![双列文档中的 sidewaystable* - emulateapj](https://linux22.com/image/262480/%E5%8F%8C%E5%88%97%E6%96%87%E6%A1%A3%E4%B8%AD%E7%9A%84%20sidewaystable*%20-%20emulateapj%20.png)
我有一个大表格,想要在文档中横向显示emulateapj
,但得到了一个奇怪的结果:
\documentclass[]{emulateapj}
\usepackage{amsmath}
\usepackage{amssymb}
\usepackage{booktabs}
\let\captionbox\relax
\usepackage[
font = small,
labelfont = bf,
labelformat = simple,
labelsep = period,
margin = 0.25in,
]{caption}
\usepackage{longtable}
\usepackage{natbib}
\usepackage{paralist}
\usepackage{rotating}
\setlength{\rotFPtop}{0pt plus 1fil}
\usepackage[referable]{threeparttablex}
\newcommand{\fns}{}
\begin{document}
\makeatletter
\renewcommand\p@enumii{} % make \ref display only innermost label of nested list
\makeatother
%\begin{table*}
\begin{sidewaystable*}
\begin{ThreePartTable}
\begin{TableNotes} \footnotesize
\item[\dag] \label{Tbl:Src:Note:halo} The radio source is coincident with the cluster RH.
\item[\ddag] \label{Tbl:Src:Note:edge} The radio source might be coincident with the cluster RH (edge of diffuse emission).
\end{TableNotes}
\begin{longtable}{cccccccc}
\caption{Radio sources analyzed in previous work\label{Tbl:Src}} \\
\toprule
{\fns(\ref{Tbl:Src:GC})} & {\fns(\ref{Tbl:Src:Name})} & {\fns(\ref{Tbl:Src:Morph})} & {\fns(\ref{Tbl:Src:FR})}
& {\fns(\ref{Tbl:Src:Class})} & {\fns(\ref{Tbl:Src:b})} & {\fns(\ref{Tbl:Src:LOS})} & {\fns(\ref{Tbl:Src:Ref})} \\
Cluster & Source & Morph. & FR & Class & $r_{\bot}/r_c$ & LOS & Ref. \\
\midrule
\endfirsthead
\caption*{\tablename\ \thetable\ -- \textit{Continued from previous page}} \\
\toprule
{\fns(\ref{Tbl:Src:GC})} & {\fns(\ref{Tbl:Src:Name})} & {\fns(\ref{Tbl:Src:Morph})} & {\fns(\ref{Tbl:Src:FR})}
& {\fns(\ref{Tbl:Src:Class})} & {\fns(\ref{Tbl:Src:b})} & {\fns(\ref{Tbl:Src:LOS})} & {\fns(\ref{Tbl:Src:Ref})} \\
Cluster & Source & Morph. & FR & Class & $r_{\bot}/r_c$ & LOS & Ref. \\
\midrule
\endhead
\bottomrule
\endfoot
\bottomrule
\insertTableNotes\\
\captionsetup{position=bottom}
\caption*{\fns
\textbf{Notes.}
The radio sources for which RM maps have been derived and analyzed in previous works, along with some of their relevant characteristics. In this work we analyzed the sources in Coma, A2065, A2142, A2199, and Ophiuchus (italicized).
\begin{inparaenum}[(1)]
\item \label{Tbl:Src:GC} Host GC name;
\item \label{Tbl:Src:Name} Source name;
\item \label{Tbl:Src:Morph} Radio morphology: (H)T = (Head) Tail, (N/W)AT = (Narrow/Wide) Angle Tail;
\item \label{Tbl:Src:FR} Fanaroff-Riley classification;
\item \label{Tbl:Src:Class} Source object type;
\item \label{Tbl:Src:b} Impact parameter relative to X-ray center;
\item \label{Tbl:Src:LOS} Line of sight position: $\infty$ = background source, $0$ = cluster member;
\item \label{Tbl:Src:Ref} RM reference:
\begin{inparaenum}[1.]
\item \label{Tbl:Src:Ref:Bonafede2010} \citealt{Bonafede2010};
\item \label{Tbl:Src:Ref:Eilek2002} \citealt{Eilek2002};
\item \label{Tbl:Src:Ref:Feretti1999} \citealt{Feretti1999};
\item \label{Tbl:Src:Ref:Govoni2001} \citealt{Govoni2001};
\item \label{Tbl:Src:Ref:Govoni2006} \citealt{Govoni2006};
\item \label{Tbl:Src:Ref:Govoni2010} \citealt{Govoni2010};
\item \label{Tbl:Src:Ref:Guidetti2008} \citealt{Guidetti2008};
\item \label{Tbl:Src:Ref:Perley1991} \citealt{Perley1991};
\item \label{Tbl:Src:Ref:Pizzo2011} \citealt{Pizzo2011};
\item \label{Tbl:Src:Ref:Taylor1993} \citealt{Taylor1993};
\item \label{Tbl:Src:Ref:Taylor2001} \citealt{Taylor2001};
\item \label{Tbl:Src:Ref:Taylor2002} \citealt{Taylor2002};
\item \label{Tbl:Src:Ref:Vacca2010} \citealt{Vacca2010};
\item \label{Tbl:Src:Ref:Vacca2012} \citealt{Vacca2012}.
\end{inparaenum}
\end{inparaenum}
}
\endlastfoot
3C 129 & 3C 129 & HT & & galaxy & 1.73 & $0$ & \ref{Tbl:Src:Ref:Taylor2001} \\
& 3C 129.1 & & I & galaxy & 0.01 & $0$ & \ref{Tbl:Src:Ref:Taylor2001} \\
A0119 & 0053-015 & NAT & & E & 0.15 & $0$ & \ref{Tbl:Src:Ref:Feretti1999} \\
& 0053-016 & NAT & & galaxy & 0.90 & $0$ & \ref{Tbl:Src:Ref:Feretti1999} \\
& 3C 029 & & I & S & 2.83 & $0$ & \ref{Tbl:Src:Ref:Feretti1999} \\
A0400 & 3C 075 & T & & E0 & 0.24 & $0$ & \ref{Tbl:Src:Ref:Eilek2002} \\
A0401 & A401A & NAT & & galaxy & 2.93 & $0$ & \ref{Tbl:Src:Ref:Govoni2010} \\
& A401B & HT & & galaxy & 4.20 & $0$ & \ref{Tbl:Src:Ref:Govoni2010} \\
A0514 & A514A & & II & & 2.63 & $\infty$ & \ref{Tbl:Src:Ref:Govoni2001} \\
& A514B2 & NAT & & D & 1.48 & $0$ & \ref{Tbl:Src:Ref:Govoni2001} \\
& A514C & & II & & 4.53 & $\infty$ & \ref{Tbl:Src:Ref:Govoni2001} \\
& A514D & T & I & galaxy & 2.71 & $0$ & \ref{Tbl:Src:Ref:Govoni2001} \\
& A514E & & & QSO & 5.32 & $\infty$ & \ref{Tbl:Src:Ref:Govoni2001} \\
Hydra A & Hydra A & & & galaxy & 20.0 & $0$ & \ref{Tbl:Src:Ref:Taylor1993} \\
\textit{Coma} & 5C 04.042 & & II & galaxy & 5.77 & $\infty$ & \ref{Tbl:Src:Ref:Bonafede2010} \\
& 5C 04.074\tnotex{Tbl:Src:Note:edge}
& & II & & 1.95 & $\infty$ & \ref{Tbl:Src:Ref:Bonafede2010} \\
& 5C 04.081\tnotex{Tbl:Src:Note:halo}
& NAT & I & cD & 0.87 & $0$ & \ref{Tbl:Src:Ref:Bonafede2010} \\
& 5C 04.085\tnotex{Tbl:Src:Note:halo}
& WAT & I-II & cD & 0.40 & $0$ & \ref{Tbl:Src:Ref:Bonafede2010} \\
& 5C 04.114\tnotex{Tbl:Src:Note:edge}
& & I & & 2.04 & $\infty$ & \ref{Tbl:Src:Ref:Bonafede2010} \\
& 5C 04.127 & & & QSO & 3.66 & $\infty$ & \ref{Tbl:Src:Ref:Bonafede2010} \\
& 5C 04.152 & & II & galaxy & 6.68 & $\infty$ & \ref{Tbl:Src:Ref:Bonafede2010} \\
\textit{A2065} & A2065A & & II & galaxy & 1.96 & $\infty$ & \ref{Tbl:Src:Ref:Govoni2010} \\
\textit{A2142} & A2142A & HT & I & galaxy & 2.66 & $0$ & \ref{Tbl:Src:Ref:Govoni2010} \\
\textit{A2199} & 3C 338 & & I & cD2 & 0.05 & $\infty$ & \ref{Tbl:Src:Ref:Vacca2012} \\
A2255 & Double\tnotex{Tbl:Src:Note:edge}
& HT & & galaxy & 2.98 & & \ref{Tbl:Src:Ref:Pizzo2011} \\
& Goldfish\tnotex{Tbl:Src:Note:halo}
& NAT & & galaxy & 1.72 & & \ref{Tbl:Src:Ref:Pizzo2011} \\
& TRG\tnotex{Tbl:Src:Note:halo}
& NAT & & galaxy & 1.03 & & \ref{Tbl:Src:Ref:Pizzo2011} \\
& Bean & HT & & galaxy & 11.6 & & \ref{Tbl:Src:Ref:Pizzo2011} \\
& Embryo & WAT & & & 7.93 & & \ref{Tbl:Src:Ref:Pizzo2011} \\
& Beaver & NAT & & galaxy & 4.33 & & \ref{Tbl:Src:Ref:Pizzo2011} \\
& F1, F2, F3\tnotex{Tbl:Src:Note:halo}
& & & filaments & & & \ref{Tbl:Src:Ref:Pizzo2011} \\
& J1712.4+6401\tnotex{Tbl:Src:Note:halo}
& & & & 0.78 & & \ref{Tbl:Src:Ref:Govoni2006} \\
& J1713.3+6347 & & & & 4.35 & & \ref{Tbl:Src:Ref:Govoni2006} \\
& J1713.5+6402\tnotex{Tbl:Src:Note:edge}
& & & & 3.05 & & \ref{Tbl:Src:Ref:Govoni2006} \\
& J1715.1+6402 & & & & 8.14 & & \ref{Tbl:Src:Ref:Govoni2006} \\
A2382 & PKS 2149-158 A & & I & E & 0.44 & $0$ & \ref{Tbl:Src:Ref:Guidetti2008} \\
& PKS 2149-158 B & & I & E & 0.41 & $0$ & \ref{Tbl:Src:Ref:Guidetti2008} \\
& PKS 2149-158 C & & I & E & 0.15 & $0$ & \ref{Tbl:Src:Ref:Guidetti2008} \\
A2634 & 3C 465 & T & I & cD & 0.39 & $0$ & \ref{Tbl:Src:Ref:Eilek2002} \\
Centaurus & PKS 1246-410 & & I & cD1 & 0.34 & $0$ & \ref{Tbl:Src:Ref:Taylor2002} \\
\textit{Ophiuchus} & OPHIB & HT & I & galaxy & 2.50 & $0$ & \ref{Tbl:Src:Ref:Govoni2010} \\
\end{longtable}
\end{ThreePartTable}
\end{sidewaystable*}
%\end{table*}
\end{document}
序言中加载软件包后的行rotating
取自这里。 我怎样才能解决这个问题?