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 $princ = ioc_get_person($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.$campn.".analysis.php"; // END PHP. ?> <? echo "MIPS-$caid, Campaign $campn IOC/SV Analysis"; ?>

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Task Outcome Summary


Abstract

The 24 micron dark calibration image has been created, and is nominal. The mean dark current is 8.8 +/- 2.6 e/s, The read noise measurement yields RN=37.5 +/- 8.3 e.

Analysis

All data were processed with DAT version 2.4 in order to derive calibrated images; the set of 50 dark DCEs (not including those with bias boosts) were coadded using mips_enhancer with the dark flag turned on. The read noise was calculated from the set of 35 read noise DCEs with the IDL script get_rdnoise, which has been modified to reject cosmic rays from 24 micron SUR data.


Results

24 µm Data

Figure 1 shows the coadded dark calibration image. The illumination pattern and mean counts are nearly identical to darks obtained on the ground. The read noise was measured from these data, with a value 37.5 +/- 8.3 e. The numbers are slightly lower (by roughly 15%) than most of the measurements in previous campaigns.


Figure 1: 24 micron dark calibration image, a coaddition of 45 10-second exposures. The data range from ~ 1 to 3 DN/s.



Conclusions

The routine dark calibration and read noise are nominal.


Output and Deliverable Products

Dark calibration image, plus read noise measurement.

Actions Following Analysis

None