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Latex 表格超出页面宽度

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Latex 表格超出页面宽度

我现在面临的一个最小工作示例：

\begin{table}
\centering

\begin{tabular}{|c|c|c|c|c|c|c|}
\hline
\multicolumn{1}{p{2cm}}{\centering Mass ($h^{-1}\;M_{\odot}$)}
& \multicolumn{1}{p{2cm}}{\centering $z$}
& \multicolumn{1}{p{2cm}}{\centering $r_{0}$} & 
$\gamma$ & $r_{0} \: (\gamma=2.0)$ & $N_{clusters}$ & bias \\ 
\hline
$M_{halo}>2\times10^{13}$ & $0.1<z_c<0.4$ & 9.89$\pm$0.20 & 1.76$\pm$0.05
             & 9.53$\pm$0.29 & 10492 & 1.81$\pm$0.03 \\ [1ex] 
        & $0.4<z_c<0.7$ & 10.22$\pm$0.14 & 1.84$\pm$0.04 & 10.01$\pm$0.17 & 27224 & 2.00$\pm$0.03 \\ [1ex] 
        & $0.7<z_c<1.0$ & 11.10$\pm$0.15 & 1.87$\pm$0.04 & 10.85$\pm$0.17 & 35133 & 2.52$\pm$0.02 \\ [1ex] 
        & $1.0<z_c<1.3$ & 11.62$\pm$0.23 & 1.98$\pm$0.05 & 11.58$\pm$0.19 & 31815 & 3.01$\pm$0.06 \\ [1ex] 
        & $1.3<z_c<1.6$ & 12.41$\pm$0.42 & 2.13$\pm$0.09 & 12.49$\pm$0.52 & 22978 & 3.37$\pm$0.19 \\ [1ex] 
        & $1.6<z_c<2.1$ & 14.78$\pm$0.21 & 2.06$\pm$0.05 & 14.78$\pm$0.22 & 18931 & 4.65$\pm$0.23 \\ [1ex] \hline \noalign{\vskip 0.1cm}    

\end{tabular} 

\caption{The best-fit values of the parameters of the real-space correlation function $\xi(r)$ for the light-cone at different (1) mass thresholds and (2) redshift ranges. For each sample we quote (3) the correlation length $r_{0}$, (4) slope $\gamma$, (5) correlation length $r_{0}$ at fixed slope $\gamma=2.0$, (6) number of clusters $N_{clusters}$ and (7) the bias $b$ obtained.} 
\label{table:clustering_with_mass}

\end{table}

我的表格最终超出了指定的页面宽度，看起来像这样。

在此处输入图片描述

我检查了使用等的几个答案tabularx，但它们似乎不能正常工作。

答案1

如果你需要保持表格纵向，我建议

  • 您设置长度参数\thickmuskip和\medmuskip为0mu；

  • 简化第二列的结构；

  • 摆脱固定宽度的标题单元格定义；

  • 使用tabular*环境而不是tabular环境；并且

  • 从 切换\normalsize到\small。

在此处输入图片描述

\documentclass{report}
\usepackage{amsmath}
\usepackage{booktabs}

\begin{document}
\begin{table}
\setlength\tabcolsep{0pt}
\setlength\thickmuskip{0mu}
\setlength\medmuskip{0mu}
\small
\begin{tabular*}{\textwidth}{c@{\extracolsep{\fill}}*{6}{c}}
\toprule
Mass  & $z_c$ & $r_{0}$ & $\gamma$ 
& $r_{0}$ ($\gamma=2.0$) & $N_{\textrm{clusters}}$ & bias \\ 
($h^{-1}M_{\odot}$)\\
\midrule
$M_{\textrm{halo}}>2\times10^{13}$ & $0.1\text{--}0.4$ & 9.89$\pm$0.20 & 1.76$\pm$0.05 & 9.53$\pm$0.29 & 10492 & 1.81$\pm$0.03 \\ \addlinespace 
& $0.4\text{--}0.7$ & 10.22$\pm$0.14 & 1.84$\pm$0.04 & 10.01$\pm$0.17 & 27224 & 2.00$\pm$0.03 \\ \addlinespace 
& $0.7\text{--}1.0$ & 11.10$\pm$0.15 & 1.87$\pm$0.04 & 10.85$\pm$0.17 & 35133 & 2.52$\pm$0.02 \\ \addlinespace 
& $1.0\text{--}1.3$ & 11.62$\pm$0.23 & 1.98$\pm$0.05 & 11.58$\pm$0.19 & 31815 & 3.01$\pm$0.06 \\ \addlinespace 
& $1.3\text{--}1.6$ & 12.41$\pm$0.42 & 2.13$\pm$0.09 & 12.49$\pm$0.52 & 22978 & 3.37$\pm$0.19 \\ \addlinespace 
& $1.6\text{--}2.1$ & 14.78$\pm$0.21 & 2.06$\pm$0.05 & 14.78$\pm$0.22 & 18931 & 4.65$\pm$0.23 \\ 
\bottomrule  

\end{tabular*} 

\caption[The best-fit values of the parameters of the real-space correlation function $\xi(r)$]{The best-fit values of the parameters of the real-space correlation function $\xi(r)$ for the light-cone at different (1)~mass thresholds and (2)~redshift ranges. For each sample we quote (3)~the correlation length $r_{0}$, (4)~slope $\gamma$, (5)~correlation length $r_{0}$ at fixed slope $\gamma=2.0$, (6)~number of clusters $N_{\textrm{clusters}}$, and (7)~the bias $b$ obtained.} 
\label{table:clustering_with_mass}

\end{table}
\end{document}

答案2

另一方面，这是旋转表格的解决方案。我还对您的代码进行了一些整理。

% My standard header for TeX.SX answers:
\documentclass[a4paper]{article} % To avoid confusion, let us explicitly 
                                 % declare the paper format.

\usepackage[T1]{fontenc}         % Not always necessary, but recommended.
% End of standard header.  What follows pertains to the problem at hand.

\usepackage{rotating,booktabs,amstext}
\usepackage{lipsum}



\begin{document}

\lipsum[1-4]

\begin{sidewaystable}
    \centering
    \begin{tabular}{*{7}c}
        \toprule
        \multicolumn{1}{p{2cm}}{\centering Mass ($h^{-1}\;M_{\odot}$)}
        & \multicolumn{1}{p{2cm}}{\centering $z$}
        & \multicolumn{1}{p{2cm}}{\centering $r_{0}$} & 
        $\gamma$ & $r_{0} \: (\gamma=2.0)$ & $N_{\text{clusters}}$ & bias \\ 
        \midrule
        $M_{halo}>2\times10^{13}$ & $0.1<z_c<0.4$ & 9.89$\pm$0.20 & 1.76$\pm$0.05
             & 9.53$\pm$0.29 & 10492 & 1.81$\pm$0.03 \\ [1ex] 
        & $0.4<z_c<0.7$ & 10.22$\pm$0.14 & 1.84$\pm$0.04 & 10.01$\pm$0.17 & 27224 & 2.00$\pm$0.03 \\ [1ex] 
        & $0.7<z_c<1.0$ & 11.10$\pm$0.15 & 1.87$\pm$0.04 & 10.85$\pm$0.17 & 35133 & 2.52$\pm$0.02 \\ [1ex] 
        & $1.0<z_c<1.3$ & 11.62$\pm$0.23 & 1.98$\pm$0.05 & 11.58$\pm$0.19 & 31815 & 3.01$\pm$0.06 \\ [1ex] 
        & $1.3<z_c<1.6$ & 12.41$\pm$0.42 & 2.13$\pm$0.09 & 12.49$\pm$0.52 & 22978 & 3.37$\pm$0.19 \\ [1ex] 
        & $1.6<z_c<2.1$ & 14.78$\pm$0.21 & 2.06$\pm$0.05 & 14.78$\pm$0.22 & 18931 & 4.65$\pm$0.23 \\ [1ex]
        \bottomrule
    \end{tabular} 
    \smallskip
    \caption[A short caption for the LOT\@]
        {The best-fit values of the parameters of the real-space correlation
        function~$\xi(r)$ for the light-cone at different (1)~mass thresholds
        and (2)~redshift ranges.  For each sample we quote (3)~the correlation
        length~$r_{0}$, (4)~slope~$\gamma$, (5)~correlation length~$r_{0}$ at
        fixed slope $\gamma=2.0$, (6)~number of clusters $N_{\text{clusters}}$
        and (7)~the bias~$b$ obtained.}
    \label{table:clustering_with_mass}
\end{sidewaystable}

\lipsum[5-8]

\end{document}

包含该表格的页面图像如下：

表格图片

答案3

\small如果您使用字体大小，并且将第二行第一个单元格的内容（ ）设为副标题，则它可以适合文本宽度，M_halo位于其自己的一行上。这是一个代码，对表格进行了一些改进，代码更简单。特别是，我使用了一个array环境，并且只保留了一些水平规则，这要归功于booktabs包：

\documentclass[a4paper,11pt]{article}

\usepackage[showframe]{geometry}%
\usepackage{booktabs}
\usepackage{array, tabularx, makecell}
\usepackage{siunitx}

\begin{document}

\begin{table}
  \centering
  \small\setlength\extrarowheight{1ex}%
  $ \begin{array}{ccrrrcc}
  \makecell{\text{Mass}\\ (h⁻¹\;M_{\odot})}
  & z & \makecell{r_{0}} & \makecell{γ} & \makecell{r_{0} \: (\gamma=2.0)} & N_\text{clusters} & \text{bias} \\
  \midrule[\heavyrulewidth]
  \multicolumn{7}{l}{M_\text{halo}>2 × 10^{13}}\\[0.5ex]
  & 0.1<z_c<0.4 & 9.89 ±0.20 & 1.76 ±0.05
  & 9.53 ±0.29 & 10492 & 1.81 ±0.03 \\ & 0.4<z_c<0.7 & 10.22 ±0.14 & 1.84 ±0.04 & 10.01 ±0.17 & 27224 & 2.00 ±0.03 \\ & 0.7<z_c<1.0 & 11.10 ±0.15 & 1.87 ±0.04 & 10.85 ±0.17 & 35133 & 2.52 ±0.02 \\ & 1.0<z_c<1.3 & 11.62 ±0.23 & 1.98 ±0.05 & 11.58 ±0.19 & 31815 & 3.01 ±0.06 \\
  & 1.3<z_c<1.6 & 12.41 ±0.42 & 2.13 ±0.09 & 12.49 ±0.52 & 22978 & 3.37 ±0.19 \\
  & 1.6<z_c<2.1 & 14.78 ±0.21 & 2.06 ±0.05 & 14.78 ±0.22 & 18931 & 4.65 ±0.23 \\
  \bottomrule
  \end{array} $%
  \caption{The best-fit values of the parameters of the real-space correlation function $ξ(r)$ for the light-cone at different (1) mass thresholds and (2) redshift ranges. For each sample we quote (3) the correlation length $r_{0}$, (4) slope $\gamma$, (5) correlation length $r_{0}$ at fixed slope $\gamma=2.0$, (6) number of clusters $N_{clusters}$ and (7) the bias $b$ obtained.}
  \label{table:clustering_with_mass}
\end{table}

\end{document}

在此处输入图片描述

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