\begin{table*}%T3
%\centering
\par
\caption{The 
equivalent width of SiO~bands (unit is \AA). 
The date is that of either ISAAC or ISO/SWS observations in $ddmmyy$
format, which is different from the observing date of the magnitudes.
Column four
($\phi _{\rm{K}}$) lists
the pulsation phase during the SiO observations,
which is estimated from infrared $K$-band light curve
\citep{Whitelock03}, where 0.0 and 1.0
are the maxima. Uncertainty 
should be about~0.1.
The optical phase ($\phi_{\rm opt}$) is estimated for the ISO sample,
based on the AAVSO light curve.
The optical phase is usually about 0.1--0.2 of a cycle ahead of the infrared phase.
Photometric magnitudes are taken from \citet{Trams99b} 
for the LMC~sample,
and 2MASS for the Galactic sample.
Luminosity class and 
spectral types  for Galactic
stars are taken from 
Simbad.
}
\label{table-oxygen}
$$
\begin{tabular}{ll cll r@{.}l | 
r@{.}l r@{.}l r@{.}l r@{.}l r@{.}l r@{.}l r@{.}l llll}\hline\hline 
Name              &  Sp. type & Date & $\phi _{\rm{K}}$ &
$\phi_{\rm opt}$ & \multicolumn{2}{c}{\Ws} & 
 \multicolumn{2}{c}{$H$}  &    \multicolumn{2}{c}{$K$}  
\\
\hline
%\it LMC sample
\multicolumn{6}{l}{{\it LMC sample}} &
\\
IRAS 04553$-$6825 & M7.5, supergiant      &12-12-01&      &&$-$2&2  &    7&96 &   6&98 \\
IRAS 05042$-$6720 & M1I, M4Ia, supergiant &12-12-01&      &&$-$9&7  &    7&20 &   6&89 \\
IRAS 05558$-$7000 &                       &13-12-01& 0.87 &&$-$7&3  &   10&10 &   8&90 \\
\hline
\multicolumn{6}{l}{{\it LMC sample (Poorer quality in \Ws)}}&\\
IRAS 04407$-$7000 &                       &14-12-01& 0.82 &&$-$24&2  &    8&92 &   8&18 \\
IRAS 05128$-$6455 &                       &13-12-01&      &&   6&0   &   12&10 &  10&55 \\
IRAS 05148$-$6730 & M1I, supergiant       &15-12-01&      &&   17&5 \\
\hline
\multicolumn{6}{l}{{\it Galactic sample from ISO}}&\\
R Aql        & Mira                &19-03-97&&0.25  &   13&4       &$-$0&355 $\pm$ 0.218 &$-$0&826 $\pm$ 0.230 \\
VY CMa       & M5Ia,e              &21-11-97&&      &    3&6       &   1&576 $\pm$ 0.210 &    0&291 $\pm$ 0.236 \\
g Her        & M6III, SR           &23-08-96&&      &   39&4       &$-$1&850 $\pm$ 0.138 &$-$2&134 $\pm$ 0.158 \\
$\alpha$ Ori & M1Iab, SR           &08-10-97&&      &   49&3       &$-$4&007 $\pm$ 0.162 &$-$4&378 $\pm$ 0.186 \\
$\rho$ Per   & M4II, SR            &05-03-98&&      &   37&0       &$-$1&675 $\pm$ 0.158 &$-$1&904 $\pm$ 0.152 \\
KK Per       & M2Iab-Ib            &03-02-98&&      &   36&4       &   2&138 $\pm$ 0.166 &    1&683 $\pm$ 0.206 \\
VX Sgr       & M5/M6III, M4eIa, SR &13-10-96&&      &$-$1&3       &   0&550 $\pm$ 0.304 & $-$0&122 $\pm$ 0.362 \\
SW Vir       & M7III, SR           &20-07-96&&      &   37&3       &$-$1&606 $\pm$ 0.260 & $-$2&003 $\pm$ 0.336 \\
\hline
\end{tabular}
$$
\end{table*}