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<H2><A NAME="SECTION003431000000000000000">&#160;</A>
 <A NAME="irac2:bad-pixel-detection-and-removal">&#160;</A>
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Bad Pixel Detection and Removal
</H2>
 Before most of the reduction process can be conducted, bad pixel
 values must be removed. This is usually achieved by flagging pixels
 above or below some threshold value as bad, and replacing their values
 by those of nearby, non-bad pixels. The LAMP ON or LAMP OFF flat field
 images are a good place to start to define your bad-pixel map. To
 determine the threshold values to use, you should examine the
 statistics of the image and set thresholds 5 to 10 standard deviations
 away from the mean in both positive and negative directions. The exact
 thresholds for determination of bad pixels will depend on the details
 of your flat field observations - filter, objective lens, integration
 time and lamp voltage - so you should experiment with different values
 until you obtain a satisfactory result.

<P>
Because IR arrays are sensitive to thermal cycling and to atmospheric
 contamination, the bad pixel lists change over time.  Recent lists are
 available via the ESO WWW pages for comparison to bad pixel maps you
 generate yourself, but are unlikely to perfectly match the list
 derived from your own data.

<P>
In MIDAS, bad pixel detection is possible with the command <TT> MASK/IRAC2</TT>; the command <TT>CMASK/IRAC2</TT> can be used for bad pixel 
 removal. Refer to the MIDAS manual for further documentation of these 
 commands.

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<ADDRESS>
<I>Petra Nass</I>
<BR><I>1999-06-15</I>
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