<? echo "MIPS-$caid, Campaign $campn IOC/SV Analysis"; ?>

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

This meta task is to track the 70 and 160 micron dark/read noise measurements for IOC/SV.

Analysis

The dark data were reduced using the DAT version 2-32, 2-41. Sensitive cosmic ray detection (mips_sloper comandline switch -q) was used and the electronic nonlinearity correction was not applied. The dark datasets were run through mips_caler. Finally, the dark images for d2a and d2b were created using mips_enhancer. The mips_enhancer was run with the commandline options "-OW -OD -D". The read noise was measured from the read noise datasets using the get_rdnoise.pro program.

Results

Darks - 70 micron

The d2a dark images are shown here along with average measurements. The d2b dark images are not shown as they systematically brighter. A comparison to ground test data (LBTC) is given as well. The numbers are tabluated below.

Campaign	A/B Bias [mV]	Stim DAC	Dark Counts MIPS70 units Side A
Ground-LBTC			(7.99 +/- 7.39)X10^-3
CamG	40/40	0x33	(6.24 +/- 3.72)X10^-3
CamH	40/40	0x33	(6.04 +/- 2.95)X10^-3
CamH1 (CE2)	40/40	0x33	(5.30 +/- 2.66)X10^-3
CamI	40/40	0x33	(5.93 +/- 6.23)X10^-3
CamK	30/22	0x3C	(3.15 +/- 3.26)X10^-3
CamO	62/50	0x2D	(7.96 +/- 4.41)X10^-3
CamP	62/50	0x2D	(10.2 +/- 5.46)X10^-3

Darks - 160 micron

The d3 dark images are shown here along with average measurements. The numbers are tabluated below.

Campaign	1/2/3/4 Module Bias [mV]	Stim DAC	Dark Counts MIPS160 units
CamK	10/15/15/15	0x4D	(2.58 +/- 1.28)X10^-2
CamO	10/15/15/15	0x4D	(2.46 +/- 1.27)X10^-2
CamP	10/15/15/15	0x4D	(2.48 +/- 1.10)X10^-2

Noise - 70 micron

The noise were determined for the d2a noise datasets taken during routine IOC darks. For details of how these measurements were make, see the task writeups for individual campaigns. The noise measurement given here is the noise in excess of that expected from photon statistics. The noise images can be found here.

Only d2a data is shown, d2b gives very similiar read noise results, expect for a factor of two higher dark current.

		Side A			Side B
Campaign	A/B Side Bias [mV]	Noise [e]	Signal [e/s]	DCEs/pixels	Noise [e]	Signal [e/s]	DCEs/pixels
Ground-LBTC	40/40	91.1 +/- 30.4	180.0 +/- 58.1	49.32/?
CamG	40/40	1024.6 +/- 234.8	537.6 +/- 182.3	48.32/?
CamH	40/40	1055.1 +/- 229.0	552.9 +/- 176.8	48.23/?
CamH1 (CE2)	40/40	1313.1 +/- 277.8	612.5 +/- 181.0	48.28/?
CamI	40/40	1135.6 +/- 262.2	531.5 +/- 166.9	48.32/?
CamK	30/22	592.7 +/- 137.3	305.1 +/- 117.7	48.3/468	3465.3 +/- 1268.0	365.1 +/- 171.7	44.5/501
CamO	62/50	1366.4 +/- 332.2	841.7 +/- 350.2	48.19/468	10603.1 +/- 4427.1	1267.6 +/- 1318.2	44.64/501
CamP	62/50	2660.4 +/- 580.6	1163.5 +/- 1456.7	48.22/468	21840.5 +/- 6636.7	2090.7 +/- 1411.4	46.53/501

Noise - 160 micron

The noise were determined for the d3 noise datasets taken during routine IOC darks. For details of how these measurements were make, see the task writeups for individual campaigns. The noise measurement given here is the noise in excess of that expected from photon statistics. The noise images can be found here.

Campaign	1/2/3/4 Module Bias [mV]	Noise [e]	Signal [e/s]	DCEs/pixels	Eng. Noise [e]
CamH	25/30/30/30	14434.5 +/- 6839.5	11424.7 +/- 7159.2	48.29/34	113.0 +/- 20.2
CamI	10/15/15/15	2503.6 +/- 1027.0	3481.7 +/- 2273.4	47.85/34	68.1 +/- 14.8
CamI	10/15/15/15	2883.2 +/- 1496.2	3748.4 +/- 2447.5	47.94/34	70.3 +/- 11.9
CamI	10/15/15/15	2186.6 +/- 938.3	3347.6 +/- 2698.8	47.65/34	66.0 +/- 9.1
CamI	15/20/20/20	4909.2 +/- 3060.0	5238.1 +/- 3994.4	47.79/34	79.2 +/- 12.0
CamI	15/20/20/20	4897.5 +/- 2773.0	5423.9 +/- 4057.4	47.85/34	78.4 +/- 22.5
CamI	20/25/25/25	10421.3 +/- 6100.4	9317.6 +/- 8108.2	47.5/34	120.1 +/- 80.4
CamI	20/25/25/25	10395.5 +/- 7040.9	8918.3 +/- 6491.6	48.18/34	139.9 +/- 99.3
CamI	30/35/35/35	59654.4 +/- 19963.0	31149.7 +/- 11428.6	39.18/33	419.0 +/- 155.5
CamI	30/35/35/35	61694.4 +/- 18138.0	29730.8 +/- 9371.3	39.18/33	651.7 +/- 267.8
CamK	10/15/15/15	1636.7 +/- 827.2	2392.1 +/- 1538.0	48.38/34	63.4 +/- 12.7
CamO	10/15/15/15	1199.9 +/- 656.0	2032.5 +/- 1328.4	48.85/34	57.6 +/- 9.6
CamP	10/15/15/15	1844.6 +/- 823.8	2314.3 +/- 1298.6	48.56/34	76.3 +/- 21.6

Other Noise measurements: Bias Voltage Optimization - Campaign I.

Conclusions

Awaiting more data.

Output and Deliverable Products

Awaiting more data.

Actions Following Analysis

None.