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diff --git a/Master/texmf-dist/doc/latex/elsevier/instructions-num.tex b/Master/texmf-dist/doc/latex/elsevier/instructions-num.tex deleted file mode 100644 index 48de5c0e93b..00000000000 --- a/Master/texmf-dist/doc/latex/elsevier/instructions-num.tex +++ /dev/null @@ -1,774 +0,0 @@ -\documentclass{elsart} -\usepackage{ifpdf} -\usepackage{graphicx,amssymb,lineno} -\ifpdf -\usepackage[% - pdftitle={Instructions for use of the document class - elsart},% - pdfauthor={Simon Pepping},% - pdfsubject={The preprint document class elsart},% - pdfkeywords={instructions for use, elsart, document class},% - pdfstartview=FitH,% - bookmarks=true,% - bookmarksopen=true,% - breaklinks=true,% - colorlinks=true,% - linkcolor=blue,anchorcolor=blue,% - citecolor=blue,filecolor=blue,% - menucolor=blue,pagecolor=blue,% - urlcolor=blue]{hyperref} -\else -\usepackage[% - breaklinks=true,% - colorlinks=true,% - linkcolor=blue,anchorcolor=blue,% - citecolor=blue,filecolor=blue,% - menucolor=blue,pagecolor=blue,% - urlcolor=blue]{hyperref} -\fi - -\renewcommand\floatpagefraction{.2} -\makeatletter -\def\elsartstyle{% - \def\normalsize{\@setfontsize\normalsize\@xiipt{14.5}} - \def\small{\@setfontsize\small\@xipt{13.6}} - \let\footnotesize=\small - \def\large{\@setfontsize\large\@xivpt{18}} - \def\Large{\@setfontsize\Large\@xviipt{22}} - \skip\@mpfootins = 18\p@ \@plus 2\p@ - \normalsize -} -\@ifundefined{square}{}{\let\Box\square} -\makeatother - -\def\file#1{\texttt{#1}} - -\pagestyle{plain} -\begin{document} - -\begin{frontmatter} -\title{Instructions for use\\of the document class \file{elsart}} - -\author{Simon Pepping} -\address{Elsevier, P.O. Box 103, 1000 AC Amsterdam, -Netherlands} - -\ead{s.pepping@elsevier.com} -\ead[url]{authors.elsevier.com/locate/latex} - -\begin{abstract} -This article discusses several features of preparing articles -with the \file{elsart} document style, using numbered style bibliographic -references. -\end{abstract} - -\begin{keyword} -\file{elsart}, document class, instructions for use -\PACS 01.30.$-$y -\end{keyword} -\end{frontmatter} - -\section{Introduction} -\label{intro} - -This article discusses how to prepare articles with the \file{elsart} -document class. For more general information about \LaTeX{}, see the -\LaTeX{} manual written by Lamport \cite{Lamp86}. - -Elsevier has prepared the following \LaTeX{} support files for -authors: -\begin{itemize} -\item The document class \file{elsart.cls}, which provides a preprint - layout. -\item The document classes \file{elsart1p.cls}, \file{elsart3p.cls}, - \file{elsart5p.cls}, which each provide a layout in one of - Elsevier's standard journal styles, called 1+, 3+ and 5+. -\item The instructions for use of \file{elsart}, - \file{instructions-harv} for use with a Harvard-style bibliography, - and \file{instructions-num} for use with a numbered style - bibliography. -\item Template files for a quick start of your \LaTeX{} article with - \file{elsart}, - \newline - \file{template-harv.tex} for use with a Harvard-style - bibliography, and - \newline - \file{template-num.tex} for use with a numbered - style bibliography. -\item Styles for BibTeX, \file{elsart-harv.bst} for a Harvard-style - bibliography, and \file{elsart-num.bst} for a numbered style - bibliography. -\end{itemize} -The files are freely available from Elsevier's Author Gateway -\url{http://authors.elsevier.com/locate/latex}. - -On Elsevier's Author Gateway you will also find support files for CRC -journal articles. Support for monographs or contributed book chapters -may be obtained via the publisher of the book. - -Elsevier's \LaTeX{} support files can also be obtained from one of the -servers of the Comprehensive TeX Archive Network (CTAN) in the -directory\newline -\href{ftp://ctan.tug.org/tex-archive/macros/latex/contrib/supported/elsevier}% -{\texttt{/tex-archive/macros/latex/contrib/supported/elsevier}}. CTAN is a -mirrored network of FTP servers, with the following web front ends: -\href{http://www.tex.ac.uk}{\texttt{www.tex.ac.uk}}, -\href{http://www.dante.de/software/ctan}{\texttt{www.dante.de/software/ctan}} -(in German) and \href{http://www.ctan.org}{\texttt{www.ctan.org}}. The -network is widely mirrored, see -\url{http://www.tug.org/tex-archive/CTAN.sites}. It holds up-to-date -copies of all the public-domain versions of \TeX, \LaTeX, Metafont and -ancillary programs. - -Note that CTAN is not related to Elsevier, and that Elsevier's author -support cannot accept complaints or answer questions about the -availability of any CTAN server. - -The non-Elsevier macro packages recommended later in this document and -many other useful macro packages can also be obtained from CTAN. - -In the following sections we show how you may use the \file{elsart} -document class. - -\section{Options} - -The \file{elsart} document class enables the following options: - -\begin{description} - -\item[doublespacing, reviewcopy] This is a single option with two - names to obtain double line spacing, as is sometimes required for - copies submitted for review. - -\item[seceqn, secthm] The option \texttt{seceqn} numbers the equation - environments per section. The option \texttt{secthm} does the same - for the \texttt{thm} environment. In elsart all predefined theorem - environments except Algorithm, Note, Summary and Case use the same - counter as the \texttt{thm} environment. - -\item[draft, final] As in many other document classes, these are - options to produce draft and final layout. In the draft layout you - will see warnings for overfull boxes. You also need draft layout to - test your formulas on a narrower display width, see option - \texttt{narrowdisplay}. - -\item[narrowdisplay] Many Elsevier journals print their text in two - columns. Because the preprint layout uses a larger line width - than such columns, the formulas are too wide for the line width in - print. In draft mode (see the \texttt{draft} option) you can use the - \texttt{narrowdisplay} option to force a narrower width for - displayed formulas. The width is roughly equal to the column width - of the printed journals, compensated for the larger font size of the - preprint layout. The \texttt{narrowdisplay} option is ineffective - with packages which redefine the equation environments, such as - \texttt{amsmath}. - - The \texttt{narrowdisplay} option is especially useful for journals - for which the articles are printed from the author's \LaTeX{} file. - This is the case for a number of mathematics journals. When you - break your formulas such that they fit in the narrow column width, - the typesetter will be able to retain most of your breaks. Article - for other journals are printed after transformation to an XML file. - For such journals the formula layout in the \LaTeX{} file is always - lost in the transformation. - - The narrow display width is obtained by giving the formulas a larger - indent. Too wide formulas in the one-line display environments - \texttt{equation} and \texttt{displaymath} will show an overfull - rule: - - \def\testformula{% - \sum_{i=0}^{\infty}A^n\int \mathrm{d}x\, \frac{F_n(x)}{A_n + B_n} = - B^n C^n \int\mathrm{d}x\,\int \mathrm{d}y\, - \frac{G_n(x,y)}{\mathcal{A}_n{x} + \mathcal{B}_n{y}} - } - \overfullrule 5pt - \mathindent\linewidth\relax - \advance\mathindent-259pt - \begin{equation} - \label{eq:1} - \testformula. - \end{equation} - - This is not the case for the multiline display environment - \texttt{eqnarray}. But in both cases too wide formulas will extend - into the right margin, giving you visual feedback: - - \begin{eqnarray} - \label{eq:2} - \testformula,\nonumber\\ - \testformula. - \end{eqnarray} - - When you switch off draft mode, the formulas will have their normal - indentation, and too wide formulas will no longer be signalled. - -\end{description} - -\section{Print layout} -\label{printlayout} - -Elsevier also makes available a few document classes that roughly -reproduce the layout of the printed journals. The majority of Elsevier -journals use one of a small set of standard layouts. We have document -classes for three of those layouts: - -\begin{description} -\item[elsart1p] text width 32 picas (134 mm), text height 47 lines, - one column. -\item[elsart3p] text width 39 picas (164 mm), text height 51 lines, - one or two columns. -\item[elsart5p] text width 43.5 picas (183 mm), text height 57 lines, - two columns. -\end{description} - -These classes can be used in the same way as elsart. If you prepared -an article for elsart, you can run it with one of these print layout -classes without changes to the markup. In fact, they use elsart and -you must have elsart on your system as well. - -Note that the layout is only roughly the same as that of the printed -journal. One major source of differences is the font. The printer uses -a different font with different character widths, which will cause -deviations in layout. There are various other sources of small -differences. You cannot use the layout of one of these classes to make -claims on the final layout of your article. - -\section{Frontmatter} -\label{frontmatter} - -The \texttt{elsart} document class has a separate -\texttt{frontmatter} environment for the title, authors, addresses, -abstract and keywords. -\begin{itemize} -\item \verb|\title|: As in standard \LaTeX, e.g. -\verb|\title{Model}|. -\item \verb|\author|: Different from standard \LaTeX, the \verb|\author| -command contains only one author and no address. -Multiple authors go into multiple \verb|\author| commands, -separated from each other by commas. -The address goes into a separate -\verb|\address| command. -Example: \verb|\author{D.E. Knuth}|. -\item \verb|\address|: Here goes the address, e.g. -\verb|\address{CERN, Geneva}|. -\item \verb|\thanks| and \verb|\thanksref|: -These provide footnotes to the title, authors and addresses. -The \verb|\thanksref| command takes a label: \verb|\thanksref{label}| -to relate it to the \verb|\thanks| command with -the same label: \verb|\thanks[label]|. There can be several -references to a single \verb|\thanks| command. Example:\\ -\verb|\title{Model\thanksref{titlefn}}| and\\ -\verb|\thanks[titlefn]{Supported by grants.}| -\item \verb|\corauth| and \verb|\corauthref|: -These provide footnotes to mark the corresponding author and the -correspondence address. They are used in the same manner as -\verb|\thanks| and \verb|\thanksref|. Example:\\ -\verb|\author{A. Name\corauthref{cor}}| and\\ -\verb|\corauth[cor]{Corresponding author. Address: ... .}| -\item \verb|\ead|: -This command should be used for the email address or the URL of the -author. It refers to the `current author', i.e., the author last -mentioned before the command. -When it holds a URL, this should be indicated by setting the -optional argument to `url'. Example: -\verb|\ead{s.pepping@elsevier.com}|, -\verb|\ead[url]{authors.elsevier.com/locate/latex}|. -\end{itemize} - -It is not necessary to give a \verb|\maketitle| command. The title, -authors and addresses are printed as soon as \TeX{} sees them. - -The authors and addresses can be combined in one of two ways: -\begin{itemize} -\item The simplest way lists the authors of one address or one group - of addresses, followed by the address or addresses, and so on for - all addresses or groups of addresses. -\item The other way first lists all authors, and then all addresses. -The authors and addresses are related to each other by labels: -\verb|\author[label1]{Name1}| corresponds to -\verb|\address[label1]{Address1}|. Example: -\begin{verbatim} -\author[South]{T.R. Marsh}, -\author[Oxford]{S.R. Duck} -\address[South]{University of Southampton, UK} -\address[Oxford]{University of Oxford, UK} -\end{verbatim} -\end{itemize} - -See the extensive examples in figs. -\ref{ex:explinput}, \ref{ex:exploutput}, -\ref{ex:implinput}, \ref{ex:imploutput}. - -If you put the frontmatter in an included file, that file should -contain the whole frontmatter, including its \texttt{begin} and -\texttt{end} commands. Otherwise, the labels of the frontmatter will -remain undefined. - -%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%ex:explinput%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% - -\begin{figure}[p] - -\caption{Article opening with explicit links (input)} \label{ex:explinput} -\vspace{1pc} - -\begin{verbatim} -\documentclass{elsart} -\usepackage{graphicx,amssymb} -\journal{New Astronomy} -\begin{document} -\begin{frontmatter} - -\title{Stroboscopic Doppler tomography of FO Aqr} -\author[South]{T.R. Marsh\corauthref{cor}}, -\corauth[cor]{Corresponding author.} -\ead{trm@astro.soton.ac.uk} - -\author[Oxford]{S.R. Duck\thanksref{now}} -\thanks[now]{Present address: Systems Engineering and Assessment Ltd., -Beckington Castle, PO Box 800, Bath BA3 6TB, UK.} -\ead{srd@sea.co.uk} - -\address[South]{University of Southampton, Department of Physics, -Highfield, Southampton SO17 1BJ, UK} -\address[Oxford]{University of Oxford, Department of Physics, Nuclear -Physics Laboratory, Keble Road, Oxford, OX1 3RH, UK} - -\begin{abstract} -FO Aqr is a close binary star in -which a magnetic white dwarf accretes from a cool companion. Light -curves and spectra show variations on the orbital frequency, the -white dwarf's spin frequency and combinations of the two. -\end{abstract} -\begin{keyword} -Accretion, accretion disks \sep Line: profiles \sep -Binaries: close \sep Novae, cataclysmic variables -\PACS 97.10.Gz \sep 97.30.Qt \sep 97.80.Gm -\end{keyword} -\end{frontmatter} - -\section{Introduction} -FO Aqr is a member of the DQ~Her class of stars which -are close binary stars in which a magnetic white dwarf accretes from -a late-type main-sequence secondary star. These stars have most -recently been reviewed in Ref. \cite{Patterson94}. -\end{verbatim} - -\end{figure} - -%%%%%%%%%%%%%%%%%%%%%%%%%%%%%ex:exploutput%%%%%%%%%%%%%%%%%%%%%%%%%%%%% - -\begin{figure}[p] -\caption{Article opening with explicit links (output)\label{ex:exploutput}} -\vspace{1pc} - -\begin{minipage}{\textwidth} -\elsartstyle -\parskip 12pt -% -\renewcommand{\thempfootnote}{\fnsymbol{mpfootnote}} -% -\leftskip=2pc -% -\begin{center} -{\LARGE Stroboscopic Doppler tomography of FO Aqr}\\[30pt] -% -\large -T.R. Marsh$^{\mathrm{a},*}$, -S.R. Duck$^{\mathrm{b},1}$\\[12pt] -% -\small\itshape -$^a$University of Southampton, Department of Physics,\\ -Highfield, Southampton SO17 1BJ, UK\\ -$^b$University of Oxford, Department of Physics, Nuclear Physics\\ -Laboratory, Keble Road, Oxford, OX1 3RH, UK - -\end{center} - -\bigskip -\leftskip=0pt - -\hrule\vskip 8pt -\begin{small} -{\bfseries Abstract} -\parindent 1em - -FO Aqr is a close binary star in -which a magnetic white dwarf accretes from a cool companion. Light -curves and spectra show variations on the orbital frequency, the -white dwarf's spin frequency and combinations of the two. - -\noindent\textit{Key words:} -Accretion, accretion disks, Line: profiles, -Binaries: close, Novae, cataclysmic variables\\ -\textit{PACS:} 97.10.Gz, 97.30.Qt, 97.80.Gm -\end{small} -% -\vskip 10pt\hrule - -\leftskip=0pt - -\vspace{24pt} - -\textbf{Introduction} - -FO Aqr is a member of the DQ~Her class of stars which -are close binary stars in which a magnetic white dwarf accretes from -a late-type main-sequence secondary star. These stars have most -recently been reviewed in Ref. [1]. - -\begin{footnotesize} -\leavevmode -\rlap{$^*$}\hspace{1pc}Corresponding author.\\ -\rlap{$^1$}\hspace{1pc}Present address: Systems Engineering and -Assessment Ltd., Beckington Castle, PO Box 800, Bath BA3 6TB, UK.\\ -\rlap{}\hspace{1pc}\textit{Email addresses:} trm@astro.soton.ac.uk -(T.R. Marsh), srd@sea.co.uk (S.R. Duck). -\end{footnotesize} - -\leavevmode\hbox to \hsize{\small\slshape Preprint submitted to New Astronomy -\hfil 21 August 1997} - -\end{minipage} - -\bigskip - -\end{figure} - -%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%ex:implinput%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% - -\begin{figure}[p] -\caption{Article opening with implicit links (input)\label{ex:implinput}} -\vspace{1pc} - -\begin{verbatim} -\documentclass{elsart} - -\begin{document} -\begin{frontmatter} -\title{Integrability in - random matrix models\thanksref{talk}} -\thanks[talk]{Expanded version of a talk - presented at the Singapore Meeting on - Particle Physics (Singapore, August 1990).} - -\author{L. Alvarez-Gaum\'{e}\corauthref{cor}} -\address{Theory Division, CERN, - CH-1211 Geneva 23, Switzerland} -\corauth[cor]{Corresponding author.} -\ead{lag@cern.ch} - -\author{C. Gomez\corauthref{cor}\thanksref{SNSF}} -\address{D\'{e}partment de Physique Th\'{e}orique, - Universit\'{e} de Gen\`{e}ve, - CH-1211 Geneva 4, Switzerland} -\ead{cg@ug.ch} - -\author{J. Lacki} -\address{School of Natural Sciences, - Institute for Advanced Study, - Princeton, NJ 08540, USA} -\ead[url]{www.ias.edu/~jl} -\thanks[SNSF]{Supported by the - Swiss National Science Foundation} - -\begin{abstract} -We prove the equivalence between the recent matrix -model formulation of 2D gravity and lattice -integrable models. For even potentials this -system is the Volterra hierarchy. -\end{abstract} -\end{frontmatter} - -\section{Introduction} -Some aspects of the recently discovered -non-perturbative solutions to non-critical strings -\cite{Patterson94} can be better understood and -clarified directly in terms of the integrability -properties of the random matrix model. -... -\end{verbatim} - -\end{figure} - -%%%%%%%%%%%%%%%%%%%%%%%%%%%%%ex:imploutput%%%%%%%%%%%%%%%%%%%%%%%%%%%%% - -\begin{figure}[p] -\caption{Article opening with implicit links (output)\label{ex:imploutput}} -\vspace{1pc} - -\begin{minipage}{\textwidth} -\elsartstyle -% -\renewcommand{\thempfootnote}{\fnstar{mpfootnote}} -% -\leftskip=2pc -% -\begin{center} -{\LARGE Integrability in random matrix models$^\star$}\\[30pt] -\footnotetext[1]{\upshape Expanded version of a talk presented at the -Singapore Meeting on Particle Physics (Singapore, August 1990).} -% -\large -L. Alvarez-Gaum\'{e}$^*$ \\[6pt] -{\small\itshape Theory Division, CERN, - CH-1211 Geneva 23, Switzerland}\\[18pt] -C. Gomez$^{*,1}$ \\[6pt] -{\small\itshape D\'{e}partment de Physique Th\'{e}orique, - Universit\'{e} de Gen\`{e}ve, - CH-1211 Geneva 4, Switzerland} \\[15pt] -J. Lacki \\[6pt] -{\small\itshape School of Natural Sciences, Institute for Advanced Study, - Princeton, NJ 08540, USA} -% BW: -\end{center} -% -\renewcommand{\thempfootnote}{\astsymbol{mpfootnote}} -\footnotetext[1]{Corresponding author.} -\setbox0=\hbox{\footnotesize 1} -\edef\thempfootnote{\hskip\wd0} -\footnotetext[0]{\textit{Email adresses:} lag@cern.ch - (L. Alvarez-Gaum\'{e}), cg@ug.ch (C. Gomez).} -\footnotetext[1]{\textit{URL:} www.ias.edu/\~{ }jl (J. Lacki).} -\renewcommand{\thempfootnote}{\arabic{mpfootnote}} -\footnotetext[1]{Supported by the Swiss National Science Foundation} - -\bigskip -\leftskip=0pt - -\hrule\vskip 8pt -\begin{small} -{\bfseries Abstract} -\parindent 1em - -We prove the equivalence between the recent matrix model -formulation of 2D gravity and lattice integrable models. For even -potentials this system is the Volterra hierarchy.\par -\end{small} -\vskip 10pt\hrule - -\medskip - -\section*{1. Introduction} - -Some aspects of the recently discovered non-perturbative -solutions to non-critical strings [1] can be better -understood and clarified directly in terms of the -integrability properties of the random matrix model. - -... -\end{minipage} - -\bigskip - -\end{figure} - -%%%%%%%%%%%%%%%%%%%%%%%%%%%% end of figures %%%%%%%%%%%%%%%%%%%%%%%%%%%% - -\section{Abstract} - -The abstract should be self-contained. Therefore, do not refer to the -list of references. Instead, quote the reference in full, as follows: -Wettig \& Brown (1996, NewA, 1, 17). - -\section{Keywords} -\label{keywd} -\enlargethispage*{2.5pc} - -In electronic publications a proper classification is more important -than ever. Elsevier's physics journals use several keyword -schemes:\ - -\begin{description} -\item[Keywords:] Uncontrolled keywords. -\item[PACS:] The PACS scheme, developed and maintained by the AIP, -covers the whole field of Physics. -See \url{http://www.aip.org/pacs/pacs.html} -or \url{http://www.elsevier.com/locate/pacs}. -\item[MSC:] The MSC scheme, developed and maintained by the AMS, -covers the whole field of Mathematics. -See \url{http://www.ams.org/msc} -or \url{http://www.elsevier.com/locate/msc}. -\end{description} - -Keywords are entered below the abstract in the following way: -\pagebreak[4] -\begin{verbatim} -\begin{keyword} -Keyword \sep Keyword -\PACS PACS code \sep PACS code -\MSC MSC code \sep MSC code -\end{keyword} -\end{verbatim} - -\section{Cross-references} -\label{xrefs} - -In electronic publications articles may be internally hyperlinked. -Hyperlinks are generated from proper cross-references in the article. - -For example, the words Fig. 1 will never be more than simple text, -whereas the proper cross-reference \verb|\ref{mapfigure}| may be -turned into a hyperlink to the figure itself. - -In the same way, the words Ref. [1] will fail to -turn into a hyperlink; the proper cross-reference is -\verb|\cite{Gea97}|. - -Cross-referencing is possible in \LaTeX{} for sections, subsections, -formulae, figures, tables, and literature references. - -\section{PostScript figures} -\label{psfigs} - -\LaTeX{} and PostScript have had a long and successful relationship. -There are three packages for including PostScript figures: -\begin{itemize} -\item \texttt{graphics}. -This simple package provides the command\\ -\verb|\includegraphics*[<llx,lly>][<urx,ury>]{file}|. -The \texttt{*} is optional; it enables the PostScript feature of clipping. -In its simplest form,\\ -\verb|\includegraphics{file}|, -it includes the figure in the PostScript file \texttt{file} -without resizing. -\item \texttt{graphicx}. -This package provides the command\\ -\verb|\includegraphics*[key--value list]{file}|. -The \texttt{*} is optional; it enables the PostScript feature of clipping. -Often used keys are: -\def\labelitemii{--} -\begin{itemize} -\item \texttt{scale=.40} to scale the size of the figure with 40\%, -\item \texttt{width=25pc}, \texttt{height=15pc} to set the width or -height of the figure, -\item \texttt{angle=90} to rotate the figure over $90^\circ$. -\end{itemize} -\item \texttt{epsfig}. -This package is really the \texttt{graphicx} package, -but it allows one to include PostScript figures using -the familiar commands from -the earlier packages \texttt{epsfig} and \texttt{psfig}. -\end{itemize} -For detailed information, see the documentation of the \texttt{graphics} -packages, in particular the file \texttt{grfguide.tex}. -\begin{figure} -\leftmargin=2pc -\begin{verbatim} -\begin{figure} -\begin{center} -\includegraphics*[width=5cm]{name.eps} -\end{center} -\caption{An example of a figure.} -\label{fig:exmp} -\end{figure} -\end{verbatim} -\caption{An example of a figure.} -\label{fig:exmp} -\end{figure} - -\section{Mathematical symbols} -\label{symbols} - -Many physics authors require more mathematical symbols than the -few that are provided in standard \LaTeX. A useful package for -additional symbols is the \texttt{amssymb} package, developed by the American -Mathematical Society. This package includes such oft used symbols as -\verb|\lesssim| for $\lesssim$, \verb|\gtrsim| for $\gtrsim$ or -\verb|\hbar| for $\hbar$. Note that your \TeX{} system should have -the \texttt{msam} and \texttt{msbm} fonts installed. -If you need only a few symbols, such as \verb|\Box| for $\Box$, -you might try the package \texttt{latexsym}. - -In the \texttt{elsart} document class vectors are preferably coded as -\verb|\vec{a}| instead of \verb|\bf{a}| or \verb|\pol{a}|. - -\section{Line numbering} -\label{linenumbering} - -\begin{linenumbers} -Reviewing an electronic version of an article has many -advantages. However, reviewers have a harder task indicating remarks -and desired changes to the article. Their task is made easier if the -lines of the article are numbered. \LaTeX's \texttt{lineno} package -performs this task. It is compatible with \texttt{elsart}. -\end{linenumbers} - -\section{The Bibliography} -\label{thebib} - -In \LaTeX{} literature references are listed in the -\verb|thebibliography| environment. Each reference is a -\verb|\bibitem|; each \verb|\bibitem| is identified by a label, by -which it can be cited in the text: \verb|\bibitem{ESG96}| is cited as -\verb|\cite{ESG96}|. - -Version 2.16 of \texttt{elsart} introduces the \texttt{subbibitems} -environment. The references in a \texttt{subbibitems} environment -have the same major reference number, and are counted by letters -a, b, etc. The \texttt{subbibitems} environment has -a label of its own: \verb|\begin{subbibitems}{label}|. -It can therefore be referred to as \verb|\cite{label}|, which produces -a citation like [7a--c]. A short citation like [7] can be produced by -adding \texttt{:s} to the label: \verb|\cite{label:s}|. Example: See -Refs. \cite{Lee}, or in short form, see Refs. \cite{Lee:s}. - -Version 2.16 of \texttt{elsart} also introduces the possibility to -insert notes into the bibliography, by using the \verb|\note| command. -In a \texttt{subbibitems} environment it must be the last item. -Example: See Refs. \cite{note,x}. - -These options do not work well with the \texttt{natbib} package. - -\section{Template article} -\label{templart} - -There is a template article \file{templat-num.tex}, which you can use as a -skeleton for your own article. It is available from Elsevier's Author -Gateway, \url{http://authors.elsevier.com/locate/latex}. - -\begin{thebibliography}{9} - -\bibitem{Lamp86} -Leslie Lamport: \LaTeX, {\em A document preparation system}, -2nd edition, Addison-Wesley (Reading, Massachusetts, 1994). - -\bibitem{WB96} -Wettig, T., \& Brown, G.E., -The evolution of relativistic binary pulsars, -1996, NewA, 1, 17-34. - -\bibitem{ESG96} -Elson, R.A.W., Santiago, B.X., \& Gilmore, G.F., -Halo stars, starbursts, and distant globular clusters: -A survey of unresolved objects in the Hubble Deep Field, -1996, NewA, 1, 1-16. -% (\url{http://www.elsevier.com/PII/S1384107696000061}) - -\bibitem{Gea97} -Governato, F., Moore, B., Cen, R., Stadel, J., Lake, G., \& Quinn, T., -The Local Group as a test of cosmological models, -1997, NewA 2, 91-106. - -\bibitem{note}% - \note We consider an exactly solvable two-band model of electrons moving in -one dimension and interacting with a $\delta$-function spin-exchange -potential. - -\begin{subbibitems}{Lee} -\bibitem{Lee:a} N.~Nagaosa and P.~A.~Lee, Phys. Rev. Lett. {\bf 79}, 3755 -(1997). -\bibitem{Lee:b}C.~P\'epin and P.~A.~Lee, Phys. Rev. Lett. {\bf 81}, - 2779 (1998). -\end{subbibitems} - -\bibitem{x} K.~Gorny, O.~M.~Vyasilev, -J.~A.~Marindale, V.~A.~Nandor, C.~H.~Pennington, P.~C.~Hammel, -W.~L.~Hults, J.~L.~Smith, P.~L.~Kuhns, A.~P.~Reyes and W.~G.~Moulton, -Phys. Rev. Lett. {\bf 82}, 177 (1999). -\note These references demonstrate that for some high-$T_c$ compounds -the gap does not seem to depend on the magnetic field. - -\end{thebibliography} - -\end{document} |