// ENTER CAID, CAMPN, and Analyst WITHIN THE QUOTES IN THE FOLLOWING 2 LINES ... $caid="910"; // e.g. $caid = "90"; $campn="O"; // e.g. $campn = "D2" or $campn = "Q"; $analyst="J. Muzerolle"; // e.g. $analyst="D. Kelly"; // YOU CAN SKIP DOWN TO THE OUTCOME SECTION NOW. include ("IOC_connect.php"); // this line isn't for you include ("IOC_log_fns.php"); // this line isn't for you $db = ioc_db_connect(); $query="select * from ioc_tasks where camp_crnt = '$campn' and caid = $caid limit 1"; $result = mysql_query($query); if (mysql_num_rows($result) != 1) { echo "
Principal: = $princ;?>
Deputy: = $deplist;?>
Analyst: = $analyst;?>
AORKEYS: if (! $aorkeys) {echo "unknown";} else { echo $aorkeys;}?>
Last Updated: if (file_exists($file)) {echo date("D M d Y, H:i:s", filemtime($file) ) ;} ?>
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.
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.
The routine dark calibration and read noise are nominal.