The binarity of Galactic dwarf stars along with effective temperature and metallicity

TL;DR

This study investigates the relationship between binary star fraction, effective temperature, and metallicity in Galactic dwarf stars using LAMOST data, revealing a correlation between binarity and stellar properties.

Contribution

It provides a detailed analysis of binary fraction dependence on Teff and [Fe/H] using a large spectroscopic dataset, highlighting the influence of metallicity and temperature.

Findings

A-type stars are more likely to be in binary systems.

An inverse correlation exists between binary fraction and metallicity.

Metal-rich, cooler stars have the most accurate radial velocity measurements.

Abstract

The fraction of binary stars (fb) is one of most valuable tool to probe the star formation and evolution of multiple systems in the Galaxy. We focus on the relationship between fb and stellar metallicity ([Fe/H]) by employing the differential radial velocity (DRV) method and the large sample observed by the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST). Main-sequence stars from A- to K-types in the third data release (DR3) of LAMOST are selected to estimate fb. Contributions to a profile of DRV from radial velocity (RV) error of single stars (\sigma) and orbital motion of binary stars are evaluated from the profile of DRV. Finally, we employ 365,911 stars with randomly repeating spectral observations to present a detailed analysis of fb and \sigma in the two-dimensional (2D) space of Teff and [Fe/H]. The A-type stars are more likely to be companions in binary star systems than other stars. Furthermore, the reverse correlation between fb and [Fe/H] can be shown statistically, which suggests that fb is a joint function of Teff and [Fe/H]. At the same time, \sigma of the sample for different Teff and [Fe/H] are fitted. Metal-rich cold stars in our sample have the best RV measurement.

Tables

Table 1. Table 1: Additional commands for special symbols commonly used in astronomy. These can be used anywhere.

Command	Output	Meaning
\sun	☉	Sun, solar
\earth	⊕	Earth, terrestrial
\micron	µm	microns
\degr	°	degrees
\arcmin	′	arcminutes
\arcsec	″	arcseconds
\fdg	$\stackrel{\circ }{.}$	fraction of a degree
\farcm	$\stackrel{\prime }{.}$	fraction of an arcminute
\farcs	$\stackrel{\prime \prime }{.}$	fraction of an arcsecond
\fd	$\stackrel{d}{.}$	fraction of a day
\fh	$\stackrel{h}{.}$	fraction of an hour
\fm	$\stackrel{m}{.}$	fraction of a minute
\fs	$\stackrel{s}{.}$	fraction of a second
\fp	$\stackrel{p}{.}$	fraction of a period
\diameter	⌀	diameter
\sq	\sq	square, Q.E.D.

Table 2. Table 2: Additional commands for mathematical symbols. These can only be used in maths mode.

Command	Output	Meaning
\upi	$\pi$	upright pi
\umu	$\mu$	upright mu
\upartial	$\partial$	upright partial derivative
\lid	$\leqq$	less than or equal to
\gid	$\geqq$	greater than or equal to
\la	$\lesssim$	less than of order
\ga	$\gtrsim$	greater than of order
\loa	$⪅$	less than approximately
\goa	$⪆$	greater than approximately
\cor	$\stackrel{\frown}{=}$	corresponds to
\sol	$⪝$	similar to or less than
\sog	$⪞$	similar to or greater than
\lse	$⪍$	less than or homotopic to
\gse	$⪎$	greater than or homotopic to
\getsto	$\leftrightarrows$	from over to
\grole	$\gtrless$	greater over less
\leogr	$\lessgtr$	less over greater

Table 3. Table 3: An example table.

Star	Mass	Luminosity
	$M_{☉}$	$L_{☉}$
Sun	1.00	1.00
$\alpha$ Cen A	1.10	1.52
$ϵ$ Eri	0.82	0.34

Table 4. Table 5: An example landscape table.

Header	Header	Header	Header	Header	Header	Header	Header	Header	Header
Unit	Unit	Unit	Unit	Unit	Unit	Unit	Unit	Unit	Unit
Data	Data	Data	Data	Data	Data	Data	Data	Data	Data
Data	Data	Data	Data	Data	Data	Data	Data	Data	Data
Data	Data	Data	Data	Data	Data	Data	Data	Data	Data
Data	Data	Data	Data	Data	Data	Data	Data	Data	Data
Data	Data	Data	Data	Data	Data	Data	Data	Data	Data
Data	Data	Data	Data	Data	Data	Data	Data	Data	Data
Data	Data	Data	Data	Data	Data	Data	Data	Data	Data
Data	Data	Data	Data	Data	Data	Data	Data	Data	Data

Table 5. Table 6: Common citation commands, provided by the natbib package.

Command	Ouput	Note
\citet{key}	Smith (2014)
\citep{key}	(Smith, 2014)
\citep{key,key2}	(Smith, 2014; Jones, 2015)	Multiple papers
\citet[table 4]{key}	Smith (2014, table 4)
\citep[see][figure 7]{key}	(see Smith, 2014, figure 7)
\citealt{key}	Smith 2014	For use with manual brackets
\citeauthor{key}	Smith	If already cited in close proximity
\defcitealias{key}{Paper~I}		Define an alias (doesn’t work in floats)
\citetalias{key}	Paper I
\citepalias{key}	(Paper I)

Table 6. Table 7: Commands for abbreviated journal names, see appendix  A .

Command	Output	Journal name
\aap or \astap	A&A	Astronomy and Astrophysicsa
\aapr	A&ARv	The Astronomy and Astrophysics Review
\aaps	A&AS	Astronomy and Astrophysics Supplement Series
\actaa	Acta Astron.	Acta Astronomica
\afz	Afz	Astrofizika
\aj	AJ	The Astronomical Journal
\ao or \applopt	Appl. Opt.	Applied Optics
\aplett	Astrophys. Lett.	Astrophysics Letters
\apj	ApJ	The Astrophysical Journal
\apjl or \apjlett	ApJ	The Astrophysical Journal Lettersa
\apjs or \apjsupp	ApJS	The Astrophysical Journal Supplement Series
\apss	Ap&SS	Astrophysics and Space Science
\araa	ARA&A	Annual Review of Astronomy and Astrophysics
\arep	Astron. Rep.	Astronomy Reportsb
\aspc	ASP Conf. Ser.	Astronomical Society of the Pacific Conference Series
\azh	Azh	Astronomicheskii Zhurnalc
\baas	BAAS	Bulletin of the American Astronomical Society
\bac	Bull. Astron. Inst. Czechoslovakia	Bulletin of the Astronomical Institutes of Czechoslovakia
\bain	Bull. Astron. Inst. Netherlands	Bull. Astron. Inst. Netherlands
\caa	Chinese Astron. Astrophys.	Chinese Astronomy and Astrophysics
\cjaa	Chinese J. Astron. Astrophys.	Chinese Journal of Astronomy and Astrophysics
\fcp	Fundamentals Cosmic Phys.	Fundamentals of Cosmic Physics
\gca	Geochimica Cosmochimica Acta	Geochimica Cosmochimica Acta
\grl	Geophys. Res. Lett.	Geophysics Research Letters
\iaucirc	IAU Circ.	International Astronomical Union Circulars
\icarus	Icarus	Icarus
\japa	J. Astrophys. Astron.	Journal of Astrophysics and Astronomy
\jcap	J. Cosmology Astropart. Phys.	Journal of Cosmology and Astroparticle Physics
\jcp	J. Chem. Phys.	Journal of Chemical Physics
\jgr	J. Geophys. Res.	Journal of Geophysics Research
\jqsrt	J. Quant. Spectrosc. Radiative Transfer	Journal of Quantitiative Spectroscopy and Radiative Transfer
\jrasc	J. R. Astron. Soc. Canada	Journal of the Royal Astronomical Society of Canada
\memras	Mem. RAS	Memoirs of the Royal Astronomical Society
\memsai	Mem. Soc. Astron. Italiana	Memoire della Societa Astronomica Italiana
\mnassa	MNASSA	Monthly Notes of the Astronomical Society of Southern Africa
\mnras	MNRAS	Monthly Notices of the Royal Astronomical Societya
\na	New Astron.	New Astronomy
\nar	New Astron. Rev.	New Astronomy Review
\nat	Nature	Nature
\nphysa	Nuclear Phys. A	Nuclear Physics A
\pra	Phys. Rev. A	Physical Review A: Atomic, molecular, and optical physics
\prb	Phys. Rev. B	Physical Review B: Condensed matter and materials physics
\prc	Phys. Rev. C	Physical Review C: Nuclear physics
\prd	Phys. Rev. D	Physical Review D: Particles, fields, gravitation, and cosmology
\pre	Phys. Rev. E	Physical Review E: Statistical, nonlinear, and soft matter physics
\prl	Phys. Rev. Lett.	Physical Review Letters
\pasa	Publ. Astron. Soc. Australia	Publications of the Astronomical Society of Australia
\pasp	PASP	Publications of the Astronomical Society of the Pacific
\pasj	PASJ	Publications of the Astronomical Society of Japan
\physrep	Phys. Rep.	Physics Reports
\physscr	Phys. Scr.	Physica Scripta
\planss	Planet. Space Sci.	Planetary and Space Science
\procspie	Proc. SPIE	Proceedings of the Society of Photo-Optical Instrumentation Engineers
\rmxaa	Rev. Mex. Astron. Astrofis.	Revista Mexicana de Astronomia y Astrofisica
\qjras	QJRAS	Quarterly Journal of the Royal Astronomical Society
\sci	Science	Science
\skytel	Sky & Telesc.	Sky and Telescope
\solphys	Sol. Phys.	Solar Physics
\sovast	Soviet Ast.	Soviet Astronomyb
\ssr	Space Sci. Rev.	Space Science Reviews
\zap	Z. Astrophys.	Zeitschrift fuer Astrophysik
a Letters are designated by an L at the start of the page number, not in the journal name
b In 1992 the English translation of this journal changed its name from Soviet Astronomy to Astronomy Reports
c Including the English translation Astronomy Letters

Equations

$$a^2=b^2+c^2$$

Full text

††pubyear: 2015††pagerange: Monthly Notices of the Royal Astronomical Society: LaTeX guide for authors–C

1. 1 Introduction

2. 2 Obtaining and installing the MNRAS package

3. 3 Preparing and submitting a paper

4. 4 Class options

5. 5 Title page

6. 5.1 Title

7. 5.2 Authors and institutions

8. 5.3 Abstract and keywords

9. 6 Sections and lists

10. 6.1 Sections

11. 6.2 Lists

12. 7 Mathematics and symbols

13. 7.1 Equations

14. 7.2 Special symbols

15. 7.3 Ions

16. 8 Figures and tables

17. 8.1 Basic examples

18. 8.2 Captions and placement

19. 9 References and citations

20. 9.1 Cross-referencing

21. 9.2 Citations

22. 9.3 The list of references

23. 10 Appendices and online material

24. 11 Packages and custom commands

25. 11.1 Additional packages

26. 11.2 Custom commands

27. Acknowledgements

28. A Journal abbreviations

29. B Advanced formatting examples

30. C Additional commands for editors only

1 Introduction

The journal Monthly Notices of the Royal Astronomical Society (MNRAS) encourages authors to prepare their papers using LaTeX. The style file mnras.cls can be used to approximate the final appearance of the journal, and provides numerous features to simplify the preparation of papers. This document, mnras_guide.tex, provides guidance on using that style file and the features it enables.

This is not a general guide on how to use LaTeX, of which many excellent examples already exist. We particularly recommend Wikibooks LaTeX111https://en.wikibooks.org/wiki/LaTeX, a collaborative online textbook which is of use to both beginners and experts. Alternatively there are several other online resources, and most academic libraries also hold suitable beginner’s guides.

For guidance on the contents of papers, journal style, and how to submit a paper, see the MNRAS Instructions to Authors222http://www.oxfordjournals.org/our_journals/mnras/for_authors/. Only technical issues with the LaTeX class are considered here.

2 Obtaining and installing the MNRAS package

Some LaTeX distributions come with the MNRAS package by default. If yours does not, you can either install it using your distribution’s package manager, or download it from the Comprehensive TeX Archive Network333http://www.ctan.org/tex-archive/macros/latex/contrib/mnras (CTAN).

The files can either be installed permanently by placing them in the appropriate directory (consult the documentation for your LaTeX distribution), or used temporarily by placing them in the working directory for your paper.

To use the MNRAS package, simply specify mnras as the document class at the start of a .tex file:

\documentclass{mnras}

Then compile LaTeX (and if necessary Bib​TeX) in the usual way.

3 Preparing and submitting a paper

We recommend that you start with a copy of the mnras_template.tex file. Rename the file, update the information on the title page, and then work on the text of your paper. Guidelines for content, style etc. are given in the instructions to authors on the journal’s website${}^{\ref{foot:itas}}$. Note that this document does not follow all the aspects of MNRAS journal style (e.g. it has a table of contents).

If a paper is accepted, it is professionally typeset and copyedited by the publishers. It is therefore likely that minor changes to presentation will occur. For this reason, we ask authors to ignore minor details such as slightly long lines, extra blank spaces, or misplaced figures, because these details will be dealt with during the production process.

Papers must be submitted electronically via the online submission system; paper submissions are not permitted. For full guidance on how to submit a paper, see the instructions to authors.

4 Class options

There are several options which can be added to the document class line like this:

\documentclass[option1,option2]{mnras}

The available options are:

• •

letters – used for papers in the journal’s Letters section.

• •

onecolumn – single column, instead of the default two columns. This should be used only if necessary for the display of numerous very long equations.

• •

doublespacing – text has double line spacing. Please don’t submit papers in this format.

• •

referee – (deprecated) single column, double spaced, larger text, bigger margins. Please don’t submit papers in this format.

• •

galley – (deprecated) no running headers, no attempt to align the bottom of columns.

• •

landscape – (deprecated) sets the whole document on landscape paper.

• •

usenatbib – (all papers should use this) this uses Patrick Daly’s natbib.sty package for citations.

• •

usegraphicx – (most papers will need this) includes the graphicx package, for inclusion of figures and images.

• •

useAMS – adds support for upright Greek characters \upi, \umu and \upartial ($\pi$, $\mu$ and $\partial$). Only these three are included, if you require other symbols you will need to include the amsmath or amsymb packages (see section 11).

• •

usedcolumn – includes the package dcolumn, which includes two new types of column alignment for use in tables.

Some of these options are deprecated and retained for backwards compatibility only. Others are used in almost all papers, but again are retained as options to ensure that papers written decades ago will continue to compile without problems. If you want to include any other packages, see section 11.

5 Title page

If you are using mnras_template.tex the necessary code for generating the title page, headers and footers is already present. Simply edit the title, author list, institutions, abstract and keywords as described below.

5.1 Title

There are two forms of the title: the full version used on the first page, and a short version which is used in the header of other odd-numbered pages (the ‘running head’). Enter them with \title[]{} like this:

\title[Running head]{Full title of the paper}

The full title can be multiple lines (use \ to start a new line) and may be as long as necessary, although we encourage authors to use concise titles. The running head must be $\leq~{}45$ characters on a single line.

See appendix B for more complicated examples.

5.2 Authors and institutions

Like the title, there are two forms of author list: the full version which appears on the title page, and a short form which appears in the header of the even-numbered pages. Enter them using the \author[]{} command.

If the author list is more than one line long, start a new line using \newauthor. Use \ to start the institution list. Affiliations for each author should be indicated with a superscript number, and correspond to the list of institutions below the author list.

For example, if I were to write a paper with two coauthors at another institution, one of whom also works at a third location:

\author[K. T. Smith et al.]{ Keith T. Smith,$^{1}$ A. N. Other,$^{2}$ and Third Author$^{2,3}$ \ $^{1}$Affiliation 1\ $^{2}$Affiliation 2\ $^{3}$Affiliation 3}

Affiliations should be in the format ‘Department, Institution, Street Address, City and Postal Code, Country’.

Email addresses can be inserted with the \thanks{} command which adds a title page footnote. If you want to list more than one email, put them all in the same \thanks and use \footnotemark[] to refer to the same footnote multiple times. Present addresses (if different to those where the work was performed) can also be added with a \thanks command.

5.3 Abstract and keywords

The abstract is entered in an abstract environment:

\begin{abstract} The abstract of the paper. \end{abstract}

Note that there is a word limit on the length of abstracts. For the current word limit, see the journal instructions to authors${}^{\ref{foot:itas}}$.

Immediately following the abstract, a set of keywords is entered in a keywords environment:

\begin{keywords} keyword 1 -- keyword 2 -- keyword 3 \end{keywords}

There is a list of permitted keywords, which is agreed between all the major astronomy journals and revised every few years. Do not make up new keywords! For the current list of allowed keywords, see the journal’s instructions to authors${}^{\ref{foot:itas}}$.

6 Sections and lists

Sections and lists are generally the same as in the standard LaTeX classes.

6.1 Sections

Sections are entered in the usual way, using \section{} and its variants. It is possible to nest up to four section levels:

\section{Main section} \subsection{Subsection} \subsubsection{Subsubsection} \paragraph{Lowest level section}

The other LaTeX sectioning commands \part, \chapter and \subparagraph{} are deprecated and should not be used.

Some sections are not numbered as part of journal style (e.g. the Acknowledgements). To insert an unnumbered section use the ‘starred’ version of the command: \section*{}.

See appendix B for more complicated examples.

6.2 Lists

Two forms of lists can be used in MNRAS – numbered and unnumbered.

For a numbered list, use the enumerate environment:

\begin{enumerate} \item First item \item Second item \item etc. \end{enumerate}

which produces

First item 2. 2.

Second item 3. 3.

etc.

Note that the list uses lowercase Roman numerals, rather than the LaTeX default Arabic numerals.

For an unnumbered list, use the description environment without the optional argument:

\begin{description} \item First item \item Second item \item etc. \end{description}

which produces

First item

Second item

etc.

Bulleted lists using the itemize environment should not be used in MNRAS; it is retained for backwards compatibility only.

7 Mathematics and symbols

The MNRAS class mostly adopts standard LaTeX handling of mathematics, which is briefly summarised here. See also section 11 for packages that support more advanced mathematics.

Mathematics can be inserted into the running text using the syntax $1+1=2$, which produces $1+1=2$. Use this only for short expressions or when referring to mathematical quantities; equations should be entered as described below.

7.1 Equations

Equations should be entered using the equation environment, which automatically numbers them:

\begin{equation} a^2=b^2+c^2 \end{equation}

which produces

[TABLE]

By default, the equations are numbered sequentially throughout the whole paper. If a paper has a large number of equations, it may be better to number them by section (2.1, 2.2 etc.). To do this, add the command \numberwithin{equation}{section} to the preamble.

It is also possible to produce un-numbered equations by using the LaTeX built-in […] and $…$ commands; however MNRAS requires that all equations are numbered, so these commands should be avoided.

7.2 Special symbols

Some additional symbols of common use in astronomy have been added in the MNRAS class. These are shown in tables 1–2. The command names are – as far as possible – the same as those used in other major astronomy journals.

Many other mathematical symbols are also available, either built into LaTeX or via additional packages. If you want to insert a specific symbol but don’t know the LaTeX command, we recommend using the Detexify website444http://detexify.kirelabs.org.

Sometimes font or coding limitations mean a symbol may not get smaller when used in sub- or superscripts, and will therefore be displayed at the wrong size. There is no need to worry about this as it will be corrected by the typesetter during production.

To produce bold symbols in mathematics, use \bmath for simple variables, and the bm package for more complex symbols (see section 11). Vectors are set in bold italic, using \mathbfit{}.

For matrices, use \mathbfss{} to produce a bold sans-serif font e.g. H; this works even outside maths mode, but not all symbols are available (e.g. Greek). For $\nabla$ (del, used in gradients, divergence etc.) use $\nabla$.

7.3 Ions

A new \ion{}{} command has been added to the class file, for the correct typesetting of ionisation states. For example, to typeset singly ionised calcium use \ion{Ca}{ii}, which produces Ca ii.

8 Figures and tables

Figures and tables (collectively called ‘floats’) are mostly the same as built into LaTeX.

8.1 Basic examples

Figures are inserted in the usual way using a figure environment and \includegraphics. The example Figure 1 was generated using the code:

\begin{figure} \includegraphics[width=\columnwidth]{example} \caption{An example figure.} \label{fig:example} \end{figure}

The example Table 3 was generated using the code:

\begin{table} \caption{An example table.} \label{tab:example} \begin{tabular}{lcc} \hline Star & Mass & Luminosity\ & $M_{\sun}$ & $L_{\sun}$\ \hline Sun & 1.00 & 1.00\ $\alpha$CenA & 1.10 & 1.52\ $\epsilon$~Eri & 0.82 & 0.34\ \hline \end{tabular} \end{table}

8.2 Captions and placement

Captions go above tables but below figures, as in the examples above.

The LaTeX float placement commands [htbp] are intentionally disabled. Layout of figures and tables will be adjusted by the publisher during the production process, so authors should not concern themselves with placement to avoid disappointment and wasted effort. Simply place the LaTeX code close to where the figure or table is first mentioned in the text and leave exact placement to the publishers.

By default a figure or table will occupy one column of the page. To produce a wider version which covers both columns, use the figure* or table* environment.

If a figure or table is too long to fit on a single page it can be split it into several parts. Create an additional figure or table which uses \contcaption{} instead of \caption{}. This will automatically correct the numbering and add ‘continued’ at the start of the caption.

Table 4 was generated using the code:

\begin{table} \contcaption{A table continued from the previous one.} \label{tab:continued} \begin{tabular}{lcc} \hline Star & Mass & Luminosity\ & $M_{\sun}$ & $L_{\sun}$\ \hline $\tau$~Cet & 0.78 & 0.52\ $\delta$~Pav & 0.99 & 1.22\ $\sigma$~Dra & 0.87 & 0.43\ \hline \end{tabular} \end{table}

To produce a landscape figure or table, use the pdflscape package and the landscape environment. The landscape Table 5 was produced using the code:

\begin{landscape} \begin{table} \caption{An example landscape table.} \label{tab:landscape} \begin{tabular}{cccccccccc} \hline Header & Header & ...\ Unit & Unit & ...\ \hline Data & Data & ...\ Data & Data & ...\ ...\ \hline \end{tabular} \end{table} \end{landscape}

Unfortunately this method will force a page break before the table appears. More complicated solutions are possible, but authors shouldn’t worry about this.

9 References and citations

9.1 Cross-referencing

The usual LaTeX commands \label{} and \ref{} can be used for cross-referencing within the same paper. We recommend that you use these whenever relevant, rather than writing out the section or figure numbers explicitly. This ensures that cross-references are updated whenever the numbering changes (e.g. during revision) and provides clickable links (if available in your compiler).

It is best to give each section, figure and table a logical label. For example, Table 2 has the label tab:mathssymbols, whilst section 11 has the label sec:packages. Add the label after the section or caption command, as in the examples in sections 6.1 and 8. Enter the cross-reference with a non-breaking space between the type of object and the number, like this: see Figure~\ref{fig:example}.

The \autoref{} command can be used to automatically fill out the type of object, saving on typing. It also causes the link to cover the whole phrase rather than just the number, but for that reason is only suitable for single cross-references rather than ranges. For example, \autoref{tab:journal_abbr} produces Table 7.

9.2 Citations

MNRAS uses the Harvard – author (year) – citation style, e.g. Author (2013). This is implemented in LaTeX via the natbib package, which in turn is included via the usenatbib package option (see section 4), which should be used in all papers.

Each entry in the reference list has a ‘key’ (see section 9.3) which is used to generate citations. There are two basic natbib commands:

\citet{key} produces an in-text citation: Author (2013)

\citep{key} produces a bracketed (parenthetical) citation: (Author, 2013)

Citations will include clickable links to the relevant entry in the reference list, if supported by your LaTeX compiler.

There are a number of other natbib commands which can be used for more complicated citations. The most commonly used ones are listed in Table 6. For full guidance on their use, consult the natbib documentation555http://www.ctan.org/pkg/natbib.

If a reference has several authors, natbib will automatically use ‘et al.’ if there are more than two authors. However, if a paper has exactly three authors, MNRAS style is to list all three on the first citation and use ‘et al.’ thereafter. If you are using Bib​TeX (see section 9.3) then this is handled automatically. If not, the \citet*{} and \citep*{} commands can be used at the first citation to include all of the authors.

9.3 The list of references

It is possible to enter references manually using the usual LaTeX commands, but we strongly encourage authors to use Bib​TeX instead. Bib​TeX ensures that the reference list is updated automatically as references are added or removed from the paper, puts them in the correct format, saves on typing, and the same reference file can be used for many different papers – saving time hunting down reference details. An MNRAS Bib​TeX style file, mnras.bst, is distributed as part of this package. The rest of this section will assume you are using Bib​TeX.

References are entered into a separate .bib file in standard Bib​TeX formatting. This can be done manually, or there are several software packages which make editing the .bib file much easier. We particularly recommend JabRef666http://jabref.sourceforge.net/, which works on all major operating systems. Bib​TeX entries can be obtained from the NASA Astrophysics Data System777http://adsabs.harvard.edu (ADS) by clicking on ‘Bibtex entry for this abstract’ on any entry. Simply copy this into your .bib file or into the ‘BibTeX source’ tab in JabRef.

Each entry in the .bib file must specify a unique ‘key’ to identify the paper, the format of which is up to the author. Simply cite it in the usual way, as described in section 9.2, using the specified key. Compile the paper as usual, but add an extra step to run the bibtex command. Consult the documentation for your compiler or latex distribution.

Correct formatting of the reference list will be handled by Bib​TeX in almost all cases, provided that the correct information was entered into the .bib file. Note that ADS entries are not always correct, particularly for older papers and conference proceedings, so may need to be edited. If in doubt, or if you are producing the reference list manually, see the MNRAS instructions to authors${}^{\ref{foot:itas}}$ for the current guidelines on how to format the list of references.

10 Appendices and online material

To start an appendix, simply place the \appendix command before the next \section{}. This will automatically adjust the section headings, figures, tables, and equations to reflect the fact that they are part of an appendix. It is only necessary to enter the \appendix command once – everything after that command is in an appendix. Remember that appendices should be placed after the list of references.

Unlike other astronomy class files, there are no special commands for online material. If your paper has any online material, it should be placed in a separate file. See our instructions to authors${}^{\ref{foot:itas}}$ for guidance.

11 Packages and custom commands

11.1 Additional packages

Sometimes authors need to include additional LaTeX packages, which provide extra features. For example, the bm package provides extra bold maths symbols, whilst the pdflscape package adds support for landscape pages. Packages can be included by adding the \usepackage{} command to the preamble of the document (not the main body).

Please only include packages which are actually used in the paper, and include a comment to explain what each one does. This will assist the typesetters. If you are using mnras_template.tex, it includes a specific section for this purpose, near the start of the file with the header ’authors - place your own packages here’.

For example, to include pdflscape, use:

\usepackage{pdflscape}Ψ% Landscape pages

Consult the documentation for that package for instructions on how to use the additional features.

11.2 Custom commands

Authors should avoid duplicating or redefining commands which are already available in LaTeX or mnras.cls. However it may sometimes be necessary to introduce a custom command e.g. as a shortcut while writing the paper.

Please only include commands which are actually used in the paper, and include a comment to explain what each one does. This will assist the typesetters. Use \newcommand, not \def, as this will avoid accidentally overwriting existing commands. Place custom commands in the preamble of the document (not the main body). If you are using mnras_template.tex, it includes a specific section for this purpose, near the start of the file with the header ’authors - place your own commands here’.

As an example, a shortcut for the unit  km s*-1*can be defined like this:

\newcommand{\kms}{,km,s$^{-1}$}Ψ% kilometres per second

Velocities can then be written as e.g. 2.3\kms which produces 2.3 km s*-1*. Similar shortcuts can be used for frequently quoted object designations.

Acknowledgements

This guide replaces an earlier one originally prepared by Cambridge University Press (CUP) in 1994, and last updated in 2002 by Blackwell Publishing. Some code segments are reproduced from, and some examples are based upon, that guide. The authors were: A. Woollatt, M. Reed, R. Mulvey, K. Matthews, D. Starling, Y. Yu, A. Richardson (all CUP), and Penny Smith, N. Thompson and Gregor Hutton (all Blackwell), whose work is gratefully acknowledged.

The accompanying Bib​TeX style file was written by John Sleath, Tim Jenness and Norman Gray, without whom Bib​TeX support would not have been possible.

Some special symbols in tables 1–2 were taken from the Springer Verlag Astronomy & Astrophysics LaTeX class, with their permission.

KTS thanks Nelson Beebe (University of Utah) for helpful advice regarding CTAN.

Appendix A Journal abbreviations

Abbreviations for cited journals can be accessed using the commands listed in table 7. Although some of these may appear to be outdated or rarely cited, they have been selected to be compatible with the Bib​TeX output by the NASA Astrophysics Data System${}^{\ref{foot:ads}}$, commands used by other astronomy journals, and with additional entries for journals with non-standard abbreviations in MNRAS. For journals which are not on this list, see our instructions to authors${}^{\ref{foot:itas}}$ for guidance on how to abbreviate titles.

Appendix B Advanced formatting examples

Sometimes formatting doesn’t behave exactly as expected when used in titles or section headings, and must be modified to obtain the correct appearance. Generally the publishers can fix these problems during the typesetting process after a paper is accepted, but authors may wish to adjust these themselves to minimise the possibility of errors and/or for the benefit of the refereeing process. Below are some examples of output, followed by the LaTeX code which produces them.

Most mathematics and text formatting works as expected, but some commands might not be the correct size, bold or italic. If so they can be finessed by hand, as in the bold mathematics here: Herschel* observations of galaxies at $\bm{\delta>60\degr}$***

** \title{\textit{Herschel} observations of galaxies at $\bm{\delta > 60\degr}$} **

Most fonts do not provide bold and italic versions of small capitals, so the \ion{}{} command doesn’t produce the expected output in headings. The effect has to be ‘faked’ using font size commands, remembering that the running head is a different style: Abundances in H II regions

** \title [Abundances in H,{\normalsize \textit{II}} regions] {Abundances in H,{\Large \textbf{II}} regions} **

Complex mathematics can cause problems with links, so might require adding a less formatted short version of the heading: 2 FINDING Mg II ABSORBERS AT $\bm{z>2}$

** \section [Finding Mg II absorbers at z > 2] {Finding M\lowercase{g},{\sevensize II} absorbers at $\lowercase{\bm{z > 2}}$} **

Using square brackets in headings can cause additional linking problems, which are solved by wrapping them in {…}: 2.1 [C II] 158$\mn@boldsymbol{\mu}$m emission

** \subsection [{[C II] 158$\umu$m emission}] {[C,{\sevensize II}] 158$\bmath{\umu}$m emission} **

Use \text{} (not \rm) for non-variables in mathematics, which preserves the formatting of the surrounding text. For the same reasons, use \textit{} for italics (not \it). 3.1 Measuring $\bm{T}_{\text{eff}}$ from Gaia photometry

** \subsection{Measuring $\bm{T}_\text{eff}$ from \textit{Gaia} photometry} **

Appendix C Additional commands for editors only

The following commands are available for the use of editors and production staff only. They should not be used (or modified in the template) by authors.

\maketitle** inserts the title, authors and institution list in the correct formatting.**

\nokeywords** tidies up the spacing if there are no keywords, but authors should always enter at least one.**

\volume{}** sets the volume number (default is 000)**

\pagerange{}** sets the page range. The standard template generates this automatically, starting from 1.**

\bsp** adds the ‘This paper has been typeset…’ comment at the end of the paper. The command name refers to Blackwell Science Publishing, who were the publishers at the time when MNRAS began accepting LaTeX submissions in 1993.**

\mniiiauth{}** used by the Bib​TeX style to handle MNRAS style for citing papers with three authors. It should not be used manually.**

\eprint{}** used by the Bib​TeX style for citing arXiv eprints.**

\doi{}** used by the Bib​TeX style for citing Digital Object Identifiers.**