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Michelle Readnoise

For Michelle the readnoise from the calibration system is also first divided by a factor to take multiple non-destructive reads into account:


\begin{displaymath}RNE = \frac{RN}{\sqrt{\frac{N_{ND} * ( N_{ND} + 1 )}{12 * ( N_{ND} + 1 )}}} \end{displaymath}

where RNE is the readnoise per exposure, in electrons, RN is the readnoise in electrons, and NND is the number of non-destructive reads.

The formula used to determine the variance due to readnoise is:


\begin{displaymath}V_{RN} = \frac{RNE^{2}}{N_e * gain^{2}} \end{displaymath}

where RNE is the readnoise per exposure, in electrons, Ne is the number of exposures per integration, and gain is the detector gain in electrons per ADU.



next up previous 306
Next: UIST Readnoise
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ORAC-DR -- spectroscopy data reduction
Starlink User Note 236
Paul Hirst
Brad Cavanagh
Joint Astronomy Centre, Hilo, Hawaii
October 2005
E-mail:ussc@star.rl.ac.uk

Copyright © 2005 Particle Physics and Astronomy Research Council