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:
Deputy:
Analyst:
AORKEYS:
Last Updated:
Task Outcome Summary
- DATA STATUS: Nominal
- TASK OUTCOME: Nominal
Abstract
To measure the pixel locations (i.e. array orientation, scale) as a function of scan mirror angle for the 70 micron narrow array. The goal of this task is to estimate the location of the 70 micron narrow prime frame with repsect to the telescope boresight. The location of the MIPS instrument frames are found in the frame tables and are given as brown angles. In order to estimate the instrument pointing frame (IPF), a combinations of spacecraft moves and mirror motions places the star on several locations on the array. In addition, these observations are "sandwiched" between observations of stars with the two PCRS. The MIPS team calibrates data and centroids the star on the 70 micron narrow array. These centroided values are passed to the IPF team who uses observations of stars with the PCRS to provide the final calibration and estimate brown angles need to locate the instrument frame.
Our first frame table change for the 70 micron narrow field (FTU 10) was a result of analyzing the 966 campaign G data (this was a bouns!).
We calibrated the data with the data and used IPD3 to centroid the images. We did not receive all the data for this campaign because the Solar storm caused SIRTF to go into stand-by mode during the observations. However we received enough data to use for the coarse focal plane survey.
We centroided this data 3 times. First we used IPD3 in an interactive fashion to centroid 59 images. The IPF result from these centroids is in report ID102118.pdf They recommended brown angles went into to FTU 12 and were:
The centroiding program written for the FPS did not work to the desired level because of the large noise on side B. Therefore we had to search for another automatic centroiding rountine. We found two methods,one using IDP3 (in an automatic fashion) and one using IRAF. Using both of these software packages we re-centroided the data and sent the new centroids to the IPF team. The results from using the IRAF centoiding program are in ID202118.pdf and the results from the IDP3 routine are in ID203118.pdf . They differed little from each other. FTU 14 was done with the results from ID203118.dat. The resulting brown angles were
After FTU 14 the IPF team gave an accuracy of the locating the 70 micron narrow prime frame center as 0.3013 arc seconds. The requirement was 1.12 arc seconds.
For a complete summary of frame table updates see :
Frame Table Updates: Meta task 2080
Analysis
The data was calibrated using mips_sloper and mips_caler and calibration files provided for this campaign. We centroided 59 images with IDP3. We looked at another 26 images but either the image fell in the dead read out or the signal was bad and we did not use it.
Results
This data was centroided three times. The first time 59 images were centroided using IDP3 in
an interactive mode. The results from this run are in report ID102118.pdf and were used for FTU12. The comments from this report are as follows:
This data was also centroided using IRAF and the results are in report ID202118.pdf The comments from this report are as follows:
Finally this data was centroided using IDP3 in an automatic mode and the IPF results are in
report ID203118.pdf . THe brown angles calculated from this run went into FTU 14. The comments from this report are as follows:
Conclusions
Output and Deliverable Products
Delivered a CA and CS file to the IPF team
Actions Following Analysis
Updated FTU 12 and FTU 14.