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%
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\providecommand{\TheTitle}{MIRA Manual - v. 2.3} 
\title{MIRA Manual - v. 2.3}
\author{Helmut Wiesemeyer}


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% !!! IMAGES START HERE !!!



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\begin{lrbox}{\savepar}
   \begin{minipage}[b]{\textwidth}{\bf Tip:} If you search with FIND in a large data archive, the search procedure
becomes slow, since it has to open each individual fits file. Note that FIND
is {\it not} a prerequesite for MIRA command SCAN (see below). You can also
accelerate the search by using at least one of the options /BACKEND, /OBSERVED 
or /SCAN (SCAN will be fastest). \end{minipage}\end{lrbox}%

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\begin{lrbox}{\savepar}
   \begin{minipage}[b]{\textwidth}{\bf Note:} It may happen that your index list contains observations from 
different days, but with the same scan number. By default, MIRA loads the 
last observation found. If you want to load another observation, you have to 
use option \verb+/OBSERVED+ of command \verb+FIND+.\end{minipage}\end{lrbox}%


\begin{lrbox}{\savepar}
   \begin{minipage}[b]{\textwidth}{\bf Tip:} Occasionally, spikes appear in the raw data. If they are stronger 
than the total power level, they can be removed from the raw data with MIRA's 
command DESPIKE. If they are comparable to the total power level, you should 
first calibrate the pointing, then despike, and then solve the pointing fit.\end{minipage}\end{lrbox}%


\begin{lrbox}{\savepar}
   \begin{minipage}[b]{\textwidth}{\bf Tip:} By default, MIRA's pointing procedure halts for a while after the 
subscan plots, and then displays the results of the coadded azimuth respectively
elevation subscans. This is for online data processing. For offline data 
processing, you may want to have a close look at the subscans. In that case, 
please enter {\bf LET doPause yes}.\end{minipage}\end{lrbox}%

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\begin{lrbox}{\savepar}
   \begin{minipage}[b]{\textwidth}{\bf Tip:} For large OTF maps, or HERA OTF maps, the amount of data shown makes
it impossible to show fine features in an appropriate way. In that case, the 
command \verb+VIEW /ZOOM+ allows the user to show a subset of the data: it calls
the interactive cursor, which is used to define two diagonally opposite corners
with two single mouse clicks). The plot is then re-displayed, with new ordinate
and abscissa scales. For HERA data, this option works for a single pixel only
(command syntax for pixel \verb+ipix+: \verb+VIEW /PIXEL ipix /ZOOM+).\end{minipage}\end{lrbox}%


\begin{lrbox}{\savepar}
   \begin{minipage}[b]{\textwidth}{\bf Tip:} For OTF maps observed with frequency switching, the amount of data
may become large for short switch cycles, and the calibration may be painfully 
slow. It can be accelerated by averaging dumps before calibration. Please use
\verb+SCAN /COMPRESS dumpTime+ (if the argument \verb+dumpTime+ is not an 
integer multiple of the uncompressed dump time, the compression factor is 
rounded to the next integer).\end{minipage}\end{lrbox}%


\begin{lrbox}{\savepar}
   \begin{minipage}[b]{\textwidth}{\bf Tip:} If there are no (or not enough) data from the reference position,
it is possible to use the data from the OTF subscans themselves to get a 
reference spectrum (syntax: \verb+ CAL all /GAINS /TCAL /OFF /MASK n1 n2 [n3 n4 ...]\+
where n1 and n2 respectively n3 and n4 etc. are the first and last OTF dumps on
the source). This works only if the OTF map is large enough to contain
emission-free positions.  For weak sources, one has to work iteratively.\end{minipage}\end{lrbox}%

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$-$%
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