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+%% This is emulateapj reformatting of the AASTEX sample document
+%%
+\documentclass{emulateapj}
+
+\newcommand{\vdag}{(v)^\dagger}
+\newcommand{\myemail}{skywalker@galaxy.far.far.away}
+
+%% You can insert a short comment on the title page using the command below.
+
+\slugcomment{Not to appear in Nonlearned J., 45.}
+
+%% If you wish, you may supply running head information, although
+%% this information may be modified by the editorial offices.
+%% The left head contains a list of authors,
+%% usually a maximum of three (otherwise use et al.). The right
+%% head is a modified title of up to roughly 44 characters.
+%% Running heads will not print in the manuscript style.
+
+\shorttitle{Collapsed Cores in Globular Clusters}
+\shortauthors{Djorgovski et al.}
+
+%% This is the end of the preamble. Indicate the beginning of the
+%% paper itself with \begin{document}.
+
+\begin{document}
+
+%% LaTeX will automatically break titles if they run longer than
+%% one line. However, you may use \\ to force a line break if
+%% you desire.
+
+\title{Collapsed Cores in Globular Clusters, \\
+ Gauge-Boson Couplings, and AAS\TeX\ Examples}
+
+%% Use \author, \affil, and the \and command to format
+%% author and affiliation information.
+%% Note that \email has replaced the old \authoremail command
+%% from AASTeX v4.0. You can use \email to mark an email address
+%% anywhere in the paper, not just in the front matter.
+%% As in the title, use \\ to force line breaks.
+
+\author{S. Djorgovski\altaffilmark{1,2,3} and Ivan R. King\altaffilmark{1}}
+\affil{Astronomy Department, University of California,
+ Berkeley, CA 94720}
+
+\author{C. D. Biemesderfer\altaffilmark{4,5}}
+\affil{National Optical Astronomy Observatories, Tucson, AZ 85719}
+\email{aastex-help@aas.org}
+
+\and
+
+\author{R. J. Hanisch\altaffilmark{5}}
+\affil{Space Telescope Science Institute, Baltimore, MD 21218}
+
+%% Notice that each of these authors has alternate affiliations, which
+%% are identified by the \altaffilmark after each name. Specify alternate
+%% affiliation information with \altaffiltext, with one command per each
+%% affiliation.
+
+\altaffiltext{1}{Visiting Astronomer, Cerro Tololo Inter-American Observatory.
+CTIO is operated by AURA, Inc.\ under contract to the National Science
+Foundation.}
+\altaffiltext{2}{Society of Fellows, Harvard University.}
+\altaffiltext{3}{present address: Center for Astrophysics,
+ 60 Garden Street, Cambridge, MA 02138}
+\altaffiltext{4}{Visiting Programmer, Space Telescope Science Institute}
+\altaffiltext{5}{Patron, Alonso's Bar and Grill}
+
+%% Mark off your abstract in the ``abstract'' environment. In the manuscript
+%% style, abstract will output a Received/Accepted line after the
+%% title and affiliation information. No date will appear since the author
+%% does not have this information. The dates will be filled in by the
+%% editorial office after submission.
+
+\begin{abstract}
+This is a preliminary report on surface photometry of the major
+fraction of known globular clusters, to see which of them show the signs
+of a collapsed core.
+We also explore some diversionary mathematics and recreational tables.
+\end{abstract}
+
+%% Keywords should appear after the \end{abstract} command. The uncommented
+%% example has been keyed in ApJ style. See the instructions to authors
+%% for the journal to which you are submitting your paper to determine
+%% what keyword punctuation is appropriate.
+
+%% Authors who wish to have the most important objects in their paper
+%% linked in the electronic edition to a data center may do so in the
+%% subject header. Objects should be in the appropriate "individual"
+%% headers (e.g. quasars: individual, stars: individual, etc.) with the
+%% additional provision that the total number of headers, including each
+%% individual object, not exceed six. The \objectname{} macro, and its
+%% alias \object{}, is used to mark each object. The macro takes the object
+%% name as its primary argument. This name will appear in the paper
+%% and serve as the link's anchor in the electronic edition if the name
+%% is recognized by the data centers. The macro also takes an optional
+%% argument in parentheses in cases where the data center identification
+%% differs from what is to be printed in the paper.
+
+\keywords{globular clusters: general ---
+globular clusters: individual(\objectname{NGC 6397},
+\object{NGC 6624}, \objectname[M 15]{NGC 7078},
+\object[Cl 1938-341]{Terzan 8})}
+
+%% From the front matter, we move on to the body of the paper.
+%% In the first two sections, notice the use of 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. We have
+%% chosen the first three characters of the first author's name plus
+%% the last two numeral of the year of publication as our KEY for
+%% each reference.
+
+\section{Introduction}
+
+A focal problem today in the dynamics of globular clusters is
+core collapse. It has been predicted by theory
+for decades \citep{hen61,lyn68,spi85}, but
+observation has been less alert to the phenomenon. For many years the
+central brightness peak in M15 \citep{kin75,new78}
+seemed a unique anomaly. Then \citet{aur82} suggested a central peak
+in NGC 6397, and a limited photographic survey of ours \citep[Paper I]{djo84}
+found three more cases, including NGC 6624, whose sharp center had often
+been remarked on \citep{can78}.
+
+\section{Observations}
+
+%% In a manner similar to \objectname authors can provide links to dataset
+%% hosted at participating data centers via the \dataset{} command. The
+%% second curly bracket argument is printed in the text while the first
+%% parentheses argument serves as the valid data set identifier. Large
+%% lists of data set are best provided in a table (see Table 3 for an example).
+%% Valid data set identifiers should be obtained from the data center that
+%% is currently hosting the data.
+
+All our observations were short direct exposures with CCD's. We also have
+a some random \dataset[ADS/Sa.ASCA\#X/86008020]{{\it Chandra} data} and a
+neat \dataset[ADS/Sa.HST#Y0Q70101T]{HST FOS spectrum} that readers can
+access via the links in the electronic edition. Unfortunately
+this has nothing whatsoever to do with this research.
+At Lick Observatory we used a TI 500$\times$500 chip
+and a GEC 575$\times$385, on the 1-m Nickel reflector. The only
+filter available at Lick was red. At CTIO we used a GEC 575$\times$385, with
+$B, V,$ and $R$ filters, and an RCA 512$\times$320, with $U, B, V, R,$ and $I$
+filters, on the 1.5-m reflector. In the CTIO observations we tried to
+concentrate on the shortest practicable wavelengths; but faintness, reddening,
+and poor short-wavelength sensitivity often kept us from observing in $U$ or
+even in $B$. All four cameras had scales of the order of 0.4 arcsec/pixel, and
+our field sizes were around 3 arcmin.
+
+The CCD images are unfortunately not always suitable, for very poor
+clusters or for clusters with large cores. Since the latter are easily
+studied by other means, we augmented our own CCD profiles by collecting
+from the literature a number of star-count
+profiles \citep{kin68,pet76,har84,ort85},
+as well as photoelectric profiles \citep{kin66,kin75} and
+electronographic profiles \citep{kro84}.
+In a few cases we judged normality by eye estimates on one of the Sky
+Surveys.
+
+%% In this section, we use the \subsection command to set off
+%% a subsection. \footnote is used to insert a footnote to the text.
+
+%% 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.
+
+%% This section also includes several of the displayed math environments
+%% mentioned in the Author Guide.
+
+\section{Helicity Amplitudes}
+
+It has been realized that helicity amplitudes provide a convenient means
+for Feynman diagram\footnote{Footnotes can be inserted like this.}
+evaluations. These amplitude-level techniques
+are particularly convenient for calculations involving many Feynman
+diagrams, where the usual trace techniques for the amplitude
+squared becomes unwieldy. Our calculations use the helicity techniques
+developed by other authors \cite[]{hag86}; we briefly summarize below.
+
+\subsection{Formalism} \label{bozomath}
+
+%% The equation environment wil produce a numbered display equation.
+
+A tree-level amplitude in $e^+e^-$ collisions can be expressed in
+terms of fermion strings of the form
+\begin{equation}
+\bar v(p_2,\sigma_2)P_{-\tau}\hat a_1\hat a_2\cdots
+\hat a_nu(p_1,\sigma_1) ,
+\end{equation}
+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 $P_\tau=\frac{1}{2}(1+\tau\gamma_5)$ is a chirality projection
+operator $(\tau = \pm1)$. The $a^\mu_i$ may be formed from particle
+four-momenta, gauge-boson polarization vectors or fermion strings with
+an uncontracted Lorentz index associated with final-state fermions.
+
+%% The \notetoeditor{TEXT} command allows the author to communicate
+%% information to the copy editor. This information will appear as a
+%% footnote on the printed copy for the manuscript style file. Nothing will
+%% appear on the printed copy if the preprint or
+%% preprint2 style files are used.
+
+%% The eqnarray environment produces multi-line display math. The end of
+%% each line is marked with a \\. Lines will be numbered unless the \\
+%% is preceded by a \nonumber command.
+%% Alignment points are marked by ampersands (&). There should be two
+%% ampersands (&) per line.
+
+In the chiral \notetoeditor{Figures 1 and 2 should appear side-by-side in
+print} representation the $\gamma$ matrices are expressed
+in terms of $2\times 2$ Pauli matrices $\sigma$ and the unit matrix 1 as
+\begin{eqnarray}
+\gamma^\mu & = &
+ \left(
+\begin{array}{cc}
+0 & \sigma^\mu_+ \\
+\sigma^\mu_- & 0
+\end{array} \right) ,
+ \gamma^5= \left(
+\begin{array}{cc}
+-1 & 0\\
+0 & 1
+\end{array} \right) , \nonumber \\
+\sigma^\mu_{\pm} & = & ({\bf 1} ,\pm \sigma) , \nonumber
+\end{eqnarray}
+giving
+\begin{equation}
+\hat a= \left(
+\begin{array}{cc}
+0 & (\hat a)_+\\
+(\hat a)_- & 0
+\end{array}\right), (\hat a)_\pm=a_\mu\sigma^\mu_\pm ,
+\end{equation}
+The spinors are expressed in terms of two-component Weyl spinors as
+\begin{equation}
+u=\left(
+\begin{array}{c}
+(u)_-\\
+(u)_+
+\end{array}\right), v={\bf (}\vdag_+{\bf ,} \vdag_-{\bf )} .
+\end{equation}
+
+%% Putting eqnarrays or equations inside the mathletters environment groups
+%% the enclosed equations by letter. For instance, the eqnarray below, instead
+%% 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.
+
+The Weyl spinors are given in terms of helicity eigenstates
+$\chi_\lambda(p)$ with $\lambda=\pm1$ by
+\begin{mathletters}
+\begin{eqnarray}
+u(p,\lambda)_\pm & = & (E\pm\lambda|{\bf p}|)^{1/2}\chi_\lambda(p) , \\
+v(p,\lambda)_\pm & = & \pm\lambda(E\mp\lambda|{\bf p}|)^{1/2}\chi
+_{-\lambda}(p)
+\end{eqnarray}
+\end{mathletters}
+
+%% This section contains more display math examples, including unnumbered
+%% equations (displaymath environment). The last paragraph includes some
+%% examples of in-line math featuring a couple of the AASTeX symbol macros.
+
+\section{Floating material and so forth}
+
+%% The displaymath environment will produce the same sort of equation as
+%% the equation environment, except that the equation will not be numbered
+%% by LaTeX.
+
+Consider a task that computes profile parameters for a modified
+Lorentzian of the form
+\begin{equation}
+I = \frac{1}{1 + d_{1}^{P (1 + d_{2} )}}
+\end{equation}
+where
+\begin{displaymath}
+d_{1} = \sqrt{ \left( \begin{array}{c} \frac{x_{1}}{R_{maj}}
+\end{array} \right) ^{2} +
+\left( \begin{array}{c} \frac{y_{1}}{R_{min}} \end{array} \right) ^{2} }
+\end{displaymath}
+\begin{displaymath}
+d_{2} = \sqrt{ \left( \begin{array}{c} \frac{x_{1}}{P R_{maj}}
+\end{array} \right) ^{2} +
+\left( \begin{array}{c} \case{y_{1}}{P R_{min}} \end{array} \right) ^{2} }
+\end{displaymath}
+\begin{displaymath}
+x_{1} = (x - x_{0}) \cos \Theta + (y - y_{0}) \sin \Theta
+\end{displaymath}
+\begin{displaymath}
+y_{1} = -(x - x_{0}) \sin \Theta + (y - y_{0}) \cos \Theta
+\end{displaymath}
+
+In these expressions $x_{0}$,$y_{0}$ is the star center, and $\Theta$ is the
+angle with the $x$ axis. Results of this task are shown in table~\ref{tbl-1}.
+It is not clear how these sorts of analyses may affect determination of
+ $M_{\sun}$, but the assumption is that the alternate results
+should be less than 90\degr\ out of phase with previous values.
+We have no observations of \ion{Ca}{2}.
+Roughly \slantfrac{4}{5} of the electronically submitted abstracts
+for AAS meetings are error-free.
+
+%% If you wish to include an acknowledgments section in your paper,
+%% separate it off from the body of the text using the \acknowledgments
+%% command.
+
+%% Included in this acknowledgments section are examples of the
+%% AASTeX hypertext markup commands. Use \url without the optional [HREF]
+%% argument when you want to print the url directly in the text. Otherwise,
+%% use either \url or \anchor, with the HREF as the first argument and the
+%% text to be printed in the second.
+
+\acknowledgments
+
+We are grateful to V. Barger, T. Han, and R. J. N. Phillips for
+doing the math in section~\ref{bozomath}.
+More information on the AASTeX macros package is available \\ at
+\url{http://www.aas.org/publications/aastex}.
+For technical support, please write to
+\email{aastex-help@aas.org}.
+
+%% To help institutions obtain information on the effectiveness of their
+%% telescopes, the AAS Journals has created a group of keywords for telescope
+%% facilities. A common set of keywords will make these types of searches
+%% significantly easier and more accurate. In addition, they will also be
+%% useful in linking papers together which utilize the same telescopes
+%% within the framework of the National Virtual Observatory.
+%% See the AASTeX Web site at http://www.journals.uchicago.edu/AAS/AASTeX
+%% for information on obtaining the facility keywords.
+
+%% After the acknowledgments section, use the following syntax and the
+%% \facility{} macro to list the keywords of facilities used in the research
+%% for the paper. Each keyword will be checked against the master list during
+%% copy editing. Individual instruments can be provided in parentheses,
+%% after the keyword, but they will not be verified.
+
+Facilities: \facility{Nickel}, \facility{HST(STIS)}, \facility{CXO(ASIS)}.
+
+%% Appendix material should be preceded with a single \appendix command.
+%% There should be a \section command for each appendix. Mark appendix
+%% subsections with the same markup you use in the main body of the paper.
+
+%% Each Appendix (indicated with \section) will be lettered A, B, C, etc.
+%% The equation counter will reset when it encounters the \appendix
+%% command and will number appendix equations (A1), (A2), etc.
+
+\appendix
+
+\section{Appendix material}
+
+Consider once again a task that computes profile parameters for a modified
+Lorentzian of the form
+\begin{equation}
+I = \frac{1}{1 + d_{1}^{P (1 + d_{2} )}}
+\end{equation}
+where
+\begin{mathletters}
+\begin{displaymath}
+d_{1} = \frac{3}{4} \sqrt{ \left( \begin{array}{c} \frac{x_{1}}{R_{maj}}
+\end{array} \right) ^{2} +
+\left( \begin{array}{c} \frac{y_{1}}{R_{min}} \end{array} \right) ^{2} }
+\end{displaymath}
+\begin{equation}
+d_{2} = \case{3}{4} \sqrt{ \left( \begin{array}{c} \frac{x_{1}}{P R_{maj}}
+\end{array} \right) ^{2} +
+\left( \begin{array}{c} \case{y_{1}}{P R_{min}} \end{array} \right) ^{2} }
+\end{equation}
+\begin{eqnarray}
+x_{1} & = & (x - x_{0}) \cos \Theta + (y - y_{0}) \sin \Theta \\
+y_{1} & = & -(x - x_{0}) \sin \Theta + (y - y_{0}) \cos \Theta
+\end{eqnarray}
+\end{mathletters}
+
+For completeness, here is one last equation.
+\begin{equation}
+e = mc^2
+\end{equation}
+
+%% The reference list follows the main body and any appendices.
+%% Use LaTeX's thebibliography environment to mark up your reference list.
+%% Note \begin{thebibliography} is followed by an empty set of
+%% curly braces. If you forget this, LaTeX will generate the error
+%% "Perhaps a missing \item?".
+%%
+%% thebibliography produces citations in the text using \bibitem-\cite
+%% cross-referencing. Each reference is preceded by a
+%% \bibitem command that defines in curly braces the KEY that corresponds
+%% to the KEY in the \cite commands (see the first section above).
+%% Make sure that you provide a unique KEY for every \bibitem or else the
+%% paper will not LaTeX. The square brackets should contain
+%% the citation text that LaTeX will insert in
+%% place of the \cite commands.
+
+%% We have used macros to produce journal name abbreviations.
+%% AASTeX provides a number of these for the more frequently-cited journals.
+%% See the Author Guide for a list of them.
+
+%% Note that the style of the \bibitem labels (in []) is slightly
+%% different from previous examples. The natbib system solves a host
+%% of citation expression problems, but it is necessary to clearly
+%% delimit the year from the author name used in the citation.
+%% See the natbib documentation for more details and options.
+
+\begin{thebibliography}{}
+\bibitem[Auri\`ere(1982)]{aur82} Auri\`ere, M. 1982, \aap,
+ 109, 301
+\bibitem[Canizares et al.(1978)]{can78} Canizares, C. R.,
+ Grindlay, J. E., Hiltner, W. A., Liller, W., \&
+ McClintock, J. E. 1978, \apj, 224, 39
+\bibitem[Djorgovski \& King(1984)]{djo84} Djorgovski, S.,
+ \& King, I. R. 1984, \apjl, 277, L49
+\bibitem[Hagiwara \& Zeppenfeld(1986)]{hag86} Hagiwara, K., \&
+ Zeppenfeld, D. 1986, Nucl.Phys., 274, 1
+\bibitem[Harris \& van den Bergh(1984)]{har84} Harris, W. E.,
+ \& van den Bergh, S. 1984, \aj, 89, 1816
+\bibitem[H\`enon(1961)]{hen61} H\'enon, M. 1961, Ann.d'Ap., 24, 369
+\bibitem[Heiles \& Troland(2003)]{heiles03} Heiles, C. \& Troland, T. H., 2003, \apjs, preprint doi:10.1086/381753
+\bibitem[Kim, Ostricker, \& Stone(2003)]{kim03} Kim, W.-T., Ostriker, E., \& Stone, J. M., 2003, \apj, 599, 1157
+\bibitem[King(1966)]{kin66} King, I. R. 1966, \aj, 71, 276
+\bibitem[King(1975)]{kin75} King, I. R. 1975, Dynamics of
+ Stellar Systems, A. Hayli, Dordrecht: Reidel, 1975, 99
+\bibitem[King et al.(1968)]{kin68} King, I. R., Hedemann, E.,
+ Hodge, S. M., \& White, R. E. 1968, \aj, 73, 456
+\bibitem[Kron et al.(1984)]{kro84} Kron, G. E., Hewitt, A. V.,
+ \& Wasserman, L. H. 1984, \pasp, 96, 198
+\bibitem[Lynden-Bell \& Wood(1968)]{lyn68} Lynden-Bell, D.,
+ \& Wood, R. 1968, \mnras, 138, 495
+\bibitem[Newell \& O'Neil(1978)]{new78} Newell, E. B.,
+ \& O'Neil, E. J. 1978, \apjs, 37, 27
+\bibitem[Ortolani et al.(1985)]{ort85} Ortolani, S., Rosino, L.,
+ \& Sandage, A. 1985, \aj, 90, 473
+\bibitem[Peterson(1976)]{pet76} Peterson, C. J. 1976, \aj, 81, 617
+\bibitem[Rudnick et al.(2003)]{rudnick03} Rudnick, G. et al., 2003, \apj, 599, 847
+\bibitem[Spitzer(1985)]{spi85} Spitzer, L. 1985, Dynamics of
+ Star Clusters, J. Goodman \& P. Hut, Dordrecht: Reidel, 109
+\bibitem[Treu et al.(2003)]{treu03} Treu, T. et al., 2003, \apj, 591, 53
+\end{thebibliography}
+
+\clearpage
+
+%% Use the figure environment and \plotone or \plottwo to include
+%% figures and captions in your electronic submission.
+%% To embed the sample graphics in
+%% the file, uncomment the \plotone, \plottwo, and
+%% \includegraphics commands
+%%
+%% If you need a layout that cannot be achieved with \plotone or
+%% \plottwo, you can invoke the graphicx package directly with the
+%% \includegraphics command or use \plotfiddle. For more information,
+%% please see the tutorial on "Using Electronic Art with AASTeX" in the
+%% documentation section at the AASTeX Web site,
+%% http://www.journals.uchicago.edu/AAS/AASTeX.
+%%
+%% The examples below also include sample markup for submission of
+%% supplemental electronic materials. As always, be sure to check
+%% the instructions to authors for the journal you are submitting to
+%% for specific submissions guidelines as they vary from
+%% journal to journal.
+
+
+%% This example uses \plotone to include an EPS file scaled to
+%% 80% of its natural size with \epsscale. Its caption
+%% has been written to indicate that additional figure parts will be
+%% available in the electronic journal.
+
+\begin{figure}
+\epsscale{.80}
+%%\plotone{f1.eps}
+\caption{Derived spectra for 3C138 \citep[see][]{heiles03}. Plots for all sources are available
+in the electronic edition of {\it The Astrophysical Journal}.\label{fig1}}
+\end{figure}
+
+\clearpage
+
+%% Here we use \plottwo to present two versions of the same figure,
+%% one in black and white for print the other in RGB color
+%% for online presentation. Note that the caption indicates
+%% that a color version of the figure will be available online.
+%%
+
+\begin{figure}
+%%\plottwo{f2.eps}{f2_color.eps}
+\caption{A panel taken from Figure 2 of \citet{rudnick03}. See the electronic edition of the Journal for a color version of this figure.\label{fig2}}
+\end{figure}
+
+%% This figure uses \includegraphics to scale and rotate the still frame
+%% for an mpeg animation.
+
+\begin{figure}
+%%\includegraphics[angle=90,scale=.50]{f3.eps}
+\caption{Animation still frame taken from \citet{kim03}.
+This figure is also available as an mpeg
+animation in the electronic edition of the
+{\it Astrophysical Journal}.}
+\end{figure}
+
+%% If you are not including electonic art with your submission, you may
+%% mark up your captions using the \figcaption command. See the
+%% User Guide for details.
+%%
+%% No more than seven \figcaption commands are allowed per page,
+%% so if you have more than seven captions, insert a \clearpage
+%% after every seventh one.
+
+%% Tables should be submitted one per page, so put a \clearpage before
+%% each one.
+
+%% Two options are available to the author for producing tables: the
+%% deluxetable environment provided by the AASTeX package or the LaTeX
+%% table environment. Use of deluxetable is preferred.
+%%
+
+%% Three table samples follow, two marked up in the deluxetable environment,
+%% one marked up as a LaTeX table.
+
+%% In this first example, note that the \tabletypesize{}
+%% command has been used to reduce the font size of the table.
+%% We also use the \rotate command to rotate the table to
+%% landscape orientation since it is very wide even at the
+%% reduced font size.
+%%
+%% Note also that the \label command needs to be placed
+%% inside the \tablecaption.
+
+%% This table also includes a table comment indicating that the full
+%% version will be available in machine-readable format in the electronic
+%% edition.
+%%
+\clearpage
+
+\begin{turnpage}
+\begin{deluxetable}{ccrrrrrrrrcrl}
+\tabletypesize{\scriptsize}
+\tablecaption{Sample table taken from \citet{treu03}\label{tbl-1}}
+\tablewidth{0pt}
+\tablehead{
+\colhead{POS} & \colhead{chip} & \colhead{ID} & \colhead{X} & \colhead{Y} &
+\colhead{RA} & \colhead{DEC} & \colhead{IAU$\pm$ $\delta$ IAU} &
+\colhead{IAP1$\pm$ $\delta$ IAP1} & \colhead{IAP2 $\pm$ $\delta$ IAP2} &
+\colhead{star} & \colhead{E} & \colhead{Comment}
+}
+\startdata
+0 & 2 & 1 & 1370.99 & 57.35 & 6.651120 & 17.131149 & 21.344$\pm$0.006 & 2
+4.385$\pm$0.016 & 23.528$\pm$0.013 & 0.0 & 9 & - \\
+0 & 2 & 2 & 1476.62 & 8.03 & 6.651480 & 17.129572 & 21.641$\pm$0.005 & 2
+3.141$\pm$0.007 & 22.007$\pm$0.004 & 0.0 & 9 & - \\
+0 & 2 & 3 & 1079.62 & 28.92 & 6.652430 & 17.135000 & 23.953$\pm$0.030 & 2
+4.890$\pm$0.023 & 24.240$\pm$0.023 & 0.0 & - & - \\
+0 & 2 & 4 & 114.58 & 21.22 & 6.655560 & 17.148020 & 23.801$\pm$0.025 & 2
+5.039$\pm$0.026 & 24.112$\pm$0.021 & 0.0 & - & - \\
+0 & 2 & 5 & 46.78 & 19.46 & 6.655800 & 17.148932 & 23.012$\pm$0.012 & 2
+3.924$\pm$0.012 & 23.282$\pm$0.011 & 0.0 & - & - \\
+0 & 2 & 6 & 1441.84 & 16.16 & 6.651480 & 17.130072 & 24.393$\pm$0.045 & 2
+6.099$\pm$0.062 & 25.119$\pm$0.049 & 0.0 & - & - \\
+0 & 2 & 7 & 205.43 & 3.96 & 6.655520 & 17.146742 & 24.424$\pm$0.032 & 2
+5.028$\pm$0.025 & 24.597$\pm$0.027 & 0.0 & - & - \\
+0 & 2 & 8 & 1321.63 & 9.76 & 6.651950 & 17.131672 & 22.189$\pm$0.011 & 2
+4.743$\pm$0.021 & 23.298$\pm$0.011 & 0.0 & 4 & edge \\
+\enddata
+
+%% Text for table notes should follow after the \enddata but before
+%% the \end{deluxetable}. Make sure there is at least one \tablenotemark
+%% in the table for each \tablenotetext.
+
+\tablecomments{Table \ref{tbl-1} is published in its entirety in the electronic edition of the {\it Astrophysical Journal}. A portion is shown here for guidance
+regarding its form and content.}
+
+\tablenotetext{a}{Sample footnote for table~\ref{tbl-1} that was generated
+with the deluxetable environment}
+\tablenotetext{b}{Another sample footnote for table~\ref{tbl-1}}
+
+\end{deluxetable}
+\end{turnpage}
+
+%% If you use the table environment, please indicate horizontal rules using
+%% \tableline, not \hline.
+%% Do not put multiple tabular environments within a single table.
+%% The optional \label should appear inside the \caption command.
+
+\clearpage
+
+\begin{table}
+\begin{center}
+\caption{More terribly relevant tabular information.\label{tbl-2}}
+\begin{tabular}{crrrrrrrrrrr}
+\tableline
+\tableline
+Star & Height & $d_{x}$ & $d_{y}$ & $n$ & $\chi^2$ & $R_{maj}$ & $R_{min}$ &
+\multicolumn{1}{c}{$P$\tablenotemark{a}} & $P R_{maj}$ & $P R_{min}$ &
+\multicolumn{1}{c}{$\Theta$\tablenotemark{b}} \\
+\tableline
+1 &33472.5 &-0.1 &0.4 &53 &27.4 &2.065 &1.940 &3.900 &68.3 &116.2 &-27.639\\
+2 &27802.4 &-0.3 &-0.2 &60 &3.7 &1.628 &1.510 &2.156 &6.8 &7.5 &-26.764\\
+3 &29210.6 &0.9 &0.3 &60 &3.4 &1.622 &1.551 &2.159 &6.7 &7.3 &-40.272\\
+4 &32733.8 &-1.2\tablenotemark{c} &-0.5 &41 &54.8 &2.282 &2.156 &4.313 &117.4 &78.2 &-35.847\\
+5 & 9607.4 &-0.4 &-0.4 &60 &1.4 &1.669\tablenotemark{c} &1.574 &2.343 &8.0 &8.9 &-33.417\\
+6 &31638.6 &1.6 &0.1 &39 &315.2 & 3.433 &3.075 &7.488 &92.1 &25.3 &-12.052\\
+\tableline
+\end{tabular}
+
+%% Any table notes must follow the \end{tabular} command.
+
+\tablenotetext{a}{Sample footnote for table~\ref{tbl-2} that was
+generated with the \LaTeX\ table environment}
+\tablenotetext{b}{Yet another sample footnote for table~\ref{tbl-2}}
+\tablenotetext{c}{Another sample footnote for table~\ref{tbl-2}}
+\tablecomments{We can also attach a long-ish paragraph of explanatory
+material to a table.}
+\end{center}
+\end{table}
+
+%% If the table is more than one page long, the width of the table can vary
+%% from page to page when the default \tablewidth is used, as below. The
+%% individual table widths for each page will be written to the log file; a
+%% maximum tablewidth for the table can be computed from these values.
+%% The \tablewidth argument can then be reset and the file reprocessed, so
+%% that the table is of uniform width throughout. Try getting the widths
+%% from the log file and changing the \tablewidth parameter to see how
+%% adjusting this value affects table formatting.
+
+%% The \dataset macro has also been applied to a few of the objects to
+%% show how many observations can be tagged in a table.
+
+\clearpage
+
+\LongTables % the next table is multi-page
+
+\begin{deluxetable}{lrrrrcrrrrr}
+\tablewidth{0pt}
+\tablecaption{Literature Data for Program Stars}
+\tablehead{
+\colhead{Star} & \colhead{V} &
+\colhead{b$-$y} & \colhead{m$_1$} &
+\colhead{c$_1$} & \colhead{ref} &
+\colhead{T$_{\rm eff}$} & \colhead{log g} &
+\colhead{v$_{\rm turb}$} & \colhead{[Fe/H]} &
+\colhead{ref}}
+\startdata
+HD 97 & 9.7& 0.51& 0.15& 0.35& 2 & \nodata & \nodata & \nodata & $-1.50$ & 2 \\
+& & & & & & 5015 & \nodata & \nodata & $-1.50$ & 10 \\
+\dataset[ADS/Sa.HST#O6H04VAXQ]{HD 2665} & 7.7& 0.54& 0.09& 0.34& 2 & \nodata & \nodata & \nodata & $-2.30$ & 2 \\
+& & & & & & 5000 & 2.50 & 2.4 & $-1.99$ & 5 \\
+& & & & & & 5120 & 3.00 & 2.0 & $-1.69$ & 7 \\
+& & & & & & 4980 & \nodata & \nodata & $-2.05$ & 10 \\
+HD 4306 & 9.0& 0.52& 0.05& 0.35& 20, 2& \nodata & \nodata & \nodata & $-2.70$ & 2 \\
+& & & & & & 5000 & 1.75 & 2.0 & $-2.70$ & 13 \\
+& & & & & & 5000 & 1.50 & 1.8 & $-2.65$ & 14 \\
+& & & & & & 4950 & 2.10 & 2.0 & $-2.92$ & 8 \\
+& & & & & & 5000 & 2.25 & 2.0 & $-2.83$ & 18 \\
+& & & & & & \nodata & \nodata & \nodata & $-2.80$ & 21 \\
+& & & & & & 4930 & \nodata & \nodata & $-2.45$ & 10 \\
+HD 5426 & 9.6& 0.50& 0.08& 0.34& 2 & \nodata & \nodata & \nodata & $-2.30$ & 2 \\
+\dataset[ADS/Sa.HST#O5F654010]{HD 6755} & 7.7& 0.49& 0.12& 0.28& 20, 2& \nodata & \nodata & \nodata & $-1.70$ & 2 \\
+& & & & & & 5200 & 2.50 & 2.4 & $-1.56$ & 5 \\
+& & & & & & 5260 & 3.00 & 2.7 & $-1.67$ & 7 \\
+& & & & & & \nodata & \nodata & \nodata & $-1.58$ & 21 \\
+& & & & & & 5200 & \nodata & \nodata & $-1.80$ & 10 \\
+& & & & & & 4600 & \nodata & \nodata & $-2.75$ & 10 \\
+\dataset[ADS/Sa.HST#O56D06010]{HD 94028} & 8.2& 0.34& 0.08& 0.25& 20 & 5795 & 4.00 & \nodata & $-1.70$ & 22 \\
+& & & & & & 5860 & \nodata & \nodata & $-1.70$ & 4 \\
+& & & & & & 5910 & 3.80 & \nodata & $-1.76$ & 15 \\
+& & & & & & 5800 & \nodata & \nodata & $-1.67$ & 17 \\
+& & & & & & 5902 & \nodata & \nodata & $-1.50$ & 11 \\
+& & & & & & 5900 & \nodata & \nodata & $-1.57$ & 3 \\
+& & & & & & \nodata & \nodata & \nodata & $-1.32$ & 21 \\
+HD 97916 & 9.2& 0.29& 0.10& 0.41& 20 & 6125 & 4.00 & \nodata & $-1.10$ & 22 \\
+& & & & & & 6160 & \nodata & \nodata & $-1.39$ & 3 \\
+& & & & & & 6240 & 3.70 & \nodata & $-1.28$ & 15 \\
+& & & & & & 5950 & \nodata & \nodata & $-1.50$ & 17 \\
+& & & & & & 6204 & \nodata & \nodata & $-1.36$ & 11 \\
+\cutinhead{This is a cut-in head}
++26\arcdeg2606& 9.7&0.34&0.05&0.28&20,11& 5980 & \nodata & \nodata &$<-2.20$ & 19 \\
+& & & & & & 5950 & \nodata & \nodata & $-2.89$ & 24 \\
++26\arcdeg3578& 9.4&0.31&0.05&0.37&20,11& 5830 & \nodata & \nodata & $-2.60$ & 4 \\
+& & & & & & 5800 & \nodata & \nodata & $-2.62$ & 17 \\
+& & & & & & 6177 & \nodata & \nodata & $-2.51$ & 11 \\
+& & & & & & 6000 & 3.25 & \nodata & $-2.20$ & 22 \\
+& & & & & & 6140 & 3.50 & \nodata & $-2.57$ & 15 \\
++30\arcdeg2611& 9.2&0.82&0.33&0.55& 2 & \nodata & \nodata & \nodata & $-1.70$ & 2 \\
+& & & & & & 4400 & 1.80 & \nodata & $-1.70$ & 12 \\
+& & & & & & 4400 & 0.90 & 1.7 & $-1.20$ & 14 \\
+& & & & & & 4260 & \nodata & \nodata & $-1.55$ & 10 \\
++37\arcdeg1458& 8.9&0.44&0.07&0.22&20,11& 5296 & \nodata & \nodata & $-2.39$ & 11 \\
+& & & & & & 5420 & \nodata & \nodata & $-2.43$ & 3 \\
++58\arcdeg1218&10.0&0.51&0.03&0.36& 2 & \nodata & \nodata & \nodata & $-2.80$ & 2 \\
+& & & & & & 5000 & 1.10 & 2.2 & $-2.71$ & 14 \\
+& & & & & & 5000 & 2.20 & 1.8 & $-2.46$ & 5 \\
+& & & & & & 4980 & \nodata & \nodata & $-2.55$ & 10 \\
++72\arcdeg0094&10.2&0.31&0.09&0.26&12 & 6160 & \nodata & \nodata & $-1.80$ & 19 \\
+\sidehead{I am a side head:}
+G5--36 & 10.8& 0.40& 0.07& 0.28& 20 & \nodata & \nodata & \nodata & $-1.19$ & 21 \\
+G18--54 & 10.7& 0.37& 0.08& 0.28& 20 & \nodata & \nodata & \nodata & $-1.34$ & 21 \\
+G20--08 & 9.9& 0.36& 0.05& 0.25& 20,11& 5849 & \nodata & \nodata & $-2.59$ & 11 \\
+& & & & & & \nodata & \nodata & \nodata & $-2.03$ & 21 \\
+G20--15 & 10.6& 0.45& 0.03& 0.27& 20,11& 5657 & \nodata & \nodata & $-2.00$ & 11 \\
+& & & & & & 6020 & \nodata & \nodata & $-1.56$ & 3 \\
+& & & & & & \nodata & \nodata & \nodata & $-1.58$ & 21 \\
+G21--22 & 10.7& 0.38& 0.07& 0.27& 20,11& \nodata & \nodata & \nodata & $-1.23$ & 21 \\
+G24--03 & 10.5& 0.36& 0.06& 0.27& 20,11& 5866 & \nodata & \nodata & $-1.78$ & 11 \\
+& & & & & & \nodata & \nodata & \nodata & $-1.70$ & 21 \\
+G30--52 & 8.6& 0.50& 0.25& 0.27& 11 & 4757 & \nodata & \nodata & $-2.12$ & 11 \\
+& & & & & & 4880 & \nodata & \nodata & $-2.14$ & 3 \\
+G33--09 & 10.6& 0.41& 0.10& 0.28& 20 & 5575 & \nodata & \nodata & $-1.48$ & 11 \\
+G66--22 & 10.5& 0.46& 0.16& 0.28& 11 & 5060 & \nodata & \nodata & $-1.77$ & 3 \\
+& & & & & & \nodata & \nodata & \nodata & $-1.04$ & 21 \\
+G90--03 & 10.4& 0.37& 0.04& 0.29& 20 & \nodata & \nodata & \nodata & $-2.01$ & 21 \\
+LP 608--62\tablenotemark{a} & 10.5& 0.30& 0.07& 0.35& 11 & 6250 & \nodata &
+\nodata & $-2.70$ & 4 \\
+\enddata
+\tablenotetext{a}{Star LP 608--62 is also known as BD+1\arcdeg 2341p. We will
+make this footnote extra long so that it extends over two lines.}
+
+%% You can append references to a table using the \tablerefs command.
+
+\tablerefs{
+(1) Barbuy, Spite, \& Spite 1985; (2) Bond 1980; (3) Carbon et al. 1987;
+(4) Hobbs \& Duncan 1987; (5) Gilroy et al. 1988: (6) Gratton \& Ortolani 1986;
+(7) Gratton \& Sneden 1987; (8) Gratton \& Sneden (1988); (9) Gratton \& Sneden 1991;
+(10) Kraft et al. 1982; (11) LCL, or Laird, 1990; (12) Leep \& Wallerstein 1981;
+(13) Luck \& Bond 1981; (14) Luck \& Bond 1985; (15) Magain 1987;
+(16) Magain 1989; (17) Peterson 1981; (18) Peterson, Kurucz, \& Carney 1990;
+(19) RMB; (20) Schuster \& Nissen 1988; (21) Schuster \& Nissen 1989b;
+(22) Spite et al. 1984; (23) Spite \& Spite 1986; (24) Hobbs \& Thorburn 1991;
+(25) Hobbs et al. 1991; (26) Olsen 1983.}
+\end{deluxetable}
+
+%% Tables may also be prepared as separate files. See the accompanying
+%% sample file table.tex for an example of an external table file.
+%% To include an external file in your main document, use the \input
+%% command. Uncomment the line below to include table.tex in this
+%% sample file. (Note that you will need to comment out the \documentclass,
+%% \begin{document}, and \end{document} commands from table.tex if you want
+%% to include it in this document.)
+
+%% \input{table}
+
+%% The following command ends your manuscript. LaTeX will ignore any text
+%% that appears after it.
+
+\end{document}
+
+%%
+%% End of file `sample.tex'.