From: http://www.astrobetter.com/how-to-make-awesome-latex-tables/
Below is the code used to generate the above table. Note that you need the file deluxetable.sty and the package nicefrac:
\begin{deluxetable}{cccccccc}\tabletypesize{\footnotesize}
\tablecolumns{8}
\tablewidth{0pt}
\tablecaption{ Cross-correlation Fit Details \label{table:results1}}
\tablehead{
\colhead{QSO} \vspace{-0.2cm} & \colhead{$R$ Range} & & & & & \colhead{Separation} & \colhead{Result}\\ \vspace{-0.2cm}
& & \colhead{$\langle f \rangle$} & \colhead{$r_0$} & \colhead{$\gamma$} & $W$ & & \\
\colhead{Division} & \colhead{(Mpc/h)} & \colhead{} & \colhead{} & \colhead{} & & \colhead{(\%)} & \colhead{Strength}}
\startdata
\vspace{-0.2cm} \nicefrac{1}{3} Bright & & $4.24 \cdot 10^{-4}$ & 6.19 & & 96.97 & & \\ \vspace{-0.2cm}
& [0.3,3] & & & 1.77 & & 96.7 & 1.9$\sigma$ \\
\nicefrac{2}{3} Dim & & $4.26 \cdot 10^{-4}$ & 4.48 & & 52.77
\enddata
\vspace{-0.8cm}
\tablecomments{Luminosity dependent quasar clustering using a cross-correlation technique between CS82 galaxies ($M < 23.5$) and SDSS, BOSS, and 2SLAQ quasars \hbox{($0.5 < z < 1.0$)}. The quasars were broken up into the \nicefrac{1}{3} brightest and \nicefrac{2}{3} dimmest, and a cross-correlation function was calculated between a range of \hbox{$[0.3-3.0]$ Mpc}. A power-law fit to the data of the form $\xi(r) = (r_0 / r)^\gamma$ found that $\gamma = 1.77$ and $r_0 = 6.19$ for the bright sample and $r_0 = 4.48$ for the dim sample.}
\end{deluxetable}
\documentclass[10pt,preprint]{aastex}
\begin{document}
\newcommand\sk[2]{Sk\,{$-#1{^\circ}#2$}}
\newcommand\tnc{\,\tablenotemark{c}}
\newcommand\tnd{\,\tablenotemark{d}}
\begin{deluxetable}{lllllllll}
\tabletypesize{\footnotesize}
\tablecolumns{7}
\tablewidth{0pt}
\tablecaption{Observational Parameters for FUSE Targets}
\tablehead{\colhead{Target} &
\multicolumn{2}{c}{RA (J2000) Dec} &
\colhead{Spectral Type} &
\colhead{Ref.\,\tablenotemark{a}} &
\colhead{$V$} &
\colhead{(\bv)} &
\colhead{Ref.\,\tablenotemark{b}} &
\colhead{Notes} \\
\colhead{} &
\colhead{{h}\phn{m}\phn{s}} &
\colhead{\phn{\arcdeg}~\phn{\arcmin}~\phn{\arcsec}} &
\colhead{} &
\colhead{} &
\colhead{} &
\colhead{} &
\colhead{} &
\colhead{} }
\startdata
\sidehead{Large Magellanic Cloud }
\sk{65}{21} & 05 01 22.33 & $-$65 41 48.1 & O9.7 Iab & W95 & 12.02 & $-$0.16 & I75 & \\
\sk{65}{22} & 05 01 24.00 & $-$65 52 00.0 & O6 Iaf+ & W77 & 12.07 & $-$0.19 & I79 & HDE\,270952 \\
\sk{66}{18} & 04 55 59.88 & $-$65 58 30.0 & O6 V((f)) & M95 & 13.50 & $-$0.20 & I79 & \\
\sk{66}{51} & 05 03 10.20 & $-$66 40 54.0 & WN8h & S96 & 12.71 & $-$0.23 & F83 & HD\,33133 \\
\sk{66}{100} & 05 27 45.59 & $-$66 55 15.0 & O6 II(f) & W95 & 13.26 & $-$0.21 & I79 & \\
& & & & & & & & \\
\sk{68}{52} & 05 07 20.60 & $-$68 32 09.6 & B0 Ia & W77 & 11.54 & $-$0.07 & A72 & HDE\,269050 \\
\sk{68}{75} & 05 23 28.52 & $-$68 12 22.8 & B1 I & J01 & 12.03 & $-$0.06 & A72 & HDE\,269463 \\
\sk{68}{80} & 05 26 30.43 & $-$68 50 26.6 & WC4+O6V-III & M90 & 12.42 & $-$0.23 & F83 & HD\,36521 \\
\sk{68}{82} & 05 26 45.30 & $-$68 49 52.8 & WN5?b+(B3I) & S96 & \phn9.86 & $-$0.03 & I82 & HDE\,269546 \\
\sk{68}{135} & 05 37 48.60 & $-$68 55 08.0 & ON9.7 Ia+ & W77 & 11.36 &\phs0.00 & A72 & HDE\,269896 \\
& & & & & & & & \\
BI\,170 & 05 26 47.79 & $-$69 06 11.7 & O9.5 Ib & W01 & 13.09 & $-$0.17 & B75 & \\
BI\,173 & 05 27 10.08 & $-$69 07 56.2 & O8 II: & W01 & 13.00 & $-$0.14 & B75 & \\
\sk{69}{142}a& 05 27 52.75 & $-$68 59 08.6 & WN10h & C97 & 11.88\tnc & $-$0.04 & S86 & BE294, HDE\,269582\\
\sk{69}{175} & 05 31 25.61 & $-$69 05 38.4 & WN11h & C97 & 11.90 & $-$0.07 & I75 & S119, HDE\,269687 \\
\sk{69}{191} & 05 34 19.39 & $-$69 45 10.0 & WC4 & T88 & 13.35 & $-$0.20 & F83 & HD\,37680 \\
& & & & & & & & \\
\sk{70}{69} & 05 05 18.73 & $-$70 25 49.8 & O5 V & W95 & 13.94 & $-$0.27:& R78 & \\
\sk{70}{91} & 05 27 33.74 & $-$70 36 48.3 & O6.5 V & C86 & 12.78 & $-$0.23 & I79 & \\
\sk{70}{115} & 05 48 49.76 & $-$70 03 57.5 & O6.5 Iaf & Wpc & 12.24 & $-$0.10 & I75 & HDE\,270145 \\
\sk{70}{120} & 05 51 20.85 & $-$70 17 08.7 & B1 Ia & F88 & 11.59 & $-$0.06 & A72 & HDE\,270196 \\
\sk{71}{45} & 05 31 15.55 & $-$71 04 08.9 & O4-5 III(f) & W77 & 11.51\tnd & $-$0.19 & H91 & HDE\,269676 \\
& & & & & & & & \\
\cutinhead{Small Magellanic Cloud}
AV\,6 & 00 45 18.20 & $-$73 15 23.4 & O9 III & L97 & 13.46 & $+$0.03 & A75 & \\
AV\,14 & 00 46 32.66 & $-$73 06 05.6 & O3-4 V & G87b & 13.77 & $-$0.19 & A75 & Sk\,9 \\
AV\,15 & 00 46 42.19 & $-$73 24 54.7 & O6.5 II(f) & W00 & 13.17 & $-$0.21 & I78 & Sk\,10 \\
AV\,26 & 00 47 50.07 & $-$73 08 20.7 & O7 III & G87b & 12.55 & $-$0.20 & A75 & Sk\,18 \\
AV\,47 & 00 48 51.35 & $-$73 25 57.6 & O8 III((f)) & W00 & 13.38 & $-$0.26 & A75 & \\
& & & & & & & & \\
AV\,69 & 00 50 17.40 & $-$72 53 29.9 & OC7.5 III((f))& W00 & 13.35 & $-$0.22 & A75 & \\
AV\,70 & 00 50 18.14 & $-$72 38 09.8 & O9.5 Iw & W83 & 12.38 & $-$0.17 & A75 & Sk\,35 \\
AV\,75 & 00 50 32.50 & $-$72 52 36.2 & O5 III(f+) & W00 & 12.79 & $-$0.16 & I78 & Sk\,38 \\
AV\,81 & 00 50 43.47 & $-$73 27 06.1 & WN5h & S96 & 13.29 & $-$0.10 & A75 & Sk\,41 \\
AV\,83 & 00 50 52.01 & $-$72 42 14.5 & O7 Iaf+ & W00 & 13.58 & $-$0.13 & W00 & \\
\enddata
\tablenotetext{a}{References for Spectral Types.~
C82 = Crampton (1982);
C86 = Conti et~al (1986);
C97 = Crowther (1997);
Wpc = Walborn, private communication,
etc }
\tablenotetext{b}{References for Photometry.~
A72 = Ardeberg (1972);
A75 = Azzopardi \& Vigneau (1975);
etc }
\tablenotetext{c}{Variable.}
\tablenotetext{d}{Photometric measurements refer to a blend of several nearby sources.}
\end{deluxetable}
\end{document}
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