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Spatial Distribution
While the spatial distribtuion of ExtCalSrc flux does not directly influence
the gain calculation, it is intimately tied to the detected count rate
of the K
lines. Two types of variation are observed. First, for a given source,
there will be a certain pattern expected from its collimation beam and
a reduction of intensity as the distance from the source axis increases.
Second, since the photons for each flavor of K
lines come from a seperate source, we expect that intensity patterns will
vary source to source. The housing for the ExtCalSrc contains locations
for four individual sources (only three are occupied). Looking down on
the focal plane such that S0 is in the lower left and I1 in the upper right
(see Figures below), the Al source is in the upper left, the Ti source
is in the upper right, and the Mn source is in lower left. Figures 4.115,
4.116, & 4.117
contain the intensity maps for each K
line. To account for chip-to-chip differences in quantum efficiency, all
the chips have been normalized to the QE of S2 at each energy. For example,
if S0 is only 90% as efficient as S2 at Al K
,
the observed Al K
intensity for S0 is multiplied by 1.0/0.9. Each 1024
1024
CCD image was binned into a 64
64 array (16 pixels
16
pixels/cell). For the typical 4800 sec exposures taken during ISIM-TV1,
the total counts in a single cell is approximately equal to the count rates
in Table 4.82. Since the Poisson
noise was rather large (19%, 17%, and 10% for Al, Ti, and Mn) the images
were smoothed with a 5
5
box car function to reduce 1
statistical fluctuations to the
5%
level. Finally, the map was normalized with respect to the mean intensity
of S2 (i.e. the mean intensity of S2 is unity for all the maps).
The most obvious of the macroscopic features is the patchy nature of
the maps that results from Poisson fluctuations. The BI chips also contain
significant banded structure along the quadrant boundaries and the top
(row 1024) of the chip. This structure results from using a global value
for the quantum efficiency, rather than accounting for the measured spatial
variations in QE. This effect is most notable in chip S1 at Ti and Mn4.11.
Finally, the intensity distribution is discernable. For example, at Mn
chips S4 and S5 have less flux, consistent with the placement of the bare
55Fe source in the lower left of the ExtCalSrc holder. The Ti
intensity dramatically dereases at the outer edge of S0, while the Al intensity
drops dramatically at the egde of S5. Both of these structures also agree
with placement of the Ti source in upper right holder position (farthest
from S0) and the Al source in the upper left holder position (farthest
from S5).
Figure 4.115: Relative intensity map
of ExtCalSrc Al K-alpha. Quantum efficiencies have been normalized with
respect to S2. Intensities were then normalized with resepct to S2.
Figure 4.116: Relative intensity map
of ExtCalSrc Ti K-alpha. Quantum efficiencies have been normalized with
respect to S2. Intensities were then normalized with resepct to S2.
Figure 4.117: Relative intensity map
of ExtCalSrc Mn K-alpha. Quantum efficiencies have been normalized with
respect to S2. Intensities were then normalized with resepct to S2.




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Sensitivity to Visible-Band
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External Calibration Source
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Please address comments and questions to Dr. John Nousek ( nousek@astro.psu.edu
)