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"; ?>

Principal:
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Last Updated:

Task Outcome Summary

Abstract

This task is designed to measure the image quality and offset from nominal focus for the MIPS 24 micron channel. The data obtained were excellent, with the exception of the left-right frame flip anomaly and the rotated world coordinates in the image headers. The focus check in campaign D2 was designed to exercise the flat fielding and PSF analysis methods needed to produce quantitative estimates during campaign E, which followed 36 hours later. The goal of rehersing for campaign E was achieved, although no conclusive results were obtained for MIPS focus. Measurements of the image core FWHM showed that the 24 micron channel was within +/- 50 microns of optimum focus.

Analysis

Results


Figure 1: MIPS 24 micron images of (left) K star HD 53501; (center) in-focus STinyTIM simulation; and (right) G star HD 2151. All are displayed in a log scale.


Figure 2: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 3: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 4: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 5: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 6: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 7: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 8: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 9: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 10: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 11: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 12: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 13: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 14: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 15: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 16: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 17: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 18: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 19: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 20: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 21: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Figure 22: MIPS 24 micron images of (left) K star HD 53501; (center) defocused STinyTIM simulation; and (right) the sky/model ratio. All are displayed in a log scale.


Conclusions

Output and Deliverable Products

Actions Following Analysis