#aastexopts: [singlecolumn] preambleinput: ["macros.tex"] bibstyle: aasjournal received: "January 1, 2018" revised: "January 7, 2018" accepted: "\today" submitjournal: ApJ title: "An Example Article using \aastex v6.2^[Released on January, 8th, 2018]" shorttitle: Sample article shortauthors: Schwarz et al. author:

name: Greg J. Schwarz ORCID: 0000-0002-0786-7307 affiliation: ["American Astronomical Society \ 2000 Florida Ave., NW, Suite 300 \ Washington, DC 20009-1231, USA"]
name: August Muench affiliation: ["American Astronomical Society \ 2000 Florida Ave., NW, Suite 300 \ Washington, DC 20009-1231, USA"] collaboration: "(AAS Journals Data Scientists collaboration)"
name: Butler Burton affiliation: ["National Radio Astronomy Observatory", "AAS Journals Associate Editor-in-Chief"] nocollaboration: 1
name: Amy Hendrickson affiliation: ["TeXnology Inc."] collaboration: "(LaTeX collaboration)"
name: Julie Steffen affiliation: ["AAS Director of Publishing", "American Astronomical Society \ 2000 Florida Ave., NW, Suite 300 \ Washington, DC 20009-1231, USA"]
name: Jeff Lewandowski affiliation: ["IOP Senior Publisher for the AAS Journals", "IOP Publishing, Washington, DC 20005"] keywords: ["editorials, notices", miscellaneous, catalogs, surveys] software: ["pandoc", "astropy [@astropy2013]", "Cloudy [@Ferland2013]", "SExtractor [@Bertin1996]"] facility: ["HST(STIS)", "Swift(XRT and UVOT)", "AAVSO", "CTIO:1.3m", "CTIO:1.5m", "CXO"] abstract: | 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 includes a history of \aastex\ and documents the new features in the previous versions as well as the new features in version 6.2. This manuscript includes many figure and table examples to illustrate these new features. Information on features not explicitly mentioned in the article can be viewed in the manuscript comments or more extensive online documentation. Authors are welcome replace the text, tables, figures, and bibliography with their own and submit the resulting manuscript to the AAS Journals peer review system. The first lesson in the tutorial is to remind authors that the AAS Journals, the Astrophysical Journal (ApJ), the Astrophysical Journal Letters (ApJL), and Astronomical Journal (AJ), all have a 250 word limit for the abstract^[Note that manuscripts submitted to the new Research Notes of the American Astronomical Society (RNAAS) do not have abstracts.]. If you exceed this length the Editorial office will ask you to shorten it. ---

Introduction {#sec:intro}

\latex\ ^[http://www.latex-project.org/] is a document markup language that is particularly well suited for the publication of mathematical and scientific articles [@lamport94]. \latex\ was written 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 \latex\ macros were developed to investigate electronic submission and publication of AAS Journal articles [@1989BAAS...21..780H]. Shortly afterwards, Chris Biemesdefer merged these macros and more into a \latex\ 2.08 style file called \aastex. These early \aastex\ versions introduced many common commands and practices that authors take for granted today. Substantial revisions 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 which uses the document class in lieu of a style file. Other improvements to version 5 included hypertext support, landscape deluxetables and improved figure support to facilitate electronic submission. \aastex\ v5.2 was released in 2005 and introduced additional graphics support plus new mark up to identifier astronomical objects, datasets and facilities.

In 1996 Maxim Markevitch modified the AAS preprint style file, aaspp4.sty, to closely emulate the very tight, two column style of a typeset Astrophysical Journal article. The result was emulateapj.sty. A year later Alexey Vikhlinin took over development and maintenance. In 2001 he converted emulateapj into a class file in \latex\ 2e and in 2003 Vikhlinin completely rewrote emulateapj based on the APS Journal's RevTEX class.

During this time emulateapj gained growing acceptance in the astronomical community as it filled an author need to obtain an approximate number of manuscript pages prior to submission for cost and length estimates. The tighter typeset also had the added advantage of saving paper when printing out hard copies.

Even though author publication charges are no longer based on print pages^[see Section \ref{sec:pubcharge} in the Appendix for more details about how current article costs are calculated.] the emulateapj class file has proven to be extremely popular with AAS Journal authors. An informal analysis of submitted \latex\ manuscripts in 2015 revealed that $\sim$ 65\% either called emulateapj or have a commented emulateapj classfile call indicating it was used at some stage of the manuscript construction. Clearly authors want to have access to a tightly typeset version of the article when corresponding with co-authors and for preprint submissions.

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 modify emulateapj for \aastex\ v6.+ instead. The change brings \aastex\ inline with what the majority of authors are already using while still delivering new and improved features. \aastex\ v6.0 through v6.2 were written by Amy Hendrickson and released in January 2016 (v6.0), October 2016 (v6.1), and January 2018 (v6.2), respectively. Some of the new features in v6.0 included:

improved citations for third party data repositories and software,
easier construction of matrix figures consisting of multiple encapsulated postscript (EPS) or portable document format (PDF) files,
figure set mark up for large collections of similar figures,
color mark up to easily enable/disable revised text highlighting,
improved url support, and
numerous table options such as the ability to hide columns, column decimal alignment, automatic column math mode and numbering, plus splitting of wide tables.

The features in v6.1 were:

ORCID support for preprints,
improved author, affiliation and collaboration mark up,
reintroduced the old AASTeX v5.2 \received, \revised, \accepted, and \published commands plus added the new \submitjournal command to document which AAS Journal the manuscript was submitted to, plus
new typeset style options.

The new features in v6.2 are:

A new RNAAS style option for Research Note manuscripts,
Titles no longer put in all caps,
No page skip between the title page and article body,
re-introduce RevTeX's widetext environment for long lines in two column style formats, and
upgrade to the \doi command.

The rest of this article provides information and examples on how to create your own AAS Journal manuscript with v6.2. Special emphasis is placed on how to use the full potential of \aastex\ v6+. The next section describes the different manuscript styles available and how they differ from past releases. Section \ref{sec:floats} describes how tables and figures are placed in a \latex\ document. Specific examples of tables, Section \ref{subsec:tables}, and figures, Section \ref{subsec:figures}, are also provided. Section \ref{sec:displaymath} discusses how to display math and incorporate equations in a manuscript while Section \ref{sec:highlight} discuss how to use the new revision mark up. The last section, \ref{sec:cite}, shows how recognize software and external data as first class references in the manuscript bibliography. An appendix is included to show how to construct one and provide some information on how article charges are calculated. Additional information is available both embedded in the comments of this \latex\ file and in the online documentation at http://journals.aas.org/authors/aastex.html.

Manuscript styles {#sec:style}

The default style in \aastex\ v6.2 is a tight single column style, e.g. 10 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 since figures and tables, see Section \ref{sec:floats}, will span the entire page, reducing the need for address float sizing.

To invoke a two column style similar to the what is produced in the published PDF copy use

\noindent \documentclass[twocolumn]{aastex62}.

\noindent Note that in the two column style figures and tables will only span one column unless specifically ordered across both with the "*" flag, e.g.

\noindent\begin{figure*} ... \end{figure*}, \ \noindent\begin{table*} ... \end{table*}, and \ \noindent\begin{deluxetable*} ... \end{deluxetable*}.

\noindent This option is ignored in the onecolumn style.

Some other style options are outlined in the commented sections of this article. Any combination of style options can be used.

Two style options that are needed to fully use the new revision tracking feature, see Section \ref{sec:highlight}, are linenumbers which uses the lineno style file to number each article line in the left margin and trackchanges which controls the revision and commenting highlight output.

There is also a new modern option that uses a Daniel Foreman-Mackey and David Hogg design to produce stylish, single column output that has wider left and right margins. It is designed to have fewer words per line to improve reader retention. It also looks better on devices with smaller displays such as smart phones.

For a Research Note use the RNAAS option which will produce a manuscript with no abstract and in the modern style.

Floats {#sec:floats}

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 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 there is not enough room at that location, hence the term "float".

Authors are encouraged to embed their tables and figures within the text as they are mentioned. Please do not place the figures and text at the end of the article as was the old practice. Editors and the vast majority of referees find it much easier to read a manuscript with embedded figures and tables.

Depending on the number of floats and the particular amount of text and equations present in a manuscript the ultimate location of any specific float can be hard to predict prior to compilation. It is recommended that authors textbf{not} spend significant time trying to get float placement perfect for peer review. The AAS Journal's publisher has sophisticated typesetting software that will produce the optimal layout during production.

Note that authors of Research Notes are only allowed one float, either one table or one figure.

\startlongtable \begin{deluxetable}{c|cc} \tablecaption{ApJ costs from 1991 to 2013\tablenotemark{a} \label{tab:table}} \tablehead{ \colhead{Year} & \colhead{Subscription} & \colhead{Publication} \ \colhead{} & \colhead{cost} & \colhead{charges\tablenotemark{b}}\ \colhead{} & \colhead{(\$)} & \colhead{(\$/page)} } \colnumbers \startdata 1991 & 600 & 100 \ 1992 & 650 & 105 \ 1993 & 550 & 103 \ 1994 & 450 & 110 \ 1995 & 410 & 112 \ 1996 & 400 & 114 \ 1997 & 525 & 115 \ 1998 & 590 & 116 \ 1999 & 575 & 115 \ 2000 & 450 & 103 \ 2001 & 490 & 90 \ 2002 & 500 & 88 \ 2003 & 450 & 90 \ 2004 & 460 & 88 \ 2005 & 440 & 79 \ 2006 & 350 & 77 \ 2007 & 325 & 70 \ 2008 & 320 & 65 \ 2009 & 190 & 68 \ 2010 & 280 & 70 \ 2011 & 275 & 68 \ 2012 & 150 & 56 \ 2013 & 140 & 55 \ \enddata \tablenotetext{a}{Adjusted for inflation} \tablenotetext{b}{Accounts for the change from page charges to digital quanta in April, 2011} \tablecomments{Note that {\tt \string \colnumbers} does not work with the vertical line alignment token. If you want vertical lines in the headers you can not use this command at this time.} \end{deluxetable}

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 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, see Table \ref{tab:table}. A better method is to force \latex\ to place a float in a general area with the use of the optional [placement specifier] parameter for figures and tables. This parameter goes after \begin{figure}, \begin{table}, and \begin{deluxetable}. The main arguments the specifier takes 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 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 calculating the float position. A sequence of rules can be created by using multiple arguments. For example, \begin{figure}[htb!] 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 proper position should be. Many of the tables and figures in this article use a placement specifier to set their positions.

Note that the \latex\ tabular environment is not a float. Only when a tabular is surrounded by \begin{table} ... \end{table} is it a true float and the rules and suggestions above apply.

In AASTeX v6.2 all deluxetables are float tables and thus if they are longer than a page will spill off the bottom. Long deluxetables should begin with the \startlongtable command. This initiates a longtable environment. Authors might have to use \clearpage to isolate a long table or optimally place it within the surrounding text.

\begin{deluxetable}{ccCrlc}[b!] \tablecaption{Column math mode in an observation log \label{tab:mathmode}} \tablecolumns{6} \tablenum{2} \tablewidth{0pt} \tablehead{ \colhead{UT start time\tablenotemark{a}} & \colhead{MJD start time\tablenotemark{a}} & \colhead{Seeing} & \colhead{Filter} & \colhead{Inst.} \ \colhead{(YYYY-mm-dd)} & \colhead{(d)} & \colhead{(arcsec)} & \colhead{} & \colhead{} } \startdata 2012-03-26 & 56012.997 & \sim 0.\arcsec5 & H$\alpha$ & NOT \ 2012-03-27 & 56013.944 & 1.\arcsec5 & grism & SMARTS \ 2012-03-28 & 56014.984 & \nodata & F814M & HST \ 2012-03-30 & 56016.978 & 1.\arcsec5\pm0.25 & B&C & Bok \ \enddata \tablenotetext{a}{At exposure start.} \tablecomments{The "C" command column identifier in the 3 column turns on math mode for that specific column. One could do the same for the next column so that dollar signs would not be needed for H$\alpha$ but then all the other text would also be in math mode and thus typeset in Latin Modern math and you will need to put it back to Roman by hand. Note that if you do change this column to math mode the dollar signs already present will not cause a problem. Table \ref{tab:mathmode} is published in its entirety in the machine readable format. A portion is shown here for guidance regarding its form and content.} \end{deluxetable}

Tables {#subsec:tables}

Tables can be constructed with \latex's standard table environment or the \aastex's deluxetable environment. The deluxetable construct handles long tables better but has a larger overhead due to the greater amount of defined mark up used set up and manipulate the table structure. The choice of which to use is up to the author. Examples of both environments are used in this manuscript. Table \ref{tab:table} is a simple deluxetable example that gives the approximate changes in the subscription costs and author publication charges from 1991 to 2013.

Tables longer than 200 data lines and complex tables should only have a short example table with the full data set available in the machine readable format. The machine readable table will be available in the HTML version of the article with just a short example in the PDF. Authors are required to indicate to the reader where the data can be obtained in the table comments. Suggested text is given in the comments of Table \ref{tab:mathmode}. Authors are encouraged to create their own machine readable tables using the online tool at http://authortools.aas.org/MRT/upload.html.

\aastex\ v6 introduces five new table features that are designed to make table construction easier and the resulting display better for AAS Journal authors. The items are:

Declaring math mode in specific columns,
Column decimal alignment,
Automatic column header numbering,
Hiding columns, and
Splitting wide tables into two or three parts.

Each of these new features are illustrated in following Table examples. All five features work with the regular \latex\ tabular environment and in \aastex's deluxetable environment. The examples in this manuscript also show where the two process differ.

Column math mode

Both the \latex\ tabular and \aastex\ deluxetable require an argument to define the alignment and number of columns. The most common values are "c", "l" and "r" for \underline{c}enter, \underline{l}eft, and \underline{r}ight justification. If these values are capitalized, e.g. "C", "L", or "R", then that specific column will automatically be in math mode meaning that \$s are not required. Note that having embedded dollar signs in the table does not affect the output. The third and forth columns of Table \ref{tab:mathmode} shows how this math mode works.

Decimal alignment

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 in the data, e.g. \phn, to align columns by hand but this can be tedious in long or complex tables. To address this \aastex\ introduces the \decimals command and a new column justification option, "D", to align data in that column on the decimal. In deluxetable the \decimals command is invoked before the \startdata call but can be anywhere in \latex's tabular environment.

Two other important thing to note when using decimal alignment is that each decimal column \textit{must end with a space before the ampersand}, e.g. "&&" is not allowed. Empty decimal columns are indicated with a decimal, e.g. ".". Do not use deluxetable's \nodata command.

The "D" alignment token works by splitting the column into two parts on the decimal. While this is invisible to the user one must be aware of how it 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 done with a multicolumn call, e.g \multicolumn2c{} or \multicolumn{2}{c}{}, or use the new \twocolhead{} command in deluxetable. Since \latex\ is 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 \latex\ compiler twice to get it right. Table \ref{tab:decimal} illustrates how decimal alignment works in the tabular environment with a $\pm$ symbol embedded between the last two columns.

\setcounter{table}{2} \begin{table}[h!] \centering \caption{Decimal alignment made easy} \label{tab:decimal} \begin{tabular}{cD@{$\pm$}D} \tablewidth{0pt} \hline \hline Column & \multicolumn2c{Value} & \multicolumn2c{Uncertainty}\ \hline \decimals A & 1234 & 100.0 \ B & 123.4 & 10.1 \ C & 12.34 & 1.01 \ D & 1.234 & 0.101 \ E & .1234 & 0.01001 \ F & 1.0 & . \ \hline \multicolumn{5}{c}{NOTE. - Two decimal aligned columns} \end{tabular} \end{table}

\subsubsection{Automatic column header numbering} \label{subsubsec:autonumber}

The command \colnumbers can be included to automatically number 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 a \latex\ tabular environment the \colnumbers should be invoked 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 has to come before \startdata. \colnumbers will not increment for columns hidden by the "h" command, see Section \ref{subsubsec:hide}. Table \ref{tab:table} uses this command to automatically generate column index numbers.

Note that when using decimal alignment in a table the command \decimalcolnumbers must be used instead of \colnumbers and \decimals. Table \ref{tab:messier} illustrates this specific functionality.

Hiding columns {#subsubsec:hide}

Entire columns can be \underline{h}idden from display simply by changing the specified column identifier to "h". In the \latex\ tabular environment this column identifier conceals the entire column including the header columns. In \aastex's deluxetables the header row is specifically declared with the \tablehead call and each header column is marked with \colhead call. In order to make a specific header disappear with the "h" column identifier in deluxetable use \nocolhead instead to suppress that particular column header.

Authors can use this option in many different ways. Since column data can 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 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 it fits on a page. This concealed column table would serve as the example table for the full machine readable version. Regardless of how columns are obscured, authors are responsible for removing any unneeded column data or alerting the editorial office about how to treat these columns during production for the final typeset article.

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 together. It has automatic column numbering, decimal alignment of the distances, and one concealed column. The Common name column 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 the column identifier preamble to another valid value. This table also uses \tablenum to renumber the table because a \latex\ tabular table was inserted before it.

\begin{deluxetable}{cchlDlc} \tablenum{4} \tablecaption{Fun facts about the first 10 messier objects\label{tab:messier}} \tablewidth{0pt} \tablehead{ \colhead{Messier} & \colhead{NGC/IC} & \nocolhead{Common} & \colhead{Object} & \multicolumn2c{Distance} & \colhead{} & \colhead{V} \ \colhead{Number} & \colhead{Number} & \nocolhead{Name} & \colhead{Type} & \multicolumn2c{(kpc)} & \colhead{Constellation} & \colhead{(mag)} } \decimalcolnumbers \startdata M1 & NGC 1952 & Crab Nebula & Supernova remnant & 2 & Taurus & 8.4 \ M2 & NGC 7089 & Messier 2 & Cluster, globular & 11.5 & Aquarius & 6.3 \ M3 & NGC 5272 & Messier 3 & Cluster, globular & 10.4 & Canes Venatici & 6.2 \ M4 & NGC 6121 & Messier 4 & Cluster, globular & 2.2 & Scorpius & 5.9 \ M5 & NGC 5904 & Messier 5 & Cluster, globular & 24.5 & Serpens & 5.9 \ M6 & NGC 6405 & Butterfly Cluster & Cluster, open & 0.31 & Scorpius & 4.2 \ M7 & NGC 6475 & Ptolemy Cluster & Cluster, open & 0.3 & Scorpius & 3.3 \ 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 \ M10 & NGC 6254 & Messier 10 & Cluster, globular & 4.42 & Ophiuchus & 6.4 \ \enddata \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 alignment you need to include the \decimals command before \\startdata and all of the values in that column have to have a space before the next ampersand.} \end{deluxetable}

\subsubsection{Splitting a table into multiple horizontal components}

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. However, there are some artificial limitations based on the width of a print page. The old way around this limitation was to rotate into landscape mode and use the smallest available table font sizes, e.g. \tablewidth, to get the table to fit. Unfortunately, this was not alway enough but now along with the hide column option outlined in Section \ref{subsubsec:hide} there is a new way to break a table into two or three components so that it flows down a page by invoking a new table type, splittabular or splitdeluxetable. Within these tables a new "B" column separator is introduced. Much like the vertical bar option, "$\vert$", that produces a vertical table lines, e.g. Table \ref{tab:table}, the new "B" separator indicates where to \underline{B}reak a table. Up to two "B"s may be included.

Table 5 % \ref{tab:deluxesplit} this freaks it out when it is used! shows how to split a wide deluxetable into three parts with the \splitdeluxetable command. The \colnumbers option is on to show how the automatic column numbering carries through the second table component, see Section \ref{subsubsec:autonumber}.

The last example, Table \ref{tab:tablesplit}, shows how to split the same table but with a regular \latex\ tabular call and into two parts. Decimal alignment is included in the third column and the "Component" column is hidden to illustrate the new features working together.

\begin{splitdeluxetable*}{lccccBcccccBcccc} \tabletypesize{\scriptsize} \tablewidth{0pt} \tablenum{5} \tablecaption{Measurements of Emission Lines: two breaks \label{tab:deluxesplit}} \tablehead{ \colhead{Model} & \colhead{Component}& \colhead{Shift} & \colhead{FWHM} & \multicolumn{10}{c}{Flux} \ \colhead{} & \colhead{} & \colhead{($\rm km~s^{-1}$)}& \colhead{($\rm km~s^{-1}$)} & \multicolumn{10}{c}{($\rm 10^{-17}~erg~s^{-1}~cm^{-2}$)} \ \cline{5-14} \colhead{} & \colhead{} & \colhead{} & \colhead{} & \colhead{Ly$\alpha$} & \colhead{N\,{\footnotesize V}} & \colhead{Si\,{\footnotesize IV}} & \colhead{C\,{\footnotesize IV}} & \colhead{Mg\,{\footnotesize II}} & \colhead{H$\gamma$} & \colhead{H$\beta$} & \colhead{H$\alpha$} & \colhead{He\,{\footnotesize I}} & \colhead{Pa$\gamma$} } \colnumbers \startdata { }& BELs& -97.13 & 9117$\pm 38$& 1033$\pm 33$&$< 35$&$< 166$& 637$\pm 31$& 1951$\pm 26$& 991$\pm 30$& 3502$\pm 42$& 20285$\pm 80$& 2025$\pm 116$& 1289$\pm 107$\ {Model 1}& IELs& -4049.123 & 1974$\pm 22$& 2495$\pm 30$&$< 42$&$< 109$& 995$\pm 186$& 83$\pm 30$& 75$\pm 23$& 130$\pm 25$& 357$\pm 94$& 194$\pm 64$& 36$\pm 23$\ { }& NELs& \nodata & 641$\pm 4$& 449$\pm 23$&$< 6$&$< 9$& -- & 275$\pm 18$& 150$\pm 11$& 313$\pm 12$& 958$\pm 43$& 318$\pm 34$& 151$\pm 17$\ \hline { }& BELs& -85 & 8991$\pm 41$& 988$\pm 29$&$< 24$&$< 173$& 623$\pm 28$& 1945$\pm 29$& 989$\pm 27$& 3498$\pm 37$& 20288$\pm 73$& 2047$\pm 143$& 1376$\pm 167$\ {Model 2}& IELs& -51000 & 2025$\pm 26$& 2494$\pm 32$&$< 37$&$< 124$& 1005$\pm 190$& 72$\pm 28$& 72$\pm 21$& 113$\pm 18$& 271$\pm 85$& 205$\pm 72$& 34$\pm 21$\ { }& NELs& 52 & 637$\pm 10$& 477$\pm 17$&$< 4$&$< 8$& -- & 278$\pm 17$& 153$\pm 10$& 317$\pm 15$& 969$\pm 40$& 325$\pm 37$&

 147$\pm       22$\\

\enddata \tablecomments{This is an example of how to split a deluxetable. You can 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" indicators in the column identifier preamble. For more information please look at the new \aastex\ instructions.} \end{splitdeluxetable*}

%\clearpage

\setcounter{table}{5} \begin{table}[h!] \caption{Measurements of Emission Lines: one break\label{tab:tablesplit}} \begin{splittabular}{lhDccccBccccccc} %\multicolumn{5}{c}{Table 6} \ %\multicolumn{5}{c}{Measurements of Emission Lines} \ \hline \hline Model & Component & \multicolumn2c{Shift} & FWHM & \multicolumn{10}{c}{Flux} \ & & \multicolumn2c{($\rm km~s^{-1}$)} & {($\rm km~s^{-1}$)} & \multicolumn{10}{c}{($\rm 10^{-17}~erg~s^{-1}~cm^{-2}$)} \ \cline{5-15} & & & & & {Ly$\alpha$} & {N\,{\footnotesize V}} & {Si\,{\footnotesize IV}} & {C\,{\footnotesize IV}} & {Mg\,{\footnotesize II}} & {H$\gamma$} & {H$\beta$} & {H$\alpha$} & {He\,{\footnotesize I}} & {Pa$\gamma$} \ %\hline \decimalcolnumbers & BELs& -97.13 & 9117$\pm 38$& 1033$\pm 33$&$< 35$&$< 166$& 637$\pm 31$& 1951$\pm 26$& 991$\pm 30$& 3502$\pm 42$& 20285$\pm 80$& 2025$\pm 116$& 1289$\pm 107$\ Model 1 & IELs& -4049.123 & 1974$\pm 22$& 2495$\pm 30$&$< 42$&$< 109$& 995$\pm 186$& 83$\pm 30$& 75$\pm 23$& 130$\pm 25$& 357$\pm 94$& 194$\pm 64$& 36$\pm 23$\ & NELs& . & 641$\pm 4$& 449$\pm 23$&$< 6$&$< 9$& -- & 275$\pm 18$& 150$\pm 11$& 313$\pm 12$& 958$\pm 43$& 318$\pm 34$& 151$\pm 17$\ \hline & BELs& -85 & 8991$\pm 41$& 988$\pm 29$&$< 24$&$< 173$& 623$\pm 28$& 1945$\pm 29$& 989$\pm 27$& 3498$\pm 37$& 20288$\pm 73$& 2047$\pm 143$& 1376$\pm 167$\ Model 2 & IELs& -51000 & 2025$\pm 26$& 2494$\pm 32$&$< 37$&$< 124$& 1005$\pm 190$& 72$\pm 28$& 72$\pm 21$& 113$\pm 18$& 271$\pm 85$& 205$\pm 72$& 34$\pm 21$\ & NELs& 52 & 637$\pm 10$& 477$\pm 17$&$< 4$&$< 8$& -- & 278$\pm 17$& 153$\pm 10$& 317$\pm 15$& 969$\pm 40$& 325$\pm 37$& 147$\pm 22$\ \hline \end{splittabular} \end{table}

demo.md 30 KB 履歴 Raw