Statistics – Applications
Scientific paper
Jul 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hstc.worke..55s&link_type=abstract
"2010 Space Telescope Science Institute Calibration Workshop - Hubble after SM4. Preparing JWST, held 21-23 July 2010 at Space T
Statistics
Applications
Scientific paper
The ACS/WFC detector consists of two CCDs, each of which is read out through two amplifiers. While reading each quadrant of the detector, the electronic crosstalk between the amplifiers induces faint, typically negative, mirror-symmetric ghost images on the other three quadrants. The effect is strongest for high-signal offending (source) pixels. Analysis of the pre-SM4 crosstalk showed that its impact on ACS/WFC science was insignificant and can be ignored in most science applications. In this report, we analyze crosstalk after SM4. Crosstalk due to low-signal offenders is much weaker than before SM4 and does not produce ghosts similar to those seen in pre-SM4 images. For high-signal offending pixels, we find substantial differences between the gain=1 e^-/DN and gain=2 e^-/DN cases. For the default gain setting of 2, the crosstalk is similar to what it was before the SM4, up to 5-8 e^-" per pixel on the same CCD. For gain=1, the crosstalk is 100 e^- per pixel for saturated offending pixels on the same CCD, which is more than an order of magnitude above the pre- SM4 level. The crosstalk from saturated pixels is 20-30 e^- per pixel on the other CCD, which is also much higher than it was before SM4. For gain=1.4, the crosstalk is very similar to that at gain=2.
Cheng Edward
Grogin Norman Andrew
Loose Marcus
Sirianni Marco
Suchkov Anatoly A.
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