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Repeatability and Estimated Errors
in Relative Quantum Efficiency Measurements of Front-Illuminated Detectors
In Table 4.61 we have
computed the fractional difference (1-XRCF/CSR) between the relative QE
measurements made at each site. The relative QE ratios at XRCF for the
frontside devices are in excellent agreement with the ratios obtained at
CSR. Indeed, averaged over seven FI chips and the lowest three energies,
the mean difference in relative quantum efficiency is
,
where the error is the standard deviation about the mean, and the RMS deviation
about the mean is 1.1%. If we assume that the CSR and XRCF relative QE
measurements in this energy range each have the same random error, and
account properly for the normalization of the CSR measurements by the efficiency
of S2 required to make this comparison, we infer that the error on a single
relative QE measurement is (very nearly)
.
This estimate is only slightly larger than the value obtained from internal
consistency of the MIT CSR measurements alone (
;
see section 4.7.2) For purposes
of QE model fitting, to be discussed in Section 4.8,
we will adopt the larger value as the uncertainty in the relative QE measurement.
Table 4.61: Fractional Difference (1-XRCF/CSR) between
Relative Detection Efficiencies at CSR and XRCF--Referenced to S2
| Flight |
Position |
Frac. Rel. Eff. Diff. vs. Energy (keV) |
| Device |
|
0.525 |
1.740 |
4.509 |
8.040 |
| |
|
O |
Si |
Ti |
Cu |
| w203c4r |
I0 |
0.019 |
-0.003 |
0.009 |
-0.006 |
| w193c2 |
I1 |
0.011 |
-0.002 |
0.006 |
-0.004 |
| w158c4r |
I2 |
-0.003 |
-0.013 |
0.005 |
0.013 |
| w215c2r |
I3 |
0.019 |
-0.015 |
0.002 |
-0.014 |
| w168c4r |
S0 |
0.029 |
0.001 |
-0.010 |
-0.026 |
| w182c4r |
S2 |
0.000 |
0.000 |
0.000 |
0.000 |
| w457c4 |
S4 |
0.004 |
-0.003 |
-0.010 |
 |
| w201c3r |
S5 |
0.012 |
0.001 |
-0.003 |
-0.042 |
| FI Mean |
|
0.013 |
-0.005 |
-0.000 |
-0.013 |
| FI Std Dev. |
|
0.011 |
0.006 |
0.008 |
0.019 |
| w140c4r |
S1 |
-0.124 |
-0.001 |
0.080 |
-0.010 |
| w134c4r |
S3 |
-0.097 |
-0.010 |
0.055 |
-0.050 |
| BI Mean |
|
-0.111 |
-0.006 |
0.068 |
-0.030 |
| BI Std Dev. |
|
0.019 |
0.006 |
0.018 |
0.028 |
This data point was excluded because the XRCF bias |
| for this point was peculiar. |
|
The data at 8 keV require special comment for two reasons. First, the
bias obtained from ACIS telemetry for S4 for the 8 keV measurement (ACIS
XRCF Science Run 93, TRW ID's I-IAS-SG-1.032 and I-IAS-EA-2.043 through
I-IAS-EA-2.048) is peculiar, showing excess charge of order 5 electrons/pixel.
The spectral resolution in S4 is severely compromised (FWHM
eV) by the bias error, and this in turn affects the measured quantum efficiency.
As a result, a replacement (telemetry) bias was used (taken from ACIS Science
Run 89) to compute the relative efficiency listed in Table 4.59.
Even with the replacement bias, the spectral resolution was not quite as
good as measured at MIT. For this reason, we regard this measurement as
suspect, and have quoted statistics in Table 4.61
with this point excluded. The cause of the bias error is not understood.
The high-speed tap data obtained for S4 during (a subset of) ACIS XRCF
Science Run 93 show no obvious anomalies.
Second, as noted above, the cross-calibration of the two reference detectors
w190c3 and w103c4 at MIT is rather uncertain at 8 keV. We require this
cross-calibration to compute the response of S2 relative to reference detector
w190c3, since S2 was only measured with respect to reference detector w103c4.
Formally, the RMS uncertainty of this cross-calibration (derived from the
reproducibility of three measurement sets) is about 0.03 (1-sigma). This
uncertainty is expected to dominate other errors in the QE, relative to
S2, of the five devices (I0, I3, S0, S4 and S5) for which w190c3 is the
primary reference standard.
Nevertheless, excluding the S4 point, we find a mean relative quantum
efficiency difference of
,
where the error is the standard deviation of the mean, and the RMS deviation
of measurements about the mean is 0.019. Thus, whatever the source of the
uncertainty in the CSR measurements of the w190c3 vs. w103c4 cross-calibration,
the value we have adopted for this cross-calibration is just consistent,
at 90% confidence, (i.e., within 1.3%) with the XRCF relative quantum efficiency
data.
A related comparison between the best-fit quantum efficiency models
and the XRCF data is presented in Section 4.8.



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