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@ -42,6 +42,9 @@ authorshort: "Author One et.al."
#% \setwatermarkfontsize{dimension} #% \setwatermarkfontsize{dimension}
#\correspondingauthor{August Muench} #\correspondingauthor{August Muench}
#\email{greg.schwarz@aas.org, gus.muench@aas.org} #\email{greg.schwarz@aas.org, gus.muench@aas.org}
#end of docs
#\allauthors
#\listofchanges
processDate: processDate:
received: "March 11, 2022" received: "March 11, 2022"
accepted: "April 11, 2022" accepted: "April 11, 2022"
@ -54,7 +57,7 @@ appendix:
abstract: | abstract: |
This example manuscript is intended to serve as a tutorial and template for This example manuscript is intended to serve as a tutorial and template for
authors to use when writing their own AAS Journal articles. The manuscript authors to use when writing their own AAS Journal articles. The manuscript
includes a history of \aastex\ and documents the new features in the includes a history of \aastex and documents the new features in the
previous versions as well as the bug fixes in version 6.31. This previous versions as well as the bug fixes in version 6.31. This
manuscript includes many figure and table examples to illustrate these new manuscript includes many figure and table examples to illustrate these new
features. Information on features not explicitly mentioned in the article features. Information on features not explicitly mentioned in the article
@ -77,7 +80,12 @@ abstractTex:
{It is shown that stability depends only upon the equations of state, the opacities and the local thermodynamic state in the layer. Stability and instability can therefore be expressed in the form of stability equations of state which are universal for a given composition.} {It is shown that stability depends only upon the equations of state, the opacities and the local thermodynamic state in the layer. Stability and instability can therefore be expressed in the form of stability equations of state which are universal for a given composition.}
{The stability equations of state are calculated for solar composition and are displayed in the domain $-14 \leq \lg \rho / \mathrm{[g\, cm^{-3}]} \leq 0 $, $ 8.8 \leq \lg e / \mathrm{[erg\, g^{-1}]} \leq 17.7$. These displays may be used to determine the one-zone stability of layers in stellar or planetary structure models by directly reading off the value of the stability equations for the thermodynamic state of these layers, specified by state quantities as density $\rho$, temperature $T$ or specific internal energy $e$. Regions of instability in the $(\rho,e)$-plane are described and related to the underlying microphysical processes.} {The stability equations of state are calculated for solar composition and are displayed in the domain $-14 \leq \lg \rho / \mathrm{[g\, cm^{-3}]} \leq 0 $, $ 8.8 \leq \lg e / \mathrm{[erg\, g^{-1}]} \leq 17.7$. These displays may be used to determine the one-zone stability of layers in stellar or planetary structure models by directly reading off the value of the stability equations for the thermodynamic state of these layers, specified by state quantities as density $\rho$, temperature $T$ or specific internal energy $e$. Regions of instability in the $(\rho,e)$-plane are described and related to the underlying microphysical processes.}
{Vibrational instability is found to be a common phenomenon at temperatures lower than the second He ionisation zone. The $\kappa$-mechanism is widespread under 'cool' conditions.} {Vibrational instability is found to be a common phenomenon at temperatures lower than the second He ionisation zone. The $\kappa$-mechanism is widespread under 'cool' conditions.}
keywords: giant planet formation -- $\kappa$-mechanism -- stability of gas spheres keywords:
# will use --- as separator
- Classical Novae (251)
- Ultraviolet astronomy(1736)
- History of astronomy(1868)
- Interdisciplinary astronomy(804)
facilities: "HST(STIS)" facilities: "HST(STIS)"
acknowledgements: acknowledgements:
@ -136,13 +144,13 @@ We use `#` on various levels. Headings should be shown as a line that prefixed b
blank line stands as a paragraph separator. No indentation for the first line (it only required in multilined lists to show that the next line is part of the item if it is non-blank and indented). blank line stands as a paragraph separator. No indentation for the first line (it only required in multilined lists to show that the next line is part of the item if it is non-blank and indented).
## Italic ## Italic
\v{*} Ex. \v{this text is *italic*} : this text is *italic* `*` Ex. `this text is *italic*` : this text is *italic*
## Bold ## Bold
\v{**} Ex. \v{this text is **bold**} : this text is **bold** `**` Ex. `this text is **bold**` : this text is **bold**
## Bold and Italic ## Bold and Italic
\v{***} Ex. \v{this text is ***bold and italic***} this text is ***bold and italic*** `***` Ex. `this text is ***bold and italic***` this text is ***bold and italic***
## Verbatim ## Verbatim
Verbatim should use backticks \v{`text`}, Ex. ``this is `the text` `` this is `the text`. Verbatim should use backticks \v{`text`}, Ex. ``this is `the text` `` this is `the text`.
@ -809,59 +817,25 @@ create label for \ref{FigVibStab} using #FigVibStab
# Introduction
\latex \footnote{\url{http://www.latex-project.org/}} is a document markup
\end{abstract}
%% Keywords should appear after the \end{abstract} command.
%% The AAS Journals now uses Unified Astronomy Thesaurus concepts:
%% https://astrothesaurus.org
%% You will be asked to selected these concepts during the submission process
%% but this old "keyword" functionality is maintained in case authors want
%% to include these concepts in their preprints.
\keywords{Classical Novae (251) --- Ultraviolet astronomy(1736) --- History of astronomy(1868) --- Interdisciplinary astronomy(804)}
%% From the front matter, we move on to the body of the paper.
%% Sections are demarcated by \section and \subsection, respectively.
%% Observe the use of the LaTeX \label
%% command after the \subsection to give a symbolic KEY to the
%% subsection for cross-referencing in a \ref command.
%% You can use LaTeX's \ref and \label commands to keep track of
%% cross-references to sections, equations, tables, and figures.
%% That way, if you change the order of any elements, LaTeX will
%% automatically renumber them.
%%
%% We recommend that authors also use the natbib \citep
%% and \citet commands to identify citations. The citations are
%% tied to the reference list via symbolic KEYs. The KEY corresponds
%% to the KEY in the \bibitem in the reference list below.
\section{Introduction} \label{sec:intro}
\latex\ \footnote{\url{http://www.latex-project.org/}} is a document markup
language that is particularly well suited for the publication of language that is particularly well suited for the publication of
mathematical and scientific articles \citep{lamport94}. \latex\ was written mathematical and scientific articles \citep{lamport94}. \latex was written
in 1985 by Leslie Lamport who based it on the \TeX\ typesetting language in 1985 by Leslie Lamport who based it on the \TeX typesetting language
which itself was created by Donald E. Knuth in 1978. In 1988 a suite of which itself was created by Donald E. Knuth in 1978. In 1988 a suite of
\latex\ macros were developed to investigate electronic submission and \latex macros were developed to investigate electronic submission and
publication of AAS Journal articles \citep{1989BAAS...21..780H}. Shortly publication of AAS Journal articles \citep{1989BAAS...21..780H}. Shortly
afterwards, Chris Biemesdefer merged these macros and more into a \latex\ afterwards, Chris Biemesdefer merged these macros and more into a \latex\
2.08 style file called \aastex. These early \aastex\ versions introduced 2.08 style file called \aastex. These early \aastex versions introduced
many common commands and practices that authors take for granted today. many common commands and practices that authors take for granted today.
Substantial revisions Substantial revisions
were made by Lee Brotzman and Pierre Landau when the package was updated to were made by Lee Brotzman and Pierre Landau when the package was updated to
v4.0. AASTeX v5.0, written in 1995 by Arthur Ogawa, upgraded to \latex\ 2e v4.0. AASTeX v5.0, written in 1995 by Arthur Ogawa, upgraded to \latex 2e
which uses the document class in lieu of a style file. Other improvements which uses the document class in lieu of a style file. Other improvements
to version 5 included hypertext support, landscape deluxetables and to version 5 included hypertext support, landscape deluxetables and
improved figure support to facilitate electronic submission. improved figure support to facilitate electronic submission.
\aastex\ v5.2 was released in 2005 and introduced additional graphics \aastex v5.2 was released in 2005 and introduced additional graphics
support plus new mark up to identifier astronomical objects, datasets and support plus new mark up to identifier astronomical objects, datasets and
facilities. facilities.
@ -869,7 +843,7 @@ In 1996 Maxim Markevitch modified the AAS preprint style file, aaspp4.sty,
to closely emulate the very tight, two column style of a typeset to closely emulate the very tight, two column style of a typeset
Astrophysical Journal article. The result was emulateapj.sty. A year Astrophysical Journal article. The result was emulateapj.sty. A year
later Alexey Vikhlinin took over development and maintenance. In 2001 he later Alexey Vikhlinin took over development and maintenance. In 2001 he
converted emulateapj into a class file in \latex\ 2e and in 2003 Vikhlinin converted emulateapj into a class file in \latex 2e and in 2003 Vikhlinin
completely rewrote emulateapj based on the APS Journal's RevTEX class. completely rewrote emulateapj based on the APS Journal's RevTEX class.
During this time emulateapj gained growing acceptance in the astronomical During this time emulateapj gained growing acceptance in the astronomical
@ -882,17 +856,17 @@ Even though author publication charges are no longer based on print pages
\footnote{see Section \ref{sec:pubcharge} in the Appendix for more details \footnote{see Section \ref{sec:pubcharge} in the Appendix for more details
about how current article costs are calculated.} the emulateapj class file about how current article costs are calculated.} the emulateapj class file
has proven to be extremely popular with AAS Journal authors. An has proven to be extremely popular with AAS Journal authors. An
analysis of submitted \latex\ manuscripts in 2015 revealed that $\sim$65\% analysis of submitted \latex manuscripts in 2015 revealed that sim65
either called emulateapj or have a commented emulateapj classfile call either called emulateapj or have a commented emulateapj classfile call
indicating it was used at some stage of the manuscript construction. indicating it was used at some stage of the manuscript construction.
Clearly authors want to have access to a tightly typeset version of the Clearly authors want to have access to a tightly typeset version of the
article when corresponding with co-authors and for preprint submissions. article when corresponding with co-authors and for preprint submissions.
When planning the next \aastex\ release the popularity of emulateapj played When planning the next \aastex release the popularity of emulateapj played
an important roll in the decision to drop the old base code and adopt and an important roll in the decision to drop the old base code and adopt and
modify emulateapj for \aastex\ v6.+ instead. The change brings \aastex\ modify emulateapj for \aastex v6.+ instead. The change brings \aastex\
inline with what the majority of authors are already using while still inline with what the majority of authors are already using while still
delivering new and improved features. \aastex\ v6.0 through v6.31 were delivering new and improved features. \aastex v6.0 through v6.31 were
written by Amy Hendrickson. The release dates were January 2016 (v6.0), written by Amy Hendrickson. The release dates were January 2016 (v6.0),
October 2016 (v6.1), January 2018 (v6.2), June 2019 (v6.3), and March 2010 October 2016 (v6.1), January 2018 (v6.2), June 2019 (v6.3), and March 2010
(v6.31) respectively. (v6.31) respectively.
@ -943,7 +917,7 @@ encapsulated postscript (EPS) or portable document format (PDF) files,
The rest of this article provides information and examples on how to create The rest of this article provides information and examples on how to create
your own AAS Journal manuscript with v6.31. Special emphasis is placed on your own AAS Journal manuscript with v6.31. Special emphasis is placed on
how to use the full potential of \aastex\ v6+. The next section describes how to use the full potential of \aastex v6+. The next section describes
the different manuscript styles available and how they differ from past the different manuscript styles available and how they differ from past
releases. Section \ref{sec:floats} describes table and figure placement. releases. Section \ref{sec:floats} describes table and figure placement.
Specific examples of tables, Section Specific examples of tables, Section
@ -955,12 +929,12 @@ discuss how to use different ways to highlight revisions. The last section,
\ref{sec:cite}, shows how recognize software and external data as first \ref{sec:cite}, shows how recognize software and external data as first
class references in the manuscript bibliography. An appendix is included class references in the manuscript bibliography. An appendix is included
for additional information readers might find useful. for additional information readers might find useful.
More documentation is embedded in the comments of this \latex\ file and in the online documentation at More documentation is embedded in the comments of this \latex file and in the online documentation at
\url{http://journals.aas.org/authors/aastex.html}. \url{http://journals.aas.org/authors/aastex.html}.
\section{Manuscript styles} \label{sec:style} # Manuscript styles
The default style in \aastex\ v6.31 is a tight single column style, e.g. 10 The default style in \aastex v6.31 is a tight single column style, e.g. 10
point font, single spaced. The single column style is very useful for point font, single spaced. The single column style is very useful for
article with wide equations. It is also the easiest to style to work with article with wide equations. It is also the easiest to style to work with
since figures and tables, see Section \ref{sec:floats}, will span the since figures and tables, see Section \ref{sec:floats}, will span the
@ -1006,11 +980,11 @@ environment. The use of this option is highly recommended for PSJ submissions.
Advice for anonymizing your manuscript for DAR is provided at Advice for anonymizing your manuscript for DAR is provided at
\url{https://journals.aas.org/manuscript-preparation/#dar}. \url{https://journals.aas.org/manuscript-preparation/#dar}.
\section{Floats} \label{sec:floats} # Floats
Floats are non-text items that generally can not be split over a page. Floats are non-text items that generally can not be split over a page.
They also have captions and can be numbered for reference. Primarily these They also have captions and can be numbered for reference. Primarily these
are figures and tables but authors can define their own. \latex\ tries to are figures and tables but authors can define their own. \latex tries to
place a float where indicated in the manuscript but will move it later if place a float where indicated in the manuscript but will move it later if
there is not enough room at that location, hence the term ``float''. there is not enough room at that location, hence the term ``float''.
@ -1035,23 +1009,23 @@ For authors that do want to take the time to optimize the locations of
their floats there are some techniques that can be used. The simplest their floats there are some techniques that can be used. The simplest
solution is to placing a float earlier in the text to get the position solution is to placing a float earlier in the text to get the position
right but this option will break down if the manuscript is altered. right but this option will break down if the manuscript is altered.
A better method is to force \latex\ to place a A better method is to force \latex to place a
float in a general area with the use of the optional {\tt\string [placement float in a general area with the use of the optional {\tt\string [placement
specifier]} parameter for figures and tables. This parameter goes after specifier]} parameter for figures and tables. This parameter goes after
{\tt\string \begin\{figure\}}, {\tt\string \begin\{table\}}, and {\tt\string \begin\{figure\}}, {\tt\string \begin\{table\}}, and
{\tt\string \begin\{deluxetable\}}. The main arguments the specifier takes {\tt\string \begin\{deluxetable\}}. The main arguments the specifier takes
are ``h'', ``t'', ``b'', and ``!''. These tell \latex\ to place the float are ``h'', ``t'', ``b'', and ``!''. These tell \latex to place the float
\underline{h}ere (or as close as possible to this location as possible), at \underline{h}ere (or as close as possible to this location as possible), at
the \underline{t}op of the page, and at the \underline{b}ottom of the page. the \underline{t}op of the page, and at the \underline{b}ottom of the page.
The last argument, ``!'', tells \latex\ to override its internal method of The last argument, ``!'', tells \latex to override its internal method of
calculating the float position. A sequence of rules can be created by calculating the float position. A sequence of rules can be created by
using multiple arguments. For example, {\tt\string \begin\{figure\}[htb!]} using multiple arguments. For example, {\tt\string \begin\{figure\}[htb!]}
tells \latex\ to try the current location first, then the top of the page tells \latex to try the current location first, then the top of the page
and finally the bottom of the page without regard to what it thinks the and finally the bottom of the page without regard to what it thinks the
proper position should be. Many of the tables and figures in this article proper position should be. Many of the tables and figures in this article
use a placement specifier to set their positions. use a placement specifier to set their positions.
Note that the \latex\ {\tt\string tabular} environment is not a float. Only Note that the \latex {\tt\string tabular} environment is not a float. Only
when a {\tt\string tabular} is surrounded by {\tt\string\begin\{table\}} ... when a {\tt\string tabular} is surrounded by {\tt\string\begin\{table\}} ...
{\tt\string\end\{table\}} is it a true float and the rules and suggestions {\tt\string\end\{table\}} is it a true float and the rules and suggestions
above apply. above apply.
@ -1062,7 +1036,7 @@ begin with the {\tt\string\startlongtable} command. This initiates a
longtable environment. Authors might have to use {\tt\string\clearpage} to longtable environment. Authors might have to use {\tt\string\clearpage} to
isolate a long table or optimally place it within the surrounding text. isolate a long table or optimally place it within the surrounding text.
\subsection{Tables} \label{subsec:tables} ## Tables
Tables can be constructed with \latex's standard table environment or the Tables can be constructed with \latex's standard table environment or the
\aastex's deluxetable environment. The deluxetable construct handles long \aastex's deluxetable environment. The deluxetable construct handles long
@ -1081,7 +1055,7 @@ Authors are encouraged to create their own machine
readable tables using the online tool at readable tables using the online tool at
\url{http://authortools.aas.org/MRT/upload.html}. \url{http://authortools.aas.org/MRT/upload.html}.
\aastex\ v6 introduced five new table features that were designed to make \aastex v6 introduced five new table features that were designed to make
table construction easier and the resulting display better for AAS Journal table construction easier and the resulting display better for AAS Journal
authors. The items are: authors. The items are:
@ -1097,9 +1071,9 @@ Full details on how to create each type are given in the following
sections. Additional details are available in the AASTeX sections. Additional details are available in the AASTeX
guidelines at \url{http://journals.aas.org/authors/aastex.html} guidelines at \url{http://journals.aas.org/authors/aastex.html}
\subsubsection{Column math mode} ### Column math mode
Both the \latex\ tabular and \aastex\ deluxetable require an argument to Both the \latex tabular and \aastex deluxetable require an argument to
define the alignment and number of columns. The most common values are define the alignment and number of columns. The most common values are
``c'', ``l'' and ``r'' for \underline{c}enter, \underline{l}eft, and ``c'', ``l'' and ``r'' for \underline{c}enter, \underline{l}eft, and
\underline{r}ight justification. If these values are capitalized, e.g. \underline{r}ight justification. If these values are capitalized, e.g.
@ -1107,12 +1081,12 @@ define the alignment and number of columns. The most common values are
mode meaning that \$s are not required. Note that having embedded dollar mode meaning that \$s are not required. Note that having embedded dollar
signs in the table does not affect the output. signs in the table does not affect the output.
\subsubsection{Decimal alignment} ### Decimal alignment
Aligning a column by the decimal point can be difficult with only center, Aligning a column by the decimal point can be difficult with only center,
left, and right justification options. It is possible to use phantom calls left, and right justification options. It is possible to use phantom calls
in the data, e.g. {\tt\string\phn}, to align columns by hand but this can in the data, e.g. {\tt\string\phn}, to align columns by hand but this can
be tedious in long or complex tables. To address this \aastex\ introduces be tedious in long or complex tables. To address this \aastex introduces
the {\tt\string\decimals} command and a new column justification option, the {\tt\string\decimals} command and a new column justification option,
``D'', to align data in that column on the decimal. In deluxetable the ``D'', to align data in that column on the decimal. In deluxetable the
{\tt\string\decimals} command is invoked before the {\tt\string\startdata} {\tt\string\decimals} command is invoked before the {\tt\string\startdata}
@ -1129,17 +1103,17 @@ works so that the headers are accounted for correctly. All decimal column
headers need to span two columns to get the alignment correct. This can be headers need to span two columns to get the alignment correct. This can be
done with a multicolumn call, e.g {\tt\string\multicolumn2c\{\}} or done with a multicolumn call, e.g {\tt\string\multicolumn2c\{\}} or
{\tt\string\multicolumn\{2\}\{c\}\{\}}, or use the new {\tt\string\multicolumn\{2\}\{c\}\{\}}, or use the new
{\tt\string\twocolhead\{\}} command in deluxetable. Since \latex\ is {\tt\string\twocolhead\{\}} command in deluxetable. Since \latex is
splitting these columns into two it is important to get the table width splitting these columns into two it is important to get the table width
right so that they appear joined on the page. You may have to run the right so that they appear joined on the page. You may have to run the
\latex\ compiler twice to get it right. \latex compiler twice to get it right.
\subsubsection{Automatic column header numbering} \label{subsubsec:autonumber} ### Automatic column header numbering
The command {\tt\string\colnumbers} can be included to automatically number The command {\tt\string\colnumbers} can be included to automatically number
each column as the last row in the header. Per the AAS Journal table format each column as the last row in the header. Per the AAS Journal table format
standards, each column index numbers will be surrounded by parentheses. In standards, each column index numbers will be surrounded by parentheses. In
a \latex\ tabular environment the {\tt\string\colnumbers} should be invoked a \latex tabular environment the {\tt\string\colnumbers} should be invoked
at the location where the author wants the numbers to appear, e.g. after at the location where the author wants the numbers to appear, e.g. after
the last line of specified table header rows. In deluxetable this command the last line of specified table header rows. In deluxetable this command
has to come before {\tt\string\startdata}. {\tt\string\colnumbers} will has to come before {\tt\string\startdata}. {\tt\string\colnumbers} will
@ -1150,10 +1124,10 @@ Note that when using decimal alignment in a table the command
{\tt\string\decimalcolnumbers} must be used instead of {\tt\string\decimalcolnumbers} must be used instead of
{\tt\string\colnumbers} and {\tt\string\decimals}. {\tt\string\colnumbers} and {\tt\string\decimals}.
\subsubsection{Hiding columns} \label{subsubsec:hide} ### Hiding columns
Entire columns can be \underline{h}idden from display simply by changing Entire columns can be \underline{h}idden from display simply by changing
the specified column identifier to ``h''. In the \latex\ tabular environment the specified column identifier to ``h''. In the \latex tabular environment
this column identifier conceals the entire column including the header this column identifier conceals the entire column including the header
columns. In \aastex's deluxetables the header row is specifically columns. In \aastex's deluxetables the header row is specifically
declared with the {\tt\string\tablehead} call and each header column is declared with the {\tt\string\tablehead} call and each header column is
@ -1165,7 +1139,7 @@ Authors can use this option in many different ways. Since column data can
be easily suppressed authors can include extra information and hid it be easily suppressed authors can include extra information and hid it
based on the comments of co-authors or referees. For wide tables that will based on the comments of co-authors or referees. For wide tables that will
have a machine readable version, authors could put all the information in have a machine readable version, authors could put all the information in
the \latex\ table but use this option to hid as many columns as needed until the \latex table but use this option to hid as many columns as needed until
it fits on a page. This concealed column table would serve as the it fits on a page. This concealed column table would serve as the
example table for the full machine readable version. Regardless of how example table for the full machine readable version. Regardless of how
columns are obscured, authors are responsible for removing any unneeded columns are obscured, authors are responsible for removing any unneeded
@ -1176,10 +1150,10 @@ Table \ref{tab:messier} provides some basic information about the first ten
Messier Objects and illustrates how many of these new features can be used Messier Objects and illustrates how many of these new features can be used
together. It has automatic column numbering, decimal alignment of the together. It has automatic column numbering, decimal alignment of the
distances, and one concealed column. The Common name column distances, and one concealed column. The Common name column
is the third in the \latex\ deluxetable but does not appear when the article is the third in the \latex deluxetable but does not appear when the article
is compiled. This hidden column can be shown simply by changing the ``h'' in is compiled. This hidden column can be shown simply by changing the ``h'' in
the column identifier preamble to another valid value. This table also the column identifier preamble to another valid value. This table also
uses {\tt\string\tablenum} to renumber the table because a \latex\ tabular uses {\tt\string\tablenum} to renumber the table because a \latex tabular
table was inserted before it. table was inserted before it.
\begin{deluxetable*}{cchlDlc} \begin{deluxetable*}{cchlDlc}
@ -1205,14 +1179,14 @@ M8 & NGC 6523 & Lagoon Nebula & Nebula with cluster & 1.25 & Sagittarius & 6.0 \
M9 & NGC 6333 & Messier 9 & Cluster, globular & 7.91 & Ophiuchus & 8.4 \\ M9 & NGC 6333 & Messier 9 & Cluster, globular & 7.91 & Ophiuchus & 8.4 \\
M10 & NGC 6254 & Messier 10 & Cluster, globular & 4.42 & Ophiuchus & 6.4 \\ M10 & NGC 6254 & Messier 10 & Cluster, globular & 4.42 & Ophiuchus & 6.4 \\
\enddata \enddata
\tablecomments{This table ``hides'' the third column in the \latex\ when compiled. \tablecomments{This table ``hides'' the third column in the \latex when compiled.
The Distance is also centered on the decimals. Note that when using decimal The Distance is also centered on the decimals. Note that when using decimal
alignment you need to include the {\tt\string\decimals} command before alignment you need to include the {\tt\string\decimals} command before
{\tt\string\startdata} and all of the values in that column have to have a {\tt\string\startdata} and all of the values in that column have to have a
space before the next ampersand.} space before the next ampersand.}
\end{deluxetable*} \end{deluxetable*}
\subsubsection{Splitting a table into multiple horizontal components} ### Splitting a table into multiple horizontal components
Since the AAS Journals are now all electronic with no print version there is Since the AAS Journals are now all electronic with no print version there is
no reason why tables can not be as wide as authors need them to be. no reason why tables can not be as wide as authors need them to be.
@ -1269,10 +1243,10 @@ V}} & \colhead{Si\,{\footnotesize IV}} & \colhead{C\,{\footnotesize IV}} &
split any table with this command into two or three parts. The location of split any table with this command into two or three parts. The location of
the split is given by the author based on the placement of the ``B'' the split is given by the author based on the placement of the ``B''
indicators in the column identifier preamble. For more information please indicators in the column identifier preamble. For more information please
look at the new \aastex\ instructions.} look at the new \aastex instructions.}
\end{splitdeluxetable*} \end{splitdeluxetable*}
\subsection{Figures\label{subsec:figures}} ## Figures
%% The "ht!" tells LaTeX to put the figure "here" first, at the "top" next %% The "ht!" tells LaTeX to put the figure "here" first, at the "top" next
%% and to override the normal way of calculating a float position %% and to override the normal way of calculating a float position
@ -1298,9 +1272,9 @@ due to a disability or offline access. This portion of the article
provides examples for setting up all these types in with the latest version provides examples for setting up all these types in with the latest version
of \aastex. of \aastex.
\subsection{General figures\label{subsec:general}} ## General figures
\aastex\ has a {\tt\string\plotone} command to display a figure consisting \aastex has a {\tt\string\plotone} command to display a figure consisting
of one EPS/PDF file. Figure \ref{fig:general} is an example which shows of one EPS/PDF file. Figure \ref{fig:general} is an example which shows
the approximate changes in the subscription costs and author publication the approximate changes in the subscription costs and author publication
charges from 1991 to 2013 in the AAS Journals. For a general figure charges from 1991 to 2013 in the AAS Journals. For a general figure
@ -1310,7 +1284,7 @@ used to position the two image files side by side.
Both {\tt\string\plotone} and {\tt\string\plottwo} take a Both {\tt\string\plotone} and {\tt\string\plottwo} take a
{\tt\string\caption} and an optional {\tt\string\figurenum} command to {\tt\string\caption} and an optional {\tt\string\figurenum} command to
specify the figure number\footnote{It is better to not use specify the figure number\footnote{It is better to not use
{\tt\string\figurenum} and let \latex\ auto-increment all the figures. If you {\tt\string\figurenum} and let \latex auto-increment all the figures. If you
do use this command you need to mark all of them accordingly.}. Each is do use this command you need to mark all of them accordingly.}. Each is
based on the {\tt\string graphicx} package command, based on the {\tt\string graphicx} package command,
{\tt\string\includegraphics}. Authors are welcome to use {\tt\string\includegraphics}. Authors are welcome to use
@ -1320,10 +1294,10 @@ More information on the full usage of {\tt\string\includegraphics} can be
found at \break found at \break
\url{https://en.wikibooks.org/wiki/LaTeX/Importing\_Graphics\#Including\_graphics}. \url{https://en.wikibooks.org/wiki/LaTeX/Importing\_Graphics\#Including\_graphics}.
\subsection{Grid figures} ## Grid figures
Including more than two EPS/PDF files in a single figure call can be tricky to Including more than two EPS/PDF files in a single figure call can be tricky to
easily format. To make the process easier for authors \aastex\ v6 offers easily format. To make the process easier for authors \aastex v6 offers
{\tt\string\gridline} which allows any number of individual EPS/PDF file {\tt\string\gridline} which allows any number of individual EPS/PDF file
calls within a single figure. Each file cited in a {\tt\string\gridline} calls within a single figure. Each file cited in a {\tt\string\gridline}
will be displayed in a row. By adding more {\tt\string\gridline} calls an will be displayed in a row. By adding more {\tt\string\gridline} calls an
@ -1338,7 +1312,7 @@ next two will right and left justify the image, respectively. The
{\tt\string\boxedfig} is similar to {\tt\string\fig} except that a box is {\tt\string\boxedfig} is similar to {\tt\string\fig} except that a box is
drawn around the figure file when displayed. Each of these commands takes drawn around the figure file when displayed. Each of these commands takes
three arguments. The first is the file name. The second is the width that three arguments. The first is the file name. The second is the width that
file should be displayed at. While any natural \latex\ unit is allowed, it file should be displayed at. While any natural \latex unit is allowed, it
is recommended that author use fractional units with the is recommended that author use fractional units with the
{\tt\string\textwidth}. The last argument is text for a subcaption. {\tt\string\textwidth}. The last argument is text for a subcaption.
@ -1361,7 +1335,7 @@ KT Eri. These individual figures are taken from \citet{2011ApJS..197...31S}.
\label{fig:pyramid}} \label{fig:pyramid}}
\end{figure*} \end{figure*}
\subsection{Enhanced graphics} ## Enhanced graphics
Enhanced graphics have an example figure to serve as an example for the Enhanced graphics have an example figure to serve as an example for the
reader and the full graphical item available in the published HTML article. reader and the full graphical item available in the published HTML article.
@ -1375,7 +1349,7 @@ March 2021 there are over 4000 videos, 1300 figure sets, and 100 interactive
figures. The next sections describe how to include these types of graphics figures. The next sections describe how to include these types of graphics
in your own manuscripts. in your own manuscripts.
\subsubsection{Figure sets} ### Figure sets
The grid commands given above works great for a limited set of individual The grid commands given above works great for a limited set of individual
figure files but what do you do if you have many 10s or 100s or even 1000s of figure files but what do you do if you have many 10s or 100s or even 1000s of
@ -1390,10 +1364,10 @@ terms of reduced publication charges, see Appendix B. All of the figure set
components, along with their html framework, are also available to the reader components, along with their html framework, are also available to the reader
for download in a single .tar.gz package. for download in a single .tar.gz package.
Special \latex\ mark up is required to create a figure set. Prior to Special \latex mark up is required to create a figure set. Prior to
\aastex\ v6 the underlying mark up commands had to be inserted by hand \aastex v6 the underlying mark up commands had to be inserted by hand
but is now included. Note that when an article with figure set is compiled but is now included. Note that when an article with figure set is compiled
in \latex\ none of the component figures are shown and a floating Figure in \latex none of the component figures are shown and a floating Figure
Set caption will appear in the resulting PDF. Set caption will appear in the resulting PDF.
\figsetstart \figsetstart
@ -1464,9 +1438,9 @@ The example figure shown for figure sets can be one component or many.
Authors are encouraged to use an online tool at Authors are encouraged to use an online tool at
\url{http://authortools.aas.org/FIGSETS/make-figset.html} to generate their \url{http://authortools.aas.org/FIGSETS/make-figset.html} to generate their
own specific figure set mark up to incorporate into their \latex\ articles. own specific figure set mark up to incorporate into their \latex articles.
\subsubsection{Animations \label{animation}} ### Animations
Authors may, and are in fact encouraged, to include animations in their Authors may, and are in fact encouraged, to include animations in their
manuscripts. The video will stream inline with the published article and manuscripts. The video will stream inline with the published article and
@ -1508,7 +1482,7 @@ summer of 2019}. If these types are not provide the compiler will issue an
error and quit. The second argument is the file that produces the enhanced error and quit. The second argument is the file that produces the enhanced
feature in the HTML article. feature in the HTML article.
\subsubsection{Interactive figures \label{sec:interactive}} ### Interactive figures
Interactive figures give the reader the ability to manipulate the Interactive figures give the reader the ability to manipulate the
information contained in an image which can add clarity or help further the information contained in an image which can add clarity or help further the
@ -1557,10 +1531,10 @@ Authors should consult the online tutorials at
for more information on what is currently supported and links to for more information on what is currently supported and links to
tutorials and examples. tutorials and examples.
\section{Displaying mathematics} \label{sec:displaymath} # Displaying mathematics
The most common mathematical symbols and formulas are in the amsmath The most common mathematical symbols and formulas are in the amsmath
package. \aastex\ requires this package so there is no need to package. \aastex requires this package so there is no need to
specifically call for it in the document preamble. Most modern \latex\ specifically call for it in the document preamble. Most modern \latex\
distributions already contain this package. If you do not have this distributions already contain this package. If you do not have this
package or the other required packages, revtex4-1, latexsym, graphicx, package or the other required packages, revtex4-1, latexsym, graphicx,
@ -1581,14 +1555,14 @@ follows.
where $p$ and $\sigma$ label the initial $e^{\pm}$ four-momenta where $p$ and $\sigma$ label the initial $e^{\pm}$ four-momenta
and helicities $(\sigma = \pm 1)$, $\hat a_i=a^\mu_i\gamma_\nu$ and helicities $(\sigma = \pm 1)$, $\hat a_i=a^\mu_i\gamma_\nu$
and $P_\tau=\frac{1}{2}(1+\tau\gamma_5)$ is a chirality projection and $P_\tau=\frac{1}{2}(1+\tau\gamma_5)$ is a chirality projection
operator $(\tau = \pm1)$. This produces a single line formula. \latex\ will operator $(\tau = \pm1)$. This produces a single line formula. \latex will
auto-number this and any subsequent equations. If no number is desired then auto-number this and any subsequent equations. If no number is desired then
the {\tt\string equation} call should be replaced with {\tt\string displaymath}. the {\tt\string equation} call should be replaced with {\tt\string displaymath}.
\latex\ can also handle a a multi-line equation. Use {\tt\string eqnarray} \latex can also handle a a multi-line equation. Use {\tt\string eqnarray}
for more than one line and end each line with a for more than one line and end each line with a
\textbackslash\textbackslash. Each line will be numbered unless the \textbackslash\textbackslash. Each line will be numbered unless the
\textbackslash\textbackslash\ is preceded by a {\tt\string\nonumber} \textbackslash\textbackslash is preceded by a {\tt\string\nonumber}
command. Alignment points can be added with ampersands (\&). There should be command. Alignment points can be added with ampersands (\&). There should be
two ampersands per line. In the examples they are centered on the equal two ampersands per line. In the examples they are centered on the equal
symbol. symbol.
@ -1621,10 +1595,10 @@ symbol.
%% of being numbered, say, (4) and (5), would be numbered (4a) and (4b). %% of being numbered, say, (4) and (5), would be numbered (4a) and (4b).
%% LaTeX the paper and look at the output to see the results. %% LaTeX the paper and look at the output to see the results.
\section{Revision tracking and color highlighting} \label{sec:highlight} # Revision tracking and color highlighting
Authors sometimes use color to highlight changes to their manuscript in Authors sometimes use color to highlight changes to their manuscript in
response to editor and referee comments. In \aastex\ new commands response to editor and referee comments. In \aastex new commands
have been introduced to make this easier and formalize the process. have been introduced to make this easier and formalize the process.
The first method is through a new set of editing mark up commands that The first method is through a new set of editing mark up commands that
@ -1682,7 +1656,7 @@ to mark up text that they are not sure should appear in the final
manuscript or as a way to communicate comments between co-authors when manuscript or as a way to communicate comments between co-authors when
writing the article. writing the article.
\section{Software and third party data repository citations} \label{sec:cite} # Software and third party data repository citations
The AAS Journals would like to encourage authors to change software and The AAS Journals would like to encourage authors to change software and
third party data repository references from the current standard of a third party data repository references from the current standard of a
@ -1706,7 +1680,7 @@ article references the external code at
not have specific bibtex entries for these types of references so the not have specific bibtex entries for these types of references so the
``@misc'' type should be used. The Repository tutorial explains how to ``@misc'' type should be used. The Repository tutorial explains how to
code the ``@misc'' type correctly. The most recent aasjournal.bst file, code the ``@misc'' type correctly. The most recent aasjournal.bst file,
available with \aastex\ v6, will output bibtex ``@misc'' type properly. available with \aastex v6, will output bibtex ``@misc'' type properly.
%% IMPORTANT! The old "\acknowledgment" command has be depreciated. It was %% IMPORTANT! The old "\acknowledgment" command has be depreciated. It was
%% not robust enough to handle our new dual anonymous review requirements and %% not robust enough to handle our new dual anonymous review requirements and
@ -1759,7 +1733,7 @@ CTIO:1.5m,CXO}
\appendix \appendix
\section{Appendix information} # Appendix information
Appendices can be broken into separate sections just like in the main text. Appendices can be broken into separate sections just like in the main text.
The only difference is that each appendix section is indexed by a letter The only difference is that each appendix section is indexed by a letter
@ -1771,7 +1745,7 @@ I = \frac{1}{1 + d_{1}^{P (1 + d_{2} )}}
Appendix tables and figures should not be numbered like equations. Instead Appendix tables and figures should not be numbered like equations. Instead
they should continue the sequence from the main article body. they should continue the sequence from the main article body.
\section{Author publication charges} \label{sec:pubcharge} # Author publication charges
Finally some information about the AAS Journal's publication charges. Finally some information about the AAS Journal's publication charges.
In April 2011 the traditional way of calculating author charges based on In April 2011 the traditional way of calculating author charges based on
@ -1787,7 +1761,7 @@ Authors may use the ApJL length calculator to get a {\tt rough} estimate of
the number of word and float quanta in their manuscript. The calculator the number of word and float quanta in their manuscript. The calculator
is located at \url{https://authortools.aas.org/ApJL/betacountwords.html}. is located at \url{https://authortools.aas.org/ApJL/betacountwords.html}.
\section{Rotating tables} \label{sec:rotate} # Rotating tables
The process of rotating tables into landscape mode is slightly different in The process of rotating tables into landscape mode is slightly different in
\aastex v6.31. Instead of the {\tt\string\rotate} command, a new environment \aastex v6.31. Instead of the {\tt\string\rotate} command, a new environment
@ -1888,15 +1862,15 @@ V838 Her & 5 (197) & 2448340.5 (197) & 2 (198) & \nodata & 0.5$\pm0.1$ (198) & 2
\end{deluxetable*} \end{deluxetable*}
\end{longrotatetable} \end{longrotatetable}
A handy "cheat sheet" that provides the necessary \latex\ to produce 17 A handy "cheat sheet" that provides the necessary \latex to produce 17
different types of tables is available at \url{http://journals.aas.org/authors/aastex/aasguide.html#table_cheat_sheet}. different types of tables is available at \url{http://journals.aas.org/authors/aastex/aasguide.html#table_cheat_sheet}.
\section{IAU recommendations for nominal units \label{nominal}} # IAU recommendations for nominal units
The IAU 2015 resolution B3 defines nominal solar and planetary values by The IAU 2015 resolution B3 defines nominal solar and planetary values by
establishing conversions between solar and planetary values and SI units. establishing conversions between solar and planetary values and SI units.
The rational and specifications are given in \citet{2016AJ....152...41P}. The rational and specifications are given in \citet{2016AJ....152...41P}.
The recommended nominal conversion constants for \latex\ have been The recommended nominal conversion constants for \latex have been
incorporate into v6.31 to help authors follow the IAU resolution. incorporate into v6.31 to help authors follow the IAU resolution.
The general commands take this form: The general commands take this form:
@ -1951,7 +1925,7 @@ parameter\\
All of these commands work equally well in text and math mode. All of these commands work equally well in text and math mode.
\section{Using Chinese, Japanese, and Korean characters} # Using Chinese, Japanese, and Korean characters
Authors have the option to include names in Chinese, Japanese, or Korean (CJK) Authors have the option to include names in Chinese, Japanese, or Korean (CJK)
characters in addition to the English name. The names will be displayed characters in addition to the English name. The names will be displayed
@ -1959,28 +1933,3 @@ in parentheses after the English name. The way to do this in AASTeX is to
use the CJK package available at \url{https://ctan.org/pkg/cjk?lang=en}. use the CJK package available at \url{https://ctan.org/pkg/cjk?lang=en}.
Further details on how to implement this and solutions for common problems, Further details on how to implement this and solutions for common problems,
please go to \url{https://journals.aas.org/nonroman/}. please go to \url{https://journals.aas.org/nonroman/}.
%% For this sample we use BibTeX plus aasjournals.bst to generate the
%% the bibliography. The sample631.bib file was populated from ADS. To
%% get the citations to show in the compiled file do the following:
%%
%% pdflatex sample631.tex
%% bibtext sample631
%% pdflatex sample631.tex
%% pdflatex sample631.tex
\bibliography{sample631}{}
\bibliographystyle{aasjournal}
%% This command is needed to show the entire author+affiliation list when
%% the collaboration and author truncation commands are used. It has to
%% go at the end of the manuscript.
%\allauthors
%% Include this line if you are using the \added, \replaced, \deleted
%% commands to see a summary list of all changes at the end of the article.
%\listofchanges
\end{document}
% End of file `sample631.tex'.

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