\begin{table}%t1
\caption{Protostar  photometry.}\label{t.photo}
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\par
%\centering
\par
\begin{tabular}{l cc cccc c cc cc}
\hline\hline\noalign{\smallskip}
HOPS & RA (J2000) & Dec  (J2000) & [3.6] & [4.5] & [5.8] & [8.0] & [24] & [70] & [160] & [350] & [870] \\
Source & (h m s) & ($^\circ$ \arcmin\ \arcsec) & (Jy) & (Jy) & (Jy) & (Jy) & (Jy) & (Jy) & (Jy) & (Jy) & (Jy) \\  
\hline
165\dotfill & 5 36 23.54 & $-$6 46 14.6 & 0.014 & 0.052 & 0.11 & 0.13 & 0.64 & 1.1 & $<$0.3 & $<$3 & ... \\
166\dotfill & 5 36 25.13 & $-$6 44 41.8 & 0.66 & 0.83 & 0.97 & 1.17 & 4.65 & 10.9 & 11.1 & 4.6 & 0.33 \\
168\dotfill & 5 36 18.93 & $-$6 45 22.7 & 0.0077 & 0.030 & 0.041 & 0.038 & 3.66 & 87.3 & 87.7 & 24 & 0.94 \\
203\dotfill & 5 36 22.84 & $-$6 46 06.2 & ... & ... & ... & 0.0091 & 0.54 & 26.6 & 75.7 & 28 & 1.2 \\
\hline
\end{tabular}
\tablefoot{Aperture radii are 3\arcsec\ from 1.2 to 2.2 $\mu$m (not shown), 2\arcsec\ from 3.6 to 8.0 $\mu$m, 5\arcsec\ at 24 $\mu$m, and 16\arcsec\ at 70 $\mu$m and longward.  Systematic uncertainties are 3\% from 1.2 to 2.2 $\mu$m, 5\% from 3.6 to 24 $\mu$m, 10\% at 70 $\mu$m, 20\% at 160 $\mu$m, 40\% at 350 $\mu$m, and 20\% at 870 $\mu$m.}
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\end{table}