysis.php file. If that checks out, then Contact Stansberry"; return ; } // get first matching task $row = mysql_fetch_array($result); $title = $row["title"]; $princ = $row["principal"]; $deputy= $row["deputy"]; $campn0 = $row["campn0"]; $aorkeys = $row["aorkeys"]; // get real name of principal, deputies $princ = ioc_get_person($princ); $princ = $princ[0]; $deps = explode(",",$deputy); foreach ($deps as $depty) { $depty = trim($depty); $depty = ioc_get_person($depty); $depty = $depty[0]; $depty = explode(",",$depty); $depty = $depty[0]; // last names only $deplist[] = $depty; } $deplist = implode(", ", $deplist); $caid = sprintf("%03d",$caid); $file = "mips-".$caid.$campn.".analysis.php"; // if more matches, append the AORKEYS from those $numrows = mysql_num_rows($result); if ($numrows > 1) { $aorkeys = " " . $numrows . " Task Executions:  ". $aorkeys; for ($i=0;$i < mysql_num_rows($result); $i++) { $row = mysql_fetch_array($result); $morekeys = $row["aorkeys"]; $aorkeys = $aorkeys .';  '.$morekeys; } } // END PHP. ?> <? echo "MIPS-$caid, Campaign $campn IOC/SV Analysis"; ?>

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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. Sets 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 was at T ~ 26 K; the data are consistent with the lowering thermal background compared to the previous campaign. The Ge arrays are both saturated; however, slopes can be fit for most of the pixels at 70 microns.

Analysis

All data were processed with DAT version 2.21 in order to derive calibrated images. The 24 micron images were coadded using mips_enhancer with the dark flag. Slopes can now be fit to most pixels at 70 microns, though almost all ramps are saturated.


Results

The 24 µm dark remains dark. Figure 1 shows the calibrated, coadded image of all 50 DCEs in the observation (combined with mips_enhancer). Mean counts are 4.7 DN/s (this is probably artificially inflated due to larger slopes in the bottom part of the array; see the MIPS-190 report).


Figure 1. Coadded 24 µm dark image (not including bias boost DCEs). Data values range from ~ 0 to 15 DN/s. Bad pixels have been masked out.


70 µm Data

The 70 µm array is getting less saturated, especially at the 70 dark A and 160 dark mirror positions. Slope images for these positions and the 70 dark B position are shown in Figure 3. Mean slopes at the 70 dark A position are ~ 28,500 DN/s.


Figure 3. 70 µm slope images at the 70 µm dark A position (left), dark B position (middle) and the 160 µm dark/SED mode position (right). Values range from 0 (saturated) to ~100,000 DN/s.


160 µm Data

The 160 µm array could not be packed due to problems with the pipeline. Inspection of MIPL data indicated it is still fully saturated.


Conclusions

The 24 µm darks are at levels comparable with ground-test data; no scattered thermal background emission is evident. The 70 µm array is getting less saturated, with enough unsaturated reads to fit slopes to a majority of pixels at the 70 dark A and 160/SED dark positions.

Output and Deliverable Products

None.

Actions Following Analysis

None.