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<H2><A NAME="SECTION003223000000000000000">
Standard values</A>
</H2>
The above information suffices for program stars.
Standard-star files, however, must also have the standard photometric values
(in place of the rough MAG column).
The column label should be the usual name of the magnitude or index in the
column, e.g., V or U-B or c1; see Table <A HREF="node565.html#tbl:band-list">I.2</A>.
The data themselves are Real*4 numbers.
Magnitudes are displayed in F5.2 or F6.3 format, which leaves room for two
digits before the decimal point.
Color and other indices are displayed in f6.3 format; this
displays leading + signs.
<P>
<BR>
<DIV ALIGN="CENTER"><A NAME="30067"> </A>
<TABLE>
<CAPTION><STRONG>Table:</STRONG>
Standard column labels for photometric indices</CAPTION>
<TR><TD>
<DIV ALIGN="CENTER">
<TABLE CELLPADDING=3 BORDER="1" ALIGN="CENTER">
<TR><TD ALIGN="LEFT">System</TD>
<TD ALIGN="CENTER">Index</TD>
<TD ALIGN="CENTER">Col. label</TD>
</TR>
<TR><TD ALIGN="LEFT">UBVRI</TD>
<TD ALIGN="CENTER">V</TD>
<TD ALIGN="CENTER"><TT> V</TT></TD>
</TR>
<TR><TD ALIGN="LEFT">UBVRI</TD>
<TD ALIGN="CENTER">B-V</TD>
<TD ALIGN="CENTER"><TT> B-V</TT></TD>
</TR>
<TR><TD ALIGN="LEFT">UBVRI</TD>
<TD ALIGN="CENTER">U-B</TD>
<TD ALIGN="CENTER"><TT> U-B</TT></TD>
</TR>
<TR><TD ALIGN="LEFT">UBVRI</TD>
<TD ALIGN="CENTER">V-R</TD>
<TD ALIGN="CENTER"><TT> V-R</TT></TD>
</TR>
<TR><TD ALIGN="LEFT">UBVRI</TD>
<TD ALIGN="CENTER">R-I</TD>
<TD ALIGN="CENTER"><TT> R-I</TT></TD>
</TR>
<TR><TD ALIGN="LEFT">UBVRI</TD>
<TD ALIGN="CENTER">V-I</TD>
<TD ALIGN="CENTER"><TT> V-I</TT></TD>
</TR>
<TR><TD ALIGN="LEFT">uvby</TD>
<TD ALIGN="CENTER">b-y</TD>
<TD ALIGN="CENTER"><TT> b-y </TT></TD>
</TR>
<TR><TD ALIGN="LEFT">uvby</TD>
<TD ALIGN="CENTER">u-v</TD>
<TD ALIGN="CENTER"><TT> u-v </TT></TD>
</TR>
<TR><TD ALIGN="LEFT">uvby</TD>
<TD ALIGN="CENTER"><IMG
WIDTH="33" HEIGHT="39" ALIGN="MIDDLE" BORDER="0"
SRC="img1139.gif"
ALT="${\rm m}_1$"></TD>
<TD ALIGN="CENTER"><TT> m1 </TT></TD>
</TR>
<TR><TD ALIGN="LEFT">uvby</TD>
<TD ALIGN="CENTER"><IMG
WIDTH="25" HEIGHT="39" ALIGN="MIDDLE" BORDER="0"
SRC="img1140.gif"
ALT="${\rm c}_1$"></TD>
<TD ALIGN="CENTER"><TT> c1 </TT></TD>
</TR>
<TR><TD ALIGN="LEFT">H-beta</TD>
<TD ALIGN="CENTER"><IMG
WIDTH="18" HEIGHT="41" ALIGN="MIDDLE" BORDER="0"
SRC="img1141.gif"
ALT="${\beta}$"></TD>
<TD ALIGN="CENTER"><TT> beta </TT></TD>
</TR>
</TABLE></DIV>
<A NAME="tbl:band-list"> </A></TD></TR>
</TABLE>
</DIV>
<BR>
<P>
In addition, standard-star files should specify the system they employ,
and the source of the standard values.
The system should be placed in a
character descriptor called <B>SYSTEM</B>.
This may be up to 32 characters long, because of the need to distinguish
between such alternatives as
<TT>'JOHNSON-MORGAN UBV'</TT>,
<TT>'LANDOLT UBV'</TT>,
and
<TT>'KRON-COUSINS UBVRI'</TT>,
<P>
Catalog stars may have not only columns specifying values in the system of
observation, but also other systems.
However, data from other systems,
except for V magnitudes, will be ignored.
<P>
There is a potential problem in the use of indices like U-B as column labels
that users should be aware of.
MIDAS table files do not distinguish between upper and lower case in column
labels.
Thus, while it is possible to use
<TT>'u-b'</TT>
as a column label for the uvby system, it cannot be distinguished from
<TT>'U-B'</TT>
by programs or MIDAS procedures that read these files.
However, the string may be entered in the proper case when the label is
created, and will appear correctly on plots, table listings, etc.
<P>
Furthermore, because the provision for column arithmetic was built into the
table system before the need for color index-names as column labels was
apparent, it will be necessary to use the double-quote mark (<TT>"</TT>)
around such indices when referring to them as column labels.
For example, in a MIDAS command line, the B-V column must be referred to as
<TT>:"B-V"</TT>.
Although this is inconvenient, it does allow such names to appear on plots,
etc.
The alternative (which will be automatically applied by MIDAS in the absence of
the double-quote marks) is to convert the minus sign to an underscore, so that
we would have B_V instead of B-V.
This appears to be even more inconvenient for photometrists than to put up with
the quotes.
<P>
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<ADDRESS>
<I>Petra Nass</I>
<BR><I>1999-06-15</I>
</ADDRESS>
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