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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 new file mode 100644 index 00000000000..48de5c0e93b --- /dev/null +++ b/Master/texmf-dist/doc/latex/elsevier/instructions-num.tex @@ -0,0 +1,774 @@ +\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} |