// ENTER CAID, CAMPN, and Analyst WITHIN THE QUOTES IN THE FOLLOWING 2 LINES ... $caid="920"; // e.g. $caid = "90"; $campn="V"; // e.g. $campn = "D2" or $campn = "Q" or $campn="meta"; $analyst="K. Su"; // 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 "; $result = mysql_query($query); if (mysql_num_rows($result) < 1) { echo "
Principal:
Deputy:
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) ) ;} ?>
As expected, this task generated a total of 30 Si:As DCEs on the star and 7 more in the stim IER.
The total counts from the star in all 30 DCEs are computed using IDL program with the same aperture parameters as before. Details about the aperture photometry and sky background in individual DCE are available here. The average total counts are 6.927+04 ± 1.218e+03 (1.76%) DN/s (ignoring the boost DCEs), and the distribution is shown in Figure 1. Using the aperture correction of 1.146, the total counts from the target is 7.938e4 DN/s, so the ratio of DN/s to Jy is 1.47e5. This conversion factor continues to be stable.
Figure 1: Counts for HD159330 as a function of DCE number.
The stimulator IER behaved as expected, producing 7 images of the flat-field stimulator. The data were processed with mips_sloper in a fashion identical to that described above for the sky images. Figure 2 shows the historgram over the whole array in individual DCE. The 5-sigmaclip mean value is also listed in each DCE. (Note that 1st DCE has SUR algorithm wrong, so the statistics from DCE#1 should be ignored.)
Figure 2: Histrogram on the Stim over DCEs
The flux calibration is delivered in this writeup. The calibration images and mosaic are available should they be needed.