\documentstyle[aaspp]{article}
%\documentstyle{article}\def\nodata{---}\def\tableline{\hline}
\begin{document}
\begin{tabular}{lllllll}
\hline
\multicolumn{1}{c}{HR \#}    &
\multicolumn{1}{c}{NAME $^a$}   &
\multicolumn{1}{c}{$m_H^b$} &
\multicolumn{1}{c}{ST}   &
\multicolumn{1}{c}{Class}  &
\multicolumn{1}{c}{RV (km s$^{-1}$) $^c$}     &
\multicolumn{1}{c}{vsini (km s$^{-1}$) }  \\\hline\hline
%
1903     & *46 $\epsilon$ Ori & 2.4    & B0         & Ia         & 26SB     & 87        \\  
1203     & 44 $\zeta$ Per    & 3.4    & B1         & Ib         & 20SB     & 59        \\  
2827     & 31 $\eta$ CMa     & 2.5    & B5         & Ia         & 41V      & 45        \\  
1713     & *19 $\beta$ Ori    & 0.1    & B8         & Ia         & 21SB     & 33        \\  
3975     & *30 $\eta$ Leo     & 3.3    & A0         & Ib         & 3V       & 20        \\  
7924     & *50 $\alpha$ Cyg   & 1.0    & A2         & Ia         & -5SBO    & 21        \\  
1865     & 11 $\alpha$ Lep   & 2.0    & F0         & Ib         & 24       & 13        \\  
1017     & *33 $\alpha$ Per   & 0.9    & F5         & Ib         & -2V      & 18        \\ 
7796     & *37 $\gamma$ Cyg   & 1.1    & F8         & Ib         & -8V      & 20        \\ 
8232     & *22 $\beta$ Aqr    & 1.5    & G0         & Ib         & 7V?      & 18        \\ 
7479     & 5 $\alpha$ Sge    & 2.4    & G1         & II         & 2V?      & 0         \\ 
7063     & $\beta$ Sct       & 2.2    & G4         & IIa        & -22SB10  & 10        \\ 
8752     & *-                & 3.6   &  G4v        & $>I^d$      & -58V?    & 35        \\ 
7314     & *21 $\theta$ Lyr   & 2.1    & K0         & +II        & -31V     & $<$19     \\ 
6713     & 93 Her            & 2.4    & K0.5       & IIb        & -24      & $<$17     \\ 
8465     & *21 $\zeta$ Cep    & 1.1    & K1.5       & Ib         & -18SB    & $<$17     \\ 
6498     & 49 $\sigma$ Oph   & 1.9    & K2         & II         & -27      & $<$19     \\  
603      & 57 $\gamma^1$ And & -0.5   & K3         & -IIb       & -12SB    & $<$17     \\ 
8089     & *63 Cyg            & 1.5    & K4         & Ib-IIa     & -26V     & --        \\    
8079     & *62 $\xi$ Cyg      & 0.5    & K4.5       & Ib-II      & -20SB    & $<$17     \\ 
2061     & 58 $\alpha$ Ori   & -2.?   & M1-2       & Ia-Iab     & 21SB     & --        \\ 
1155  & *--                & 0.5    & M2         & +IIab      & -3V      & --        \\ 
921      & 25 $\rho$ Per     & -1.7   & M4         & II         & 28       & --        \\ 
7009  & *--                & 0.6    & M4.5-M5    & +II        & -19      & --        \\ 
6406  & *64 $\alpha^1$ Her & -2.4   & M5         & Ib-II      & -33V     & 21        \\\hline
%
\multicolumn{7}{l}{\footnotesize $^a$
``*'' indicates that the object also appears in the K--band atlas of WH97.} \\
\multicolumn{7}{l}{\footnotesize $^b$
H--band magnitudes estimated from V--band magnitude from the Bright Star} \\
\multicolumn{7}{l}{\footnotesize 
Catalogue, spectral type, and intrinsic colors (Koornneef, 1983).} \\
\multicolumn{7}{l}{\footnotesize $^c$
``V'' and ``V?'' indicate variable or suspected variable radial velocity respectively.} \\
\multicolumn{7}{l}{\footnotesize 
``SB1'' and ``SB2'' indicate single-- and double--lined spectroscopic binaries respectively.} \\
\multicolumn{7}{l}{\footnotesize 
``O'' indicates that orbital data is available in the Bright Star Catalogue.}\\
\multicolumn{7}{l}{\footnotesize $^d$
Previously classified as G0Ia, but it is intrinsically brighter.  } \\
\multicolumn{7}{l}{\footnotesize $^e$
Taken from Jaschek, Jaschek, and Condi (1964).} \\
\multicolumn{7}{l}{\footnotesize $^f$
Taken from Henry, Kirkpatrick, and Simons (1994).} \\
\end{tabular}
\clearpage
%\end{document}
%\end
%\documentstyle[12pt,aaspp]{article}
%\begin{document}
\begin{tabular}{lllllll}
\hline
\multicolumn{1}{c}{HR \#}    &
\multicolumn{1}{c}{NAME $^a$}   &
\multicolumn{1}{c}{$m_H ^b$} &
\multicolumn{1}{c}{ST}   &
\multicolumn{1}{c}{Class}  &
\multicolumn{1}{c}{RV (km s$^{-1}$) $^c$}     &
\multicolumn{1}{c}{vsini (km s$^{-1}$) }  \\\hline\hline
%
1899     & 44 $\iota$ Ori    & 3.5    & O9         & III        & 22SB2O   & 130       \\ 
1552     & 3 $\pi^4$ Ori     & 4.1    & B2+B2      & III        & 23SBO    &  40       \\ 
5291     & *11 $\alpha$ Dra   & 3.5    & A0         & III        & -13SBO   & 18        \\
403      & *37 $\delta$ Cas   & 2.3    & A5         & III-IV     & 7SB      & 113       \\ 
1412     & *78 $\theta^2$ Tau & 2.9    & A7         & III        & 40SB1O   & 78        \\ 
4031     & *36 $\zeta$ Leo    & 2.8    & F0         & III        & -16SB    & 84        \\ 
21       & * 11 $\beta$ Cas   & 1.6    & F2         & III--IV    & 12SB     & 70        \\ 
5017     & *20 CVn            & 3.9    & F3         & III        & 8V?      & 17        \\ 
2706     & 48 Gem            & 5.0    & F5         & III-IV     & 13V      & 74        \\ 
8905     & *68 $\upsilon$ Peg & 3.3    & F8         & III        & -11      & 79        \\ 
4883     & *31 Com            & 3.0    & G0         & III        & -1V?     & 77        \\ 
4716     & 5 CVn             & 2.8    & G6         & III        & -12SB    & $<$17     \\ 
7328     & 1 $\kappa$ Cyg    & 1.6    & G9         & III        & -29SB    & $<$17     \\ 
7949     & 53 $\epsilon$ Cyg & 0.2    & K0         & -III       & -11SB?   & $<$17     \\ 
8317     & *11 Cep            & 2.3    & K1         & III        & -37      & $<$17     \\ 
6299     & *27 $\kappa$ Oph   & 0.8    & K2         & III        & -56V     & $<$17     \\ 
165      & 31 $\delta$ And   & 0.5    & K3         & III        & -7SB1O   & $<$17     \\ 
6705     & *33 $\gamma$ Dra   & -1.2   & K5         & III        & -28      & $<$17     \\ 
152      & --                & 1.7    & K5-M0      & III        & -33V     & $<$17     \\ 
4517     & *3 $\nu$ Vir       & 0.3    & M1         & IIIab      & 51V?     & --        \\ 
6242     & --                & 0.4    & M4         & +III-IIIa  & -7V?     & --        \\ 
7886     & *--                & -0.6   & M6         & III        & -66V?    & --        \\\hline  
\end{tabular}
\clearpage
%\end{document}
%\end
%\documentstyle[12pt,aaspp]{article}
%\begin{document}
\begin{tabular}{lllllll}
\hline
\multicolumn{1}{c}{HR \#}    &
\multicolumn{1}{c}{NAME $^a$}   &
\multicolumn{1}{c}{$m_H ^b$} &
\multicolumn{1}{c}{ST}   &
\multicolumn{1}{c}{Class}  &
\multicolumn{1}{c}{RV (km s$^{1}$) $^c$}     &
\multicolumn{1}{c}{vsini (km s$^{1}$) }  \\\hline\hline
%
6588     & 85 $\iota$ Her    & 4.3    & B3         & IV         & -20SB1O  & 11        \\ 
4033     & *33 $\lambda$ UMa  & 3.3    & A2         & IV         & 18V      & 48        \\ 
1351     & 57 Tau            & 4.9    & F0         & IV         & 42SB1?   & 109       \\ 
5235     & 8 $\eta$ Boo      & 1.5    & G0         & IV         & 0SB1O    & 13        \\ 
5409     & 105 $\phi$ Vir    & 2.8    & G2         & IV         & -10SB    & 0         \\ 
6623     & 86 $\mu$ Her      & 1.4    & G5         & IV         & -16V     & 20        \\ 
995      & 59 Ari            & 3.9    & G6         & IV         & 0V       & --        \\ 
7602     & 60 $\beta$ Aql    & 1.7    & G8         & IV         & -40V     & $<$ 16    \\ 
7957     & *3 $\eta$ Cep      & 1.2    & K0         & IV         & -87      & $<$17     \\ 
5901     & 11 $\kappa$ CrB   & 2.5    & K1         & IVa        & -24      & $<$17     \\ 
6014     & --                & 3.6    & K1.5       & IV         & -4V      & --        \\\hline
2456     & *15 Mon            & 5.5    & O7         & V(e)       & 33SB     & 63        \\ 
5191     & *85 $\eta$ UMa$^e$     & 2.4    & B3         & V          & -11SB?   & 205       \\ 
3982     & *32 $\alpha$ Leo$^e$   & 1.6    & B7         & V          & 6SB      & 329       \\ 
7001     & * $\alpha$ Lyr     & 0.0    & A0         & V          & -14V     & 15        \\ 
2491     & *9 $\alpha$ CMa    & -1.5   & A1         & Vm         & -8SBO    & 13        \\ 
4534     & *94 $\beta$ Leo$^e$    & 2.0    & A3         & V          & 0V       & 121       \\ 
4357     & *68 $\delta$ Leo$^e$   & 2.3    & A4         & V          & -20V     & 181       \\ 
4931     & 78 UMa            & 4.1    & F2         & V          & -10V?    & 92        \\ 
1279     & --                & 5.1    & F3         & V          & 36SB1?   & 25        \\ 
2943     & *10 $\alpha$ CMi   & -0.6   & F5         & IV-V       & -3SBO    & 6         \\ 
1538     & 59 Eri$^e$            & 2.3    & F6         & V          & 35       & --        \\ 
4375     & *53 $\xi$ UMa      & 3.0    & G0         & V          & -16SB1O  & 1         \\ 
4983     & 43 $\beta$ Com    & 3.1    & F9.5       & V          & 6SB?     & 6         \\ 
483      & *--                & 3.7    & G1.5       & V          & 4V?      & 2         \\ 
4374     & 53 $\xi$ UMa      & 3.5    & G0         & V          & -16SB1O  & 3         \\ 
5072     & 70 Vir            & 3.6    & G4         & V          & 5V       & 1         \\ 
4496     & *61 UMa            & 3.8    & G8         & V          & -5V      & $<$17     \\ 
7462     & *61 $\sigma$ Dra   & 3.0    & K0         & V          & 27V      & $<$17     \\ 
1084     & *18 $\epsilon$ Eri & 1.6    & K2         & V          & 15V?     & $<$17     \\ 
8832     & *--                & 3.2    & K3         & V          & -18V     & --        \\ 
--       & GL570A            & 3.0    & K4         & V          & -        & -         \\ 
8085     & *61 Cyg            & 2.4    & K5         & V          & -64V     & $<$17     \\ 
8086     & 61 Cyg            & 3.1    & K7         & V          & -64V?    & =$<$25    \\ 
--       & GL338A            & 4.5    & M0         & V          & -        & -         \\ 
--       & GL526$^f$             & 4.5    & M1.5    & V          & -        & -         \\ 
--       & *GL411             & 3.6    & M2         & V          & -        & -         \\ 
--       & *GL725A            & 4.7    & M3         & V          & -        & -         \\\hline
\end{tabular}
\clearpage
%\end{document}
%\end
%\documentstyle[12pt,aaspp]{article}
%\begin{document}
\begin{tabular}{lllllll}
\hline
\multicolumn{1}{c}{HR \#}    &
\multicolumn{1}{c}{NAME}   &
\multicolumn{1}{c}{Vmag$^1$} &
\multicolumn{1}{c}{ST}   &
\multicolumn{1}{c}{Class}  &
\multicolumn{1}{c}{RADV$^2$}     &
\multicolumn{1}{c}{ROTV$^2$}  \\\hline\hline
%
2456     & 15 Mon            & 4.66   & O7         & V((f))     & 33SB     & 63        \\ 
5191     & 85 $\eta$ UMa     & 1.86   & B3         & V          & -11SB?   & 205       \\ 
3982     & 32 $\alpha$ Leo   & 1.35   & B7         & V          & 6SB      & 329       \\ 
2491     & 9 $\alpha$ CMa    & -1.4   & A1         & Vm         & -8SBO    & 13        \\ 
4534     & 94 $\beta$ Leo    & 2.14   & A3         & V          & 0V       & 121       \\ 
4357     & 68 $\delta$ Leo   & 2.56   & A4         & V          & -20V     & 181       \\ 
4931     & 78 UMa            & 4.93   & F2         & V          & -10V?    & 92        \\ 
1279     & --                & 6.01   & F3         & V          & 36SB1?   & 25        \\ 
2943     & 10 $\alpha$ CMi   & 0.38   & F5         & IV-V       & -3SBO    & 6         \\ 
1538     & 59 Eri            & 5.77   & F6         & V          & 35       & --        \\ 
4375     & 53 $\xi$ UMa      & 4.41   & G0         & V          & -16SB1O  & 1         \\ 
4983     & 43 $\beta$ Com    & 4.26   & F9.5       & V          & 6SB?     & 6         \\ 
483      & --                & 4.95   & G1.5       & V          & 4V?      & 2         \\ 
4374     & 53 $\xi$ UMa      & 4.87   & G0         & V          & -16SB1O  & 3         \\ 
5072     & 70 Vir            & 4.98   & G4         & V          & 5V       & 1         \\ 
4496     & 61 UMa            & 5.33   & G8         & V          & -5V      & $<$17     \\ 
7462     & 61 $\sigma$ Dra   & 4.68   & K0         & V          & 27V      & $<$17     \\ 
1084     & 18 $\epsilon$ Eri & 3.73   & K2         & V          & 15V?     & $<$17     \\ 
8832     & --                & 5.56   & K3         & V          & -18V     & --        \\ 
GL570A   & -                 & -      & -          & -          & -        & -         \\ 
8085     & 61 Cyg            & 5.21   & K5         & V          & -64V     & $<$17     \\ 
8086     & 61 Cyg            & 6.03   & K7         & V          & -64V?    & =$<$25    \\ 
GL338A   & -                 & -      & -          & -          & -        & -         \\ 
GL411    & -                 & -      & -          & -          & -        & -         \\ 
GL526    & -                 & -      & -          & -          & -        & -         \\ 
GL725A   & -                 & -      & -          & -          & -        & -         \\\hline
\end{tabular}
\clearpage
%\end{document}
%\end
\begin{tabular}{rlll}
\hline
\multicolumn{1}{c}{Spectral Type $^a$} &
\multicolumn{1}{c}{T$_{I-II}^b$}    &
\multicolumn{1}{c}{T$_{III}^{b,c}$}     &
\multicolumn{1}{c}{T$_{IV-V}^b$}    \\\hline
%
O6-O8--	 & \nodata  & 37000   &  38000   \\
O9--	 & 32500    & 32000   &  33200   \\
O9.5--	 & \nodata  & \nodata &  31450   \\
B0--	 & 26000    & 29000   &  29700   \\
B1--	 & 20700    & 24000   &  25600   \\
B2--	 & 17800    & 20300   &  22300   \\
B3--	 & 15600    & 17100   &  19000   \\
B4	 & 13900    & \nodata &  17200   \\
B5--	 & 13400    & 15000   &  15400   \\
B6	 & 12700    & 14100   &  14100   \\
B7--	 & 12000    & 13200   &  13000   \\
B8--	 & 11200    & 12400   &  11800   \\
B9--	 & 10500    & 11000   &  10700   \\
A0--	 &  9730    & 10100   &   9480   \\
A1--	 &  9230    &  9480   &  \nodata \\
A2	 &  9080    &  9000   &   8810   \\
A5--	 &  8510    &  8100   &   8160   \\
A7--	 & \nodata  &  7650   &   7930   \\
F0--	 &  7700    &  7150   &   7020   \\
F2--	 &  7170    &  6870   &   6750   \\
F5--	 &  6640    &  6470   &   6530   \\
F7--	 & \nodata  & \nodata &   6240   \\
F8--	 &  6100    &  6150   &  \nodata \\\hline 
%
\multicolumn{4}{l}{\footnotesize $^a$ 
``--'' denotes full sub--class in the revised MK system.  Other full} \\
\multicolumn{4}{l}{\footnotesize 
sub--classes for which temperatures are not available without interpolation} \\ 
\multicolumn{4}{l}{\footnotesize 
include B0.5, A3, A8, F3, F9, and G5.} \\
\multicolumn{4}{l}{\footnotesize $^b$ 
Data taken from Tokunaga, 1996, Astrophysical Quantities, in press.}\\
\multicolumn{4}{l}{\footnotesize $^c$ 
For giant stars G0 and later data taken from Schmidt--Kaler (1982).} \\
\multicolumn{4}{l}{\footnotesize $^d$
Temperature for star of Luminosity Class Iab.} \\
\end{tabular}
\clearpage
\begin{tabular}{rlll}
\hline
\multicolumn{1}{c}{Spectral Type $^a$} &
\multicolumn{1}{c}{T$_{I-II}^b$}    &
\multicolumn{1}{c}{T$_{III}^{b,c}$}     &
\multicolumn{1}{c}{T$_{IV-V}^b$}    \\\hline
%
G0--	 &  5510    &  5910   &   5930   \\
G2 	 & \nodata  & \nodata &   5830   \\ 
G3	 &  4980    & \nodata &  \nodata \\
G4	 & \nodata  &  5190   &   5740   \\
G6	 & \nodata  &  5050   &   5620   \\
G8--	 &  4590    &  4960   &  \nodata \\
K0--	 &  4420    &  4810   &   5240   \\
K1--	 &  4330    &  4610   &  \nodata \\
K2--	 &  4260    &  4500   &   5010   \\
K3--	 &  4130$^d$&  4320   &  \nodata \\
K4--  	 & \nodata  &  4080   &   4560   \\
K5--	 &  3850$^d$&  3980   &   4340   \\ 
K7	 & \nodata  & \nodata &   4040   \\
M0--	 &  3650$^d$&  3820   &   3800   \\
M1--	 &  3550$^d$&  3780   &   3680   \\
M2--	 &  3450$^d$&  3710   &   3530   \\
M3--	 &  3200$^d$&  3630   &   3380   \\
M4--	 &  2980$^d$&  3560   &   3180   \\
M5--	 & \nodata  &  3420   &   3030   \\
M6--	 & \nodata  &  3250   &   2850   \\\hline 
%
\end{tabular}
\clearpage
\begin{tabular}{lll}
\hline
\multicolumn{1}{c}{Date} &
\multicolumn{1}{c}{Type} &
\multicolumn{1}{c}{ \# of Stars} \\\hline\hline
%
March 9--10, 1993 & Day & 17 \\
April 1--3, 1993 & Day/Night & 30 \\
May 18--19, 1993 & Day & 10 \\
January 30--31, 1994 & Day/Night & 42 \\\hline
%
\end{tabular}
\clearpage
\begin{table}
\caption{H--Band Spectral Indices for Classification of A-M Stars}
\begin{tabular}{lllllll}
\tableline
%
\multicolumn{1}{c}{Main Feature \tablenotemark{a}}&
\multicolumn{1}{c}{E$_{low}$ (ev) } &
\multicolumn{1}{c}{$\sigma$ (cm$^{-1}$) \tablenotemark{a}}&
\multicolumn{1}{c}{$\lambda$ ($\mu$m) } &
\multicolumn{1}{c}{$\sigma_{cent}$ (cm$^{-1}$)}&
\multicolumn{1}{c}{$\Delta \sigma$ (cm$^{-1}$)} &
\multicolumn{1}{c}{Other contr. \tablenotemark{a}} \\\tableline\tableline
%
MgI(4s--4p)          & 5.39 \tablenotemark{b}& 5843.41 & 1.71133 & 5844
& 10 & CO, Fe, Ni, OH  \\
OH($\Delta v = 2$) & 0.76 \tablenotemark{c}& 5920:   & 1.689   & 5920   &
20 & C, CO, Fe, Ni   \\
HI(4-11)             & 12.75 \tablenotemark{d}& 5948.50 & 1.68110 & 5950
& 20 & CO, Fe, Ni, Si \\
AlI(4p--4d tr)       & 4.09 \tablenotemark{e}& 5963.76 & 1.67679 & 5972.5
& 25 & CO, Fe, Ni, OH    \\
                     &      & 5968.31 & 1.67552 &        &    &     \\
                     &      & 5979.60 & 1.67235 &        &    &     \\
SiI(4p--3d)          & 5.98 \tablenotemark{f}& 5993.29 & 1.66853 & 5993
& 10 & CO, Fe, Ni, OH   \\
$^{12}$CO(8,5)bh     & 1.55 \tablenotemark{g}& 6018    & 1.662  & 6017.5 &
15 & Fe, OH, S   \\
$^{12}$CO(6,3)bh     & 1.05 \tablenotemark{g} & 6177    & 1.619  & 6170
& 50 & Ca, Fe, Ni, OH, Si      \\
SiI(4p--5s)          & 5.98 \tablenotemark{f}& 6263.92 & 1.59644 & 6264
& 10 & Fe, Mg, Ni, OH       \\
MgI(4s--4p tr)       & 5.93 \tablenotemark{b}& 6341.10 & 1.57701 & 6345
& 20 & CN, CO, Fe, H$_2$O, Ni, OH \\
                     &      & 6347.88 & 1.57533 &        &    &      \\
                     &      & 6351.22 & 1.57450 &        &    &
\\\tableline
\end{tabular}
\tablenotetext{a}{Species indentification and frequencies from LW91 and
WL92.}
\tablenotetext{b}{Lower state energy level from Risberg (1965).}
\tablenotetext{c}{Coxon and Forester (1982).}
\tablenotetext{d}{Garcia and Mack (1965).}
\tablenotetext{e}{Eriksson and Isberg (1963).}
\tablenotetext{f}{Litzen (1964).}
\tablenotetext{g}{George, Urban, \& LeFloch (1994).}
\label{ftshband}
\end{table}
%\end{small}
\clearpage
\footnotesize
\begin{tabular}{llllllllllll} 
\hline 
% 
\multicolumn{1}{c}{Source} & 
\multicolumn{1}{c}{T$_{e}$ } & 
\multicolumn{1}{c}{SNR} & 
\multicolumn{1}{c}{Mg5844} & 
\multicolumn{1}{c}{OH5920} & 
\multicolumn{1}{c}{HI5950} & 
\multicolumn{1}{c}{Al5973} & 
\multicolumn{1}{c}{Si5993} & 
\multicolumn{1}{c}{CO6018} & 
\multicolumn{1}{c}{CO6170} & 
\multicolumn{1}{c}{Si6264} & 
\multicolumn{1}{c}{Mg6345} \\\hline\hline 
% 
HR1903   & 26000 & 203 & -0.03 &  0.09 &  0.75 &  0.17 & -0.02 &  0.11 &  0.27 &  0.11 &  0.47 \\ 
HR1903   & 26000 & 167 &  0.01 &  0.07 &  0.73 &  0.11 & -0.00 &  0.09 &  0.19 &  0.12 &  0.32 \\ 
HR1203   & 20700 & 160 & -0.01 &  0.12 &  0.80 &  0.18 &  0.01 &  0.11 &  0.23 &  0.11 &  0.56 \\ 
HR2827   & 13400 & 045 & -0.05 & -0.02 &  1.06 & -0.04 &  0.20 & -0.04 &  0.01 & -0.05 &  0.08 \\
HR1713   & 11200 & 218 &  0.04 &  0.06 &  1.27 &  0.23 &  0.05 &  0.09 &  0.19 &  0.17 &  0.50 \\ 
HR3975   &  9730 & 068 & -0.08 &  0.11 &  2.12 &  0.23 &  0.12 & -0.09 &  0.33 &  0.20 &  0.58 \\ 
HR7924   &  9080 & 225 & -0.05 &  0.00 &  1.40 &  0.20 & -0.02 &  0.03 & -0.14 &  0.08 &  0.08 \\ 
HR1865   &  7700 & 196 & -0.01 &  0.22 &  2.21 &  0.32 &  0.14 & -0.13 &  0.30 &  0.25 &  0.52 \\ 
HR1017   &  6640 & 248 &  0.08 &  0.25 &  1.88 &  0.43 &  0.06 & -0.02 &  0.53 &  0.41 &  1.05 \\ 
HR7796   &  6100 & 324 &  0.10 &  0.29 &  1.58 &  0.69 &  0.14 &  0.03 &  0.79 &  0.60 &  0.94 \\ 
HR8232   &  5510 & 290 &  0.09 &  0.37 &  1.28 &  0.67 &  0.17 &  0.03 &  1.18 &  0.67 &  1.19 \\ 
HR8752   &  5510 & 084 & -0.13 &  0.34 &  1.16 &  0.14 &  0.07 &  0.02 &  0.16 &  0.16 &  0.41 \\ 
HR7479   &  5333 & 096 &  0.15 &  0.13 &  1.13 &  0.70 &  0.10 &  0.00 &  0.92 &  0.41 &  0.69 \\ 
HR7479   &  5333 & 109 &  0.10 &  0.22 &  1.07 &  0.49 &  0.11 &  0.02 &  0.76 &  0.54 &  1.04 \\ 
HR7479   &  5333 & 182 &  0.13 &  0.12 &  1.08 &  0.56 &  0.05 &  0.07 &  0.94 &  0.49 &  1.06 \\ 
HR7479   &  5333 & 093 &  0.06 & -0.02 &  1.20 &  0.53 &  0.03 &  0.14 &  1.05 &  0.54 &  0.93 \\ 
HR7063   &  4902 & 260 &  0.17 &  0.12 &  0.94 &  0.84 &  0.14 &  0.25 &  1.66 &  0.76 &  1.06 \\ 
HR7314   &  4420 & 193 &  0.23 &  0.15 &  0.84 &  0.88 &  0.15 &  0.46 &  2.25 &  1.00 &  1.60 \\ 
HR7314   &  4420 & 257 &  0.15 &  0.17 &  0.67 &  0.59 &  0.10 &  0.37 &  1.91 &  0.86 &  1.36 \\ 
HR6713   &  4375 & 265 &  0.22 &  0.19 &  0.81 &  0.80 &  0.16 &  0.40 &  1.86 &  0.79 &  1.25 \\ 
HR8465   &  4295 & 308 &  0.13 &  0.28 &  0.68 &  0.70 &  0.19 &  0.63 &  2.35 &  1.02 &  1.79 \\ 
HR6498   &  4260 & 247 &  0.24 &  0.30 &  0.84 &  1.00 &  0.21 &  0.83 &  2.75 &  1.11 &  1.84 \\ 
HR603    &  4130 & 453 &  0.24 &  0.34 &  0.69 &  0.61 &  0.19 &  0.49 &  2.09 &  0.87 &  1.46 \\ 
HR8089   &  3990 & 202 &  0.21 &  0.45 &  0.50 &  0.67 &  0.14 &  0.68 &  2.26 &  0.94 &  1.59 \\ 
HR8079   &  3920 & 445 &  0.24 &  0.67 &  0.62 &  0.80 &  0.24 &  1.05 &  2.70 &  1.05 &  1.72 \\ 
HR2061   &  3550 & 327 &  0.54 &  1.08 &  0.36 &  1.39 &  0.23 &  1.46 &  3.92 &  0.89 &  2.22 \\ 
HR1155   &  3450 & 237 &  0.46 &  1.31 &  0.58 &  1.12 &  0.38 &  1.37 &  3.35 &  1.12 &  2.03 \\ 
HR921    &  2980 & 225 &  0.77 &  1.41 &  0.29 &  1.27 &  0.37 &  1.10 &  4.08 &  0.67 &  1.52 \\ 
HR7009   &  2925 & 292 &  0.63 &  1.43 &  0.79 &  1.55 &  0.54 &  1.79 &  4.68 &  1.26 &  2.21 \\ 
HR6406   &  2800 & 319 &  0.59 &  1.41 &  0.80 &  1.66 &  0.54 &  1.85 &  4.98 &  1.31 &  2.31 \\ 
\end{tabular} 
\clearpage
\begin{tabular}{llllllllllll} 
\hline 
% 
\multicolumn{1}{c}{Source} & 
\multicolumn{1}{c}{T$_{e}$ } & 
\multicolumn{1}{c}{SNR} & 
\multicolumn{1}{c}{Mg5844} & 
\multicolumn{1}{c}{OH5920} & 
\multicolumn{1}{c}{HI5950} & 
\multicolumn{1}{c}{Al5973} & 
\multicolumn{1}{c}{Si5993} & 
\multicolumn{1}{c}{CO6018} & 
\multicolumn{1}{c}{CO6170} & 
\multicolumn{1}{c}{Si6264} & 
\multicolumn{1}{c}{Mg6345} \\\hline\hline 
% 
HR1899   & 32000 & 164 & -0.03 &  0.17 &  0.54 &  0.15 & -0.04 &  0.03 &  0.18 &  0.10 &  0.49 \\ 
HR1899   & 32000 & 182 & -0.04 &  0.20 &  0.62 &  0.11 &  0.05 & -0.03 &  0.07 & -0.00 &  0.07 \\ 
HR1552   & 20300 & 115 & -0.07 &  0.13 &  1.29 &  0.31 &  0.10 & -0.09 &  0.12 & -0.01 &  0.09 \\ 
HR5291   & 10100 & 159 & -0.07 &  0.19 &  2.65 &  0.78 &  0.02 &  0.05 &  0.28 &  0.11 &  0.41 \\ 
HR403    &  8100 & 202 & -0.02 &  0.39 &  2.79 &  0.77 &  0.09 & -0.13 &  0.25 &  0.08 &  0.54 \\ 
HR1412   &  7650 & 186 & -0.02 &  0.43 &  2.70 &  0.71 &  0.05 & -0.10 &  0.60 &  0.25 &  0.91 \\ 
HR4031   &  7150 & 193 &  0.02 &  0.29 &  2.30 &  0.54 &  0.12 & -0.09 &  0.25 &  0.13 &  0.48 \\ 
HR21     &  6870 & 245 &  0.03 &  0.32 &  1.99 &  0.55 &  0.04 & -0.11 &  0.20 &  0.22 &  0.82 \\ 
HR21     &  6870 & 179 &  0.01 &  0.25 &  2.21 &  0.63 &  0.13 & -0.14 &  0.46 &  0.24 &  0.69 \\ 
HR5017   &  6700 & 174 &  0.04 &  0.28 &  2.58 &  0.83 &  0.07 & -0.03 &  0.43 &  0.36 &  0.96 \\ 
HR2706   &  6470 & 086 &  0.01 &  0.39 &  2.08 &  0.47 &  0.16 & -0.10 &  0.13 &  0.20 &  0.64 \\ 
HR8905   &  6270 & 059 &  0.06 &  0.13 &  1.06 &  0.45 & -0.01 & -0.16 &  0.30 &  0.28 &  1.02 \\ 
HR4883   &  5910 & 280 &  0.15 &  0.20 &  1.07 &  0.52 &  0.09 &  0.04 &  0.90 &  0.43 &  1.02 \\ 
HR4716   &  5050 & 133 &  0.17 &  0.10 &  0.97 &  0.47 &  0.13 &  0.07 &  1.29 &  0.54 &  0.92 \\ 
HR7328   &  4885 & 281 &  0.19 &  0.20 &  0.78 &  0.57 &  0.11 &  0.11 &  1.33 &  0.67 &  1.35 \\ 
HR7949   &  4810 & 369 &  0.21 &  0.24 &  0.77 &  0.59 &  0.13 &  0.18 &  1.39 &  0.67 &  1.38 \\ 
HR8317   &  4710 & 191 &  0.29 &  0.14 &  0.63 &  0.58 &  0.08 &  0.26 &  1.79 &  0.83 &  1.64 \\ 
HR6299   &  4500 & 532 &  0.26 &  0.09 &  0.77 &  0.81 &  0.10 &  0.44 &  1.92 &  0.76 &  1.40 \\ 
HR165    &  4320 & 266 &  0.34 &  0.24 &  0.64 &  0.58 &  0.18 &  0.41 &  1.98 &  0.89 &  1.45 \\ 
HR6705   &  3990 & 298 &  0.39 &  0.60 &  0.77 &  1.12 &  0.26 &  0.96 &  3.05 &  1.12 &  1.75 \\ 
HR6705   &  3990 & 694 &  0.41 &  0.61 &  0.76 &  1.07 &  0.25 &  0.89 &  2.87 &  1.06 &  1.66 \\ 
HR152    &  3956 & 270 &  0.37 &  0.86 &  0.58 &  0.92 &  0.34 &  0.87 &  2.59 &  0.78 &  1.40 \\ 
HR4517   &  3780 & 673 &  0.66 &  1.06 &  0.33 &  1.07 &  0.21 &  0.89 &  3.14 &  0.70 &  1.93 \\ 
HR6242   &  3560 & 458 &  0.52 &  1.12 &  0.57 &  1.18 &  0.39 &  1.45 &  3.93 &  1.16 &  1.96 \\ 
HR7886   &  3250 & 574 &  0.61 &  1.54 &  0.89 &  1.71 &  0.64 &  2.25 &  5.69 &  1.41 &  2.42 \\ 
\end{tabular} 
\clearpage
\begin{tabular}{llllllllllll} 
\hline 
% 
\multicolumn{1}{c}{Source} & 
\multicolumn{1}{c}{T$_{e}$ } & 
\multicolumn{1}{c}{SNR} & 
\multicolumn{1}{c}{Mg5844} & 
\multicolumn{1}{c}{OH5920} & 
\multicolumn{1}{c}{HI5950} & 
\multicolumn{1}{c}{Al5973} & 
\multicolumn{1}{c}{Si5993} & 
\multicolumn{1}{c}{CO6018} & 
\multicolumn{1}{c}{CO6170} & 
\multicolumn{1}{c}{Si6264} & 
\multicolumn{1}{c}{Mg6345} \\\hline\hline 
% 
HR6588   & 19000 & 162 & -0.03 &  0.10 &  1.65 &  0.48 & -0.03 &  0.02 &  0.17 &  0.07 &  0.40 \\ 
HR4033   &  8810 & 146 & -0.00 &  0.33 &  2.62 &  0.73 &  0.06 &  0.02 &  0.27 &  0.13 &  0.35 \\ 
HR1351   &  7020 & 094 & -0.06 &  0.40 &  2.18 &  0.62 &  0.19 & -0.19 & -0.01 &  0.10 &  0.24 \\ 
HR5235   &  5930 & 341 &  0.16 &  0.12 &  1.21 &  0.83 &  0.11 &  0.03 &  1.30 &  0.64 &  1.14 \\ 
HR5235   &  5930 & 263 &  0.17 &  0.26 &  1.26 &  0.68 &  0.18 & -0.01 &  0.97 &  0.50 &  1.03 \\ 
HR5409   &  5830 & 158 &  0.16 &  0.16 &  1.02 &  0.51 &  0.12 & -0.03 &  0.91 &  0.44 &  0.95 \\ 
HR6623   &  5680 & 211 &  0.33 &  0.12 &  0.87 &  0.87 &  0.09 &  0.09 &  1.21 &  0.69 &  1.38 \\ 
HR995    &  5620 & 143 &  0.22 &  0.08 &  0.80 &  0.61 &  0.23 &  0.03 &  1.09 &  0.48 &  1.14 \\ 
HR7602   &  5430 & 056 &  0.46 &  0.15 &  0.71 &  0.86 &  0.01 &  0.17 &  1.40 &  0.57 &  1.49 \\ 
HR7957   &  5240 & 189 &  0.22 &  0.09 &  0.68 &  0.70 &  0.07 &  0.15 &  1.04 &  0.46 &  0.99 \\ 
HR7957   &  5240 & 192 &  0.09 &  0.18 &  0.56 &  0.52 & -0.01 &  0.09 &  0.75 &  0.40 &  1.17 \\ 
HR5901   &  5125 & 395 &  0.37 &  0.13 &  0.55 &  0.62 &  0.08 &  0.21 &  1.61 &  0.74 &  1.60 \\ 
HR5901   &  5125 & 153 &  0.37 &  0.09 &  0.75 &  0.93 &  0.15 &  0.30 &  1.54 &  0.71 &  1.13 \\ 
HR6014   &  5068 & 072 &  0.31 & -0.12 &  0.39 &  0.59 &  0.14 &  0.05 &  1.10 &  0.70 &  1.40 \\ 
HR6014   &  5068 & 133 &  0.42 &  0.11 &  0.58 &  0.55 &  0.18 &  0.09 &  1.48 &  0.65 &  1.24 \\ 
\end{tabular} 
\clearpage
\begin{tabular}{llllllllllll} 
\hline 
% 
\multicolumn{1}{c}{Source} & 
\multicolumn{1}{c}{T$_{e}$ } & 
\multicolumn{1}{c}{SNR} & 
\multicolumn{1}{c}{Mg5844} & 
\multicolumn{1}{c}{OH5920} & 
\multicolumn{1}{c}{HI5950} & 
\multicolumn{1}{c}{Al5973} & 
\multicolumn{1}{c}{Si5993} & 
\multicolumn{1}{c}{CO6018} & 
\multicolumn{1}{c}{CO6170} & 
\multicolumn{1}{c}{Si6264} & 
\multicolumn{1}{c}{Mg6345} \\\hline\hline 
% 
HR2456   & 38000 & 053 & -0.03 &  0.36 &  0.39 &  0.26 &  0.16 &  0.12 & -0.32 &  0.11 &  0.31 \\ 
HR2456   & 38000 & 073 & -0.12 &  0.18 &  0.48 &  0.10 &  0.06 & -0.15 &  0.15 &  0.03 &  0.10 \\ 
HR5191   & 19000 & 282 & -0.05 &  0.19 &  1.71 &  0.57 &  0.08 & -0.07 &  0.22 &  0.07 &  0.24 \\ 
HR3982   & 13000 & 241 & -0.08 &  0.13 &  2.22 &  0.47 &  0.04 & -0.09 &  0.28 &  0.03 &  0.15 \\ 
HR3982   & 13000 & 241 & -0.07 &  0.09 &  2.14 &  0.51 &  0.06 & -0.09 &  0.32 &  0.12 &  0.26 \\ 
HR7001   &  9480 & 678 & -0.05 &  0.36 &  2.83 &  1.06 &  0.03 & -0.03 &  0.41 &  0.15 &  0.52 \\ 
HR7001   &  9480 & 146 & -0.10 &  0.38 &  2.81 &  1.02 &  0.10 & -0.05 &  0.43 &  0.17 &  0.41 \\ 
HR2491   &  9145 & 111 & -0.07 &  0.36 &  2.71 &  0.83 &  0.16 & -0.14 &  0.37 & -0.08 &  0.10 \\ 
HR2491   &  9145 & 148 & -0.14 &  0.40 &  2.67 &  0.93 &  0.12 & -0.13 &  0.39 &  0.05 &  0.20 \\ 
HR4534   &  8593 & 205 & -0.04 &  0.45 &  2.67 &  1.01 &  0.11 & -0.12 &  0.30 &  0.07 &  0.34 \\ 
HR4357   &  8377 & 192 & -0.05 &  0.40 &  2.83 &  0.96 &  0.09 & -0.12 &  0.24 &  0.06 &  0.38 \\ 
HR4931   &  6750 & 119 &  0.04 &  0.24 &  1.47 &  0.62 & -0.01 & -0.06 &  0.09 &  0.09 &  0.86 \\ 
HR1279   &  6677 & 080 &  0.10 &  0.32 &  1.62 &  0.67 &  0.15 & -0.09 &  0.26 &  0.12 &  0.64 \\ 
HR2943   &  6530 & 327 &  0.04 &  0.33 &  1.60 &  0.57 &  0.15 & -0.14 &  0.54 &  0.27 &  0.74 \\ 
HR1538   &  6385 & 281 &  0.06 &  0.34 &  1.26 &  0.53 &  0.18 & -0.11 &  0.51 &  0.22 &  0.90 \\ 
HR4375   &  6085 & 254 &  0.26 &  0.15 &  0.63 &  0.56 &  0.15 & -0.06 &  0.68 &  0.37 &  1.09 \\ 
HR4983   &  5930 & 123 &  0.21 &  0.16 &  0.75 &  0.66 &  0.09 &  0.04 &  0.71 &  0.45 &  1.20 \\ 
HR4983   &  5930 & 173 &  0.19 &  0.21 &  0.90 &  0.52 &  0.19 & -0.06 &  0.87 &  0.47 &  0.96 \\ 
HR483    &  5855 & 059 &  0.24 &  0.02 &  0.68 &  0.29 &  0.04 & -0.17 &  0.18 &  0.37 &  1.09 \\ 
HR483    &  5855 & 079 &  0.24 &  0.19 &  0.90 &  0.46 &  0.19 & -0.11 &  0.67 &  0.48 &  1.30 \\ 
HR4374   &  5830 & 250 &  0.28 &  0.20 &  0.62 &  0.63 &  0.10 & -0.01 &  0.90 &  0.47 &  1.35 \\ 
HR5072   &  5740 & 197 &  0.26 &  0.15 &  0.74 &  0.53 &  0.16 & -0.04 &  0.99 &  0.53 &  1.28 \\ 
HR4496   &  5430 & 105 &  0.35 &  0.17 &  0.59 &  0.59 &  0.21 & -0.08 &  1.12 &  0.61 &  1.45 \\ 
HR4496   &  5430 & 090 &  0.31 &  0.16 &  0.39 &  0.50 &  0.13 & -0.04 &  0.69 &  0.43 &  1.08 \\ 
HR7462   &  5240 & 131 &  0.52 &  0.04 &  0.38 &  0.72 &  0.09 &  0.09 &  1.20 &  0.62 &  1.89 \\ 
HR7462   &  5240 & 095 &  0.51 &  0.07 &  0.37 &  0.69 &  0.13 &  0.06 &  1.16 &  0.72 &  2.05 \\ 
HR1084   &  5010 & 223 &  0.61 &  0.19 &  0.44 &  0.74 &  0.24 & -0.01 &  1.59 &  0.76 &  2.00 \\ 
HR8832   &  4785 & 111 &  0.88 &  0.14 &  0.29 &  1.06 &  0.17 &  0.18 &  1.88 &  0.90 &  2.50 \\ 
GL570A   &  4560 & 120 &  0.90 &  0.22 &  0.37 &  1.13 &  0.28 &  0.04 &  2.02 &  0.90 &  2.29 \\ 
HR8085   &  4340 & 125 &  0.65 &  0.18 &  0.01 &  1.15 &  0.11 &  0.15 &  1.59 &  0.60 &  2.38 \\ 
HR8086   &  4040 & 170 &  0.72 &  0.39 &  0.06 &  1.46 &  0.14 &  0.11 &  1.78 &  0.50 &  2.07 \\ 
HR8086   &  4040 & 181 &  0.72 &  0.32 &  0.07 &  1.48 &  0.15 &  0.12 &  1.86 &  0.52 &  2.18 \\ 
GL338A   &  3800 & 072 &  0.98 &  0.37 &  0.08 &  1.36 &  0.13 &  0.02 &  1.51 &  0.34 &  1.80 \\ 
GL526    &  3605 & 068 &  0.62 &  0.42 & -0.13 &  1.32 &  0.16 &  0.10 &  1.04 &  0.04 &  0.92 \\ 
GL411    &  3530 & 202 &  0.48 &  0.53 & -0.04 &  1.29 &  0.16 &  0.01 &  1.17 &  0.10 &  1.19 \\ 
GL411    &  3530 & 189 &  0.47 &  0.55 & -0.07 &  1.29 &  0.18 &  0.06 &  1.21 &  0.12 &  1.23 \\ 
GL725A   &  3380 & 083 &  0.52 &  0.57 & -0.10 &  1.15 &  0.06 &  0.03 &  0.93 & -0.00 &  0.99 \\ 
GL725A   &  3380 & 107 &  0.54 &  0.56 & -0.12 &  1.25 &  0.02 &  0.08 &  1.20 & -0.02 &  1.09 \\ 
\end{tabular} 
\end{document}
