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

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<H3><A NAME="SECTION001857500000000000000">
Table file output</A>
</H3>
The individual data, reduced as described above, are put into a simple output
table file named ``results.tbl''.
Its columns give both MJD and heliocentric Julian Date (minus 2400000); the
name of the object; the band; and the corresponding standard magnitude.
This makes the results of the reductions available for further processing with
MIDAS utilities.

<P>
For example, although the table entries are written in the same order they are
printed in the logfile (star by star, so that the necessary color data are
adjacent), they can be rearranged into chronological order, or by passband,
with the <TT>SORT/TABLE</TT> command.
Columns can be extracted to a new table, using <TT>PROJECT/TABLE</TT>.
You could interpolate the values of a comparison star to every time in the
table by using <TT>FIT/TABLE</TT> or <TT>REGRESS/TABLE</TT>,
and then use <TT>COMPUTE/TABLE</TT> to
subtract these from the values for a variable star to produce
differential photometry.

<P>
Additional columns could be transferred from the original data to the new
table, using <TT>PROJECT/TABLE</TT> and <TT>JOIN/TABLE</TT> or <TT>MERGE/TABLE</TT>,
so that correlations and effects not looked for by the reduction program can be
detected.
In general, because the PEPSYS package makes heavy use of table files, the
user should try to become familiar with the utilities MIDAS provides to
deal with them.

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