ACS anomalies and artifacts
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CCD amplifier cross-talk, or electronic ghosts
Images obtained with the ACS/WFC are affected by a small amount of electronic
cross-talk between the four CCD quadrants that correspond to the four
amplifiers of the two detectors. The effect produces mostly negative
electronic "ghost" images in a given quadrant that mirror real images recorded
on other quadrants, although faint positive ghosts have also been
observed.
Figure 1
shows an image taken from program GO-9425 (the GOODS
survey) that shows the presence of cross talk.
The stretch was chosen to highlight the ghost images. The counts in
the ghost images are typically lower than the surronding background by a few
(typically 1 to 4 DN/pixel), and quantitative analysis (e.g., photometry) is
rarely affected at a significant level. A detailed analysis of the cross-talk
effect is underway and will soon be reported in an Instrument Science Report.
Preliminary analysis suggests that the strength of the cross-talk is
significantly weaker in images acquired with gain setting GAIN=2 than
in images taken with GAIN=1. For example,
Figure 2
shows a 620 sec
exposure (from GO-9425) through the F606W passband taken with GAIN=1
For comparison,
Figure 3
shows a 410 sec exposure (from program
GO-9433) of a different field but through the same passband taken with
GAIN=2.
The two exposures are relatively similar; sources with similar flux
would produce similar numbers of electrons in each image. While the
cross talk is clearly observed in Figure 2, it does not seem to affect
Figure 3.
ACS/WFC observers who are concerned about the quantitative influence
or visual appearance of cross-talk are advised to use GAIN=2 instead
of the default GAIN=1. Such observers should also consult
Section 7.6
of the ACS Instrument Handbook
for a discussion of other pros and cons of these GAIN
settings. Specifically, GAIN=2 yields better dynamic range than
GAIN=1, but has the disadvantage of slightly increased read noise
relative to GAIN=1. Further discussion of these trade-offs may be
found in
ACS ISR 2004-01.
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