Electron Bleed

Frequently stars are too bright for the CCD's "wells" to accomodate all of the photons; this causes signal to "bleed" along the adjacent rows and columns. Unlike diffraction spikes bleed only occurs when all, or part of, the star is visible on the image.

Example image of signal bleed

NON-REPORTABLE: Signal Bleed

CHARACTERISTICS:
Sharp, vertical/horizontal line(s) with high signal level relative to background (the bleed is the horizontal line that changes its extent on each pass - there is some evidence that the charge is is spilling vertically as well but that may be introduced in the electronic readout). Electron bleed always originates in a bright star or galaxy.

Example image of signal bleed

NON-REPORTABLE: Signal Bleed

CHARACTERISTICS:
Bleed favors one direction. Again, originates in a star.

« Galaxies