Sometimes the normal tables in LaTeX just don’t do it for you. You want to do something fancier or customize the table in a way that you just can’t do using the normal *tabular* environment. This is why I like using the *Deluxetable* style in latex. *Deluxetable* makes tables that are more flexible, and overall have a nicer look than normal latex tables. *Deluxetable* can handle multi-page tables, footnoting, multi-column headers, and much more that the *tabular* environment can’t do. Below is an example of a cool table with some nice features that I made for my thesis using the *Deluxetable* style package:

Some nice features of this table: adjustable table width, 1 or 2 line column headings are aligned at center, 1 or 2 line data sets are aligned at center, adjustable heights of rows.

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}

Here is an example of a more complicated Deluxetable from Charles Danforth at University of Colorado.

{ 1 comment… read it below or add one }

Many thanks for your example! I was trying to center the caption text and this works excellent :)!