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+<H2><A NAME="SECTION0004113000000000000000">SLA_MAP - Mean to Apparent</A>
+<A NAME="xref_SLA_MAP">&#160;</A><A NAME="SLA_MAP">&#160;</A>
+</H2>
+ <DL>
+<DT><STRONG>ACTION:</STRONG>
+<DD>Transform star <IMG WIDTH="42" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img3.gif"
+ ALT="$[\,\alpha,\delta\,]$"> from mean place to geocentric apparent.
+The reference frames and timescales used are post IAU&nbsp;1976.
+<P> <DT><STRONG>CALL:</STRONG>
+<DD><TT>CALL sla_MAP (RM, DM, PR, PD, PX, RV, EQ, DATE, RA, DA)</TT>
+<P> </DL>
+<P> <DL>
+<DT><STRONG>GIVEN:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>RM,DM</EM></TD>
+<TH ALIGN="LEFT"><B>D</B></TH>
+<TD ALIGN="LEFT" NOWRAP>mean <IMG WIDTH="42" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img3.gif"
+ ALT="$[\,\alpha,\delta\,]$"> (radians)</TD>
+</TR>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>PR,PD</EM></TD>
+<TD ALIGN="LEFT"><B>D</B></TD>
+<TD ALIGN="LEFT" NOWRAP>proper motions: <IMG WIDTH="42" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img3.gif"
+ ALT="$[\,\alpha,\delta\,]$"> changes per Julian year</TD>
+</TR>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>PX</EM></TD>
+<TD ALIGN="LEFT"><B>D</B></TD>
+<TD ALIGN="LEFT" NOWRAP>parallax (arcsec)</TD>
+</TR>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>RV</EM></TD>
+<TD ALIGN="LEFT"><B>D</B></TD>
+<TD ALIGN="LEFT" NOWRAP>radial velocity (km&nbsp;s<SUP>-1</SUP>, +ve if receding)</TD>
+</TR>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>EQ</EM></TD>
+<TD ALIGN="LEFT"><B>D</B></TD>
+<TD ALIGN="LEFT" NOWRAP>epoch and equinox of star data (Julian)</TD>
+</TR>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>DATE</EM></TD>
+<TD ALIGN="LEFT"><B>D</B></TD>
+<TD ALIGN="LEFT" NOWRAP>TDB for apparent place (JD-2400000.5)</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>RETURNED:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>RA,DA</EM></TD>
+<TH ALIGN="LEFT"><B>D</B></TH>
+<TD ALIGN="LEFT" NOWRAP>apparent <IMG WIDTH="42" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img3.gif"
+ ALT="$[\,\alpha,\delta\,]$"> (radians)</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>NOTES:</STRONG>
+<DD><DL COMPACT>
+<DT>1.
+<DD>EQ is the Julian epoch specifying both the reference
+frame and the epoch of the position - usually 2000.
+For positions where the epoch and equinox are
+ different, use the routine sla_PM to apply proper
+ motion corrections before using this routine.
+ <DT>2.
+<DD>The distinction between the required TDB and TT is
+ always negligible. Moreover, for all but the most
+ critical applications UTC is adequate.
+ <DT>3.
+<DD>The <IMG WIDTH="13" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
+ SRC="img24.gif"
+ ALT="$\alpha$"> proper motions are <IMG WIDTH="13" HEIGHT="13" ALIGN="BOTTOM" BORDER="0"
+ SRC="img115.gif"
+ ALT="$\dot{\alpha}$"> rather than
+ <IMG WIDTH="48" HEIGHT="13" ALIGN="BOTTOM" BORDER="0"
+ SRC="img116.gif"
+ ALT="$\dot{\alpha}\cos\delta$">, and are per year rather than per century.
+ <DT>4.
+<DD>This routine may be wasteful for some applications
+ because it recomputes the Earth position/velocity and
+ the precession/nutation matrix each time, and because
+ it allows for parallax and proper motion. Where
+ multiple transformations are to be carried out for one
+ epoch, a faster method is to call the sla_MAPPA routine
+ once and then either the sla_MAPQK routine (which includes
+ parallax and proper motion) or sla_MAPQKZ (which assumes
+ zero parallax and FK5 proper motion).
+ </DL></DL>
+<P> <DL>
+<DT><STRONG>REFERENCES:</STRONG>
+<DD><DL COMPACT>
+<DT>1.
+<DD>1984 <I>Astronomical Almanac</I>, pp B39-B41.
+<DT>2.
+<DD>Lederle &amp; Schwan, 1984. <I>Astr.Astrophys.</I> <B>134</B>, 1-6.
+</DL></DL>
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+<ADDRESS>
+<I>SLALIB --- Positional Astronomy Library<BR>Starlink User Note 67<BR>P. T. Wallace<BR>12 October 1999<BR>E-mail:ptw@star.rl.ac.uk</I>
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