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

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<H2><A NAME="SECTION003252000000000000000">
General instrumental information</A>
</H2>
The two principal classes of information needed about photometric
instruments concern filters and detectors.
We need two kinds of information for filters and detectors:
physical information about the instrument itself, and logical information
about the way it is represented in data files -
for example, the codes used to identify filter positions.

<P>
In addition, it is useful to know the condition of the
telescope optics: clean optics give not only better signal/noise ratio than
dirty ones, but also more stable zero-points from night to night.
Sometimes it is possible to have the optics cleaned before a critical observing
run; observers should consider this possibility.

<P>
Some, but by no means all, of the required information is available in the ESO
Archive - mostly in the archive log files [<A
 HREF="node649.html#E92">5</A>].
This can be stripped out and used when it is available; when it is not, the
observer will have to supply the information.

<P>
In addition to information about the instrument itself, the reduction program
needs to know the structure of the data in their table file (see
section&nbsp;<A HREF="node633.html#sect-data">I.6</A>, ``Observational data'').
Thus, you must make sure that information such as the number of filter-code
columns and the filter codes that correspond to particular passbands, which is
in the instrument-description table, agrees with the actual data tables.
Usually, this is determined by the program that converts raw data files to
table format.

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