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

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<H3><A NAME="SECTION00841300000000000000">
ANALYSE/ROMAFOT</A>
</H3>
   <TT>ANALYSE/ROMAFOT</TT>
        <FONT SIZE="-1"><TT>frame [cat_tab] [int_tab] [sigma,sat]</TT></FONT>

<P>
This command is the most interactive part in the reduction procedure. 
   Because of its flexibility, its use may not seem straightforward. 
   Therefore, after starting up the command, the user is advised to press 
   the key ``H'': it will display the help information the screen. 
   For the sake of clarity only those commands which are useful 
   at this stage will be discussed below; other commands of the 
   <TT>ANALYSE/ROMAFOT</TT> will be discussed later.

<P>
After having received the appropriate input from the MIDAS command 
   line, the command waits for a command input. Following the present 
   example, the user should type ``D'' and a number. The command then
   asks for a number, say <I>n</I>, and will read the data for the 
<!-- MATH: $n^{\rm th}$ -->
<IMG
 WIDTH="60" HEIGHT="58" ALIGN="BOTTOM" BORDER="0"
 SRC="img208.gif"
 ALT="$n^{\rm th}$">
group of components stored in the intermediate table. 
   <TT>ANALYSE/ROMAFOT</TT> will display the data profiles and the fit 
   superimposed on the upper part of the image display. On the lower 
   part of the screen, three images are shown: the subframe containing 
   the real data, the subframe containing the fit and the difference 
   of the two, respectively.

<P>
The user can squeeze the interval over which the 256 colours are 
   distributed through the command ``W'' or vary the minimum of such 
   an interval with the command ``U''. In order to have a better check of 
   the correspondence between the data and the fit, the command ``X'' 
   displays isophotes at three different levels. The key ``Y'' has the 
   same function  but starts at a level given by the user (typical 
   numbers are 0.01 to 0.001).
   Another command useful for display is ``6'' which allows the smoothing
   of the subframe containing the real data. This smoothing is performed
   via a 
<!-- MATH: $3 \times 3$ -->
<IMG
 WIDTH="9" HEIGHT="35" ALIGN="MIDDLE" BORDER="0"
 SRC="img209.gif"
 ALT="$3 \times 3$">
gaussian convolution mask on the array stored in
   memory and does not affect the original array.

<P>
By means of the displayed information one can decide if the fit is 
   adequate or for example systematically wrong (for instance, all the 
   images have overestimated <IMG
 WIDTH="44" HEIGHT="54" ALIGN="BOTTOM" BORDER="0"
 SRC="img210.gif"
 ALT="$\sigma$">'s or heights). In the latter case
   <TT>FIT/ROMAFOT</TT> can be run with different parameters. 
   The procedure continues with ``D'', <I>n</I>+1, <I>n</I>+2, ...... etc.

<P>
A mean of all fits obtained will finally give the <IMG
 WIDTH="44" HEIGHT="54" ALIGN="BOTTOM" BORDER="0"
 SRC="img211.gif"
 ALT="$\sigma$">
of the PSF.
   Since <IMG
 WIDTH="44" HEIGHT="72" ALIGN="MIDDLE" BORDER="0"
 SRC="img212.gif"
 ALT="$\beta$">
had been already fixed, the PSF is now determined.

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