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\begin{document}
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\begin{planotable}{lllllll}
\tablenum{17}
\tablewidth{6.0in}
\tablecaption{BOLOMETRIC CORRECTIONS}
\tablehead{
\colhead{}&
\colhead{Median}&
\colhead{Mean, Sigma}&
\colhead{Min}&\colhead{Max}
}
\startdata
$L_{Bol}/L_{2500\AA}$&5.6&6.3\er3.1&2.4 &16.7\\
$L_{Bol}/L_{B}$& 10.7&11.8\er4.3     &5.5 &24.7\\
$L_{Bol}/L_{V}$&13.2&14.2\er5.1     &7.1 &29.3\\
$L_{Bol}/L_{1.5\mu m}$&24.8 &25.5\er8.4&9.3&41.9\\
\\
$L_{UVOIR}/L_{2500\AA}$&3.5 & 4.2\er2.6 & 1.2 & 14.0\\
$L_{UVOIR}/L_{B}$&6.8 &7.6\er3.5 & 4.1 & 22.4\\
$L_{UVOIR}/L_{V}$&8.1 & 9.2\er3.9& 4.9 & 22.7\\
$L_{UVOIR}/L_{1.5\mu m}$&15.5 &16.1\er5.3 & 8.3 & 28.5\\
\\
$L_{Ion}/L_{Bol}$ & 0.32 & 0.32\er0.13   & 0.07 & 0.66\\
$N_{Ion}R/L_{Bol}$ &0.12 & 0.11\er0.04  & 0.02 & 0.18\\
$L_{Ion}/N_{Ion}R$ &2.8 & 3.0\er0.8    & 1.7 & 4.8\\
\tablecomments{ Bolometric correction factors
for UV, visible and infrared monochromatic luminosities.
Monochromatic luminosities are defined to be the value of
$\nu L(\nu)$ in the rest frame. Mean and standard deviation
are given, followed by the minimum and maximum values
found in the sample. Errors in the determination of
individual energy distributions have been ignored for
the purposes of this table. Also listed are estimates
of the ionizing flux discussed in the text.}
\end{planotable}

\end{document}

