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The Transfer Curve

 

The transfer curve is a plot of the square of the noise (variance) in an image after correction for flat-field effects versus the mean counts. It was first developed as a tool for investigation of CCD properties by Janesick (1987) and is used to measure the CCD conversion factor in electrons/ADU.

At illumination levels less than saturation, the variance of the signal in electron units, is given by:

where is the noise in the signal and is the readout noise in electrons. Assuming Poisson statistics, is the signal in electrons and is equal to the illumination level in electrons, which is the illumination level in ADU, , multiplied by the CCD conversion factor (or, imprecisely, the gain), g, in electrons/ADU. Similarly, is the standard deviation of the signal in ADU, , multiplied by g. Thus:

or

Therefore, the slope of the plot of the variance of the signal in ADU, , versus the mean counts, , is the inverse of the CCD conversion factor.

The readout noise is obtained from the square root of the y-intercept, which is simply the variance of the signal in a bias frame, divided by the conversion factor.

Note: at high count levels, the transfer curve levels off and may turn over. This is because the system has become saturated. Saturation may be defined in either of two ways.

Normally, the system gain should be set so that digital saturation is encountered at signal levels less than analogue saturation.





next up previous
Next: Transfer curves: Data Required Up: In situ CCD testing. Previous: Bias images: Reduction Procedure



Tim Abbott, tabbott@ctio.noao.edu
Thu Jun 29 11:07:29 HST 1995