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Detector Electronics Temperature
Prior to delivery to XRCF, the ACIS integrated flight instrument underwent
testing at MIT Lincoln Laboratories. Some of these measurements involved
operating ACIS with the Detector Electronics Assembly (DEA) at temperatures
of -17 C
and 20 C
.
These tests were used to map the gain dependence on the electronics temperature.
A detailed description and analysis of the gain calibrations are reported
in ACIS Memo #143 [Pivovaroff1997c].
The main points are summarized below:
-The DEA was stabilized at temperature Ti, (Ti = -17 C
,20 C
)
-Each chip was independently illuminated with an Al K
source and an 55Fe source
-The focal plane (FP) temperature during these measurements ranged between -116 and -119 C
-Gains were calculated by fitting a linear relationship to a gaussian centroid for the Al K
and the Mn K
line
Table 4.65 lists the mean gain
for each chip for DEA temperatures of 20 C
(hereafter LLTVhot) and -17 C
(hereafter
LLTVcold). Table 4.65
also lists the average chip gains calculated from the XRCF Flat Field (XRCFFF),
Phase I data. See Section 4.3.1 for
the details of these measurements.
Table 4.65: Mean gains for ACIS at different operating
temperatures
| FP Location |
Mean Gain (eV/ADU) |
| LLTVcold |
XRCFFF |
LLTVhot |
DEA=-17 C
FP=<-117.5> C |
DEA=13 C
FP=-110 C |
DEA=20 C
FP=<-117.5> |
| I0 |
3.812 |
3.827 |
3.840 |
| I1 |
3.809 |
3.849 |
3.857 |
| I2 |
3.563 |
3.592 |
3.610 |
| I3 |
3.839 |
3.882 |
3.891 |
| S0 |
3.689 |
3.797 |
3.811 |
| S1(BI) |
4.405 |
4.413 |
4.455 |
| S2 |
3.724 |
3.758 |
3.771 |
| S3(BI) |
4.492 |
4.507 |
4.574 |
| S4 |
4.256 |
4.306 |
4.319 |
| S5 |
4.075 |
4.101 |
4.119 |
|
It is clear from the data that the gains increase with increasing DEA temperature.
In order to quantify this relationship, we have made a linear fit of the
gains as a function of temperature. Figure 4.97
shows the linear best-fit plotted against the measured gain values. The
hash marks simply indicate the data point and are not representative of
errors. The LLTVcold data for I0 and S0 are known to
have a problem with drifting biases, so these two data points are suspect4.7.
With only three data points to fit, the incorrect LLTVcold
gains greatly influence the fits and skew the slope of the expected lines.
Excluding I0 and S0, the data seem to follow the linear relationship quite
reasonably. The small deviations from linearity are expected, as only two
data were used to define the LLTV gains.
Figure 4.97: ACIS gain variation as a function of DEA temperature.
 |



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Please address comments and questions to Dr. John Nousek ( nousek@astro.psu.edu
)