<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 3.2 Final//EN"> <!--Converted with LaTeX2HTML 98.1p1 release (March 2nd, 1998) originally by Nikos Drakos (nikos@cbl.leeds.ac.uk), CBLU, University of Leeds * revised and updated by: Marcus Hennecke, Ross Moore, Herb Swan * with significant contributions from: Jens Lippmann, Marek Rouchal, Martin Wilck and others --> <HTML> <HEAD> <TITLE>Getting started</TITLE> <META NAME="description" CONTENT="Getting started"> <META NAME="keywords" CONTENT="vol2"> <META NAME="resource-type" CONTENT="document"> <META NAME="distribution" CONTENT="global"> <META HTTP-EQUIV="Content-Type" CONTENT="text/html; charset=iso-8859-1"> <LINK REL="STYLESHEET" HREF="vol2.css"> <LINK REL="next" HREF="node264.html"> <LINK REL="previous" HREF="node249.html"> <LINK REL="up" HREF="node248.html"> <LINK REL="next" HREF="node254.html"> </HEAD> <BODY > <!--Navigation Panel--> <A NAME="tex2html4596" HREF="node254.html"> <IMG WIDTH="37" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="next" SRC="icons.gif/next_motif.gif"></A> <A NAME="tex2html4593" HREF="node248.html"> <IMG WIDTH="26" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="up" SRC="icons.gif/up_motif.gif"></A> <A NAME="tex2html4587" HREF="node252.html"> <IMG WIDTH="63" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="previous" SRC="icons.gif/previous_motif.gif"></A> <A NAME="tex2html4595" HREF="node1.html"> <IMG WIDTH="65" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="contents" SRC="icons.gif/contents_motif.gif"></A> <BR> <B> Next:</B> <A NAME="tex2html4597" HREF="node254.html">Star tables</A> <B> Up:</B> <A NAME="tex2html4594" HREF="node248.html">PEPSYS general photometry package</A> <B> Previous:</B> <A NAME="tex2html4588" HREF="node252.html">What to do with</A> <BR> <BR> <!--End of Navigation Panel--> <H1><A NAME="SECTION001820000000000000000"> Getting started</A> </H1> <P> The first step is to gather the information that will be needed to plan a program and to reduce the data. Information that is more or less permanent is stored in several MIDAS table files: <P> <UL> <P> <LI>Star tables: These give names and positions of stars to be used for calibrations, as well as program stars. Common supplementary information, such as spectral types, may be included. Standard-star tables are provided for some popular systems, but you will have to compile your own table of program stars. <P> <LI>Observatory table: This table contains the positions of various telescopes, together with essential information such as apertures, and subsidiary information. <P> <LI>Horizon table: This table describes the apparent horizon as seen from a particular telescope. <P> </UL> <P> All of the above information, except for program-star tables, should already be available to you. Only if you are the first user of PEPSYS at an observatory will you need to construct the Observatory and Horizon tables yourself. They are described in the Appendix; see also section <A HREF="node302.html#installtbl">13.6.1</A> below. The Observatory file is very simple, and data for the Horizon file for a telescope can be collected in a few hours (the command <TT>MAKE/HORFORM</TT> will help you compile the horizon data). Program-star tables are described below, along with the <TT>MAKE/STARTABLE</TT> command provided to produce them. <P> In addition, you will need information about the instrument. As instruments tend to evolve with time, you will probably need to put this information together for each observing run separately. The <TT>MAKE/PHOTOMETER</TT> command will ask you questions, and make a new file from your answers; it can also show you the contents of an existing file. If an instrument is fairly stable, and a previous instrument-configuration file is available, you may be able to just edit the old file, using the <TT>EDIT/TABLE</TT> command. <P> Some of the instrumental information may not be available at the time you plan your observing run. You can give ``don't know'' responses to questions about such things, or leave items blank if you have no information. However, for the sake of accuracy, you should try to obtain as much of the missing information as you can before reducing the observations. <P> <BR><HR> <!--Table of Child-Links--> <A NAME="CHILD_LINKS"> </A> <UL> <LI><A NAME="tex2html4598" HREF="node254.html">Star tables</A> <UL> <LI><A NAME="tex2html4599" HREF="node255.html">ASCII source files</A> <LI><A NAME="tex2html4600" HREF="node256.html">Format files</A> <LI><A NAME="tex2html4601" HREF="node257.html">Manual entry of data</A> <LI><A NAME="tex2html4602" HREF="node258.html">Multiple star files</A> <LI><A NAME="tex2html4603" HREF="node259.html">Standard-star files</A> </UL> <LI><A NAME="tex2html4604" HREF="node260.html">Observatory table</A> <LI><A NAME="tex2html4605" HREF="node261.html">Horizon tables</A> <LI><A NAME="tex2html4606" HREF="node262.html">Instrument file</A> <LI><A NAME="tex2html4607" HREF="node263.html">General advice about table files</A> </UL> <!--End of Table of Child-Links--> <HR> <!--Navigation Panel--> <A NAME="tex2html4596" HREF="node254.html"> <IMG WIDTH="37" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="next" SRC="icons.gif/next_motif.gif"></A> <A NAME="tex2html4593" HREF="node248.html"> <IMG WIDTH="26" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="up" SRC="icons.gif/up_motif.gif"></A> <A NAME="tex2html4587" HREF="node252.html"> <IMG WIDTH="63" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="previous" SRC="icons.gif/previous_motif.gif"></A> <A NAME="tex2html4595" HREF="node1.html"> <IMG WIDTH="65" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="contents" SRC="icons.gif/contents_motif.gif"></A> <BR> <B> Next:</B> <A NAME="tex2html4597" HREF="node254.html">Star tables</A> <B> Up:</B> <A NAME="tex2html4594" HREF="node248.html">PEPSYS general photometry package</A> <B> Previous:</B> <A NAME="tex2html4588" HREF="node252.html">What to do with</A> <!--End of Navigation Panel--> <ADDRESS> <I>Petra Nass</I> <BR><I>1999-06-15</I> </ADDRESS> </BODY> </HTML>
