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eso-midas-doc-13SEPpl1.2-3.mga5.i586.rpm

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<H2><A NAME="SECTION002513000000000000000">&#160;</A> 
<A NAME="reduction-steps">&#160;</A>
<BR>
Reduction Steps
</H2>

<P>
The software now available is a package for doing relative calibrations of the
pixels, for averaging frames, and for cleaning images. Cleaning in this
context means removal of instrumental faults and other defects from the
images. A list of the relevant commands is provided for reference in the 
section&nbsp;<A HREF="node453.html#ccd-commands-summary">B.1.10</A> of this appendix. 

<P>
The CCD-reduction involves the steps outlined below. Steps in paranthesis 
[...] are optional but see the following discussion to determine if they are
optional in your particular case. 
<UL>
<LI>[ Remove irrelevant columns of all frames ]
<LI>[ Bias correct all frames ]
<LI>compute an average DARK 
<!-- MATH: $\Longrightarrow$ -->
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DARK_AVG
<LI>[ remove defects from DARK_AVG ]
<LI>compute an average FLAT 
<!-- MATH: $\Longrightarrow$ -->
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FLAT_AVG
<LI>dark subtraction 
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FLAT_AVG = FLAT_AVG - DARK_AVG
<LI>[ remove defects from FLAT_AVG ]
<LI>[ normalize the FLAT_AVG,( see Eq.&nbsp;(<A HREF="node442.html#ccd-6">B.6</A>)) 
	  
<!-- MATH: $\Rightarrow$ -->
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FLAT_NRM ]
<LI>dark subtraction 
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SCIE_FRM = SCIE_FRM - DARK_AVG
<LI>[ remove defects from SCIE_FRM ]
<LI>flatfield the scie-frame SCIE_FLAT = SCIE_FRM/FLAT_NRM
<LI>compute the average of science frames 
<!-- MATH: $\Rightarrow$ -->
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SCIE_AVG
</UL>The sections below describe and discuss the various options which
are available to perform the needed operations. These sections discuss
bias corrections, techniques for computing averages, techniques for
cleaning images and removing specific defects, and finally how to
use the <TT>COMPUTE</TT> command for dark subtraction and flat fielding.

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