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author | Karl Berry <karl@freefriends.org> | 2006-01-09 00:49:07 +0000 |
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committer | Karl Berry <karl@freefriends.org> | 2006-01-09 00:49:07 +0000 |
commit | 007f67a693e4d031fd3d792df8e4d5f43e2cb2e7 (patch) | |
tree | 90d17e00e572ecb1e24764b6f29c80e098b08d29 /Master/texmf-dist/doc/latex/aastex/sample.tex | |
parent | 950209b26f70aa87ed07c54f82a95b6f03b7c3a0 (diff) |
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diff --git a/Master/texmf-dist/doc/latex/aastex/sample.tex b/Master/texmf-dist/doc/latex/aastex/sample.tex new file mode 100644 index 00000000000..3861a21a08c --- /dev/null +++ b/Master/texmf-dist/doc/latex/aastex/sample.tex @@ -0,0 +1,766 @@ +%% +%% Beginning of file 'sample.tex' +%% +%% Modified 2005 June 21 +%% +%% This is a sample manuscript marked up using the +%% AASTeX v5.x LaTeX 2e macros. + +%% The first piece of markup in an AASTeX v5.x document +%% is the \documentclass command. LaTeX will ignore +%% any data that comes before this command. + +%% The command below calls the preprint style +%% which will produce a one-column, single-spaced document. +%% Examples of commands for other substyles follow. Use +%% whichever is most appropriate for your purposes. +%% +%%\documentclass[12pt,preprint]{aastex} + +%% manuscript produces a one-column, double-spaced document: + +\documentclass[manuscript]{aastex} + +%% preprint2 produces a double-column, single-spaced document: + +%% \documentclass[preprint2]{aastex} + +%% Sometimes a paper's abstract is too long to fit on the +%% title page in preprint2 mode. When that is the case, +%% use the longabstract style option. + +%% \documentclass[preprint2,longabstract]{aastex} + +%% If you want to create your own macros, you can do so +%% using \newcommand. Your macros should appear before +%% the \begin{document} command. +%% +%% If you are submitting to a journal that translates manuscripts +%% into SGML, you need to follow certain guidelines when preparing +%% your macros. See the AASTeX v5.x Author Guide +%% for information. + +\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. + +\keywords{globular clusters: general --- globular clusters: individual(NGC 6397, +NGC 6624, NGC 7078, 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. + + +%% Authors who wish to have the most important objects in their paper +%% linked in the electronic edition to a data center may do so by tagging +%% their objects with \objectname{} or \object{}. Each macro takes the +%% object name as its required argument. The optional, square-bracket +%% argument should be used in cases where the data center identification +%% differs from what is to be printed in the paper. The text appearing +%% in curly braces is what will appear in print in the published paper. +%% If the object name is recognized by the data centers, it will be linked +%% in the electronic edition to the object data available at the data centers + +\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 \object{NGC 6397}, and a +limited photographic survey of ours \citep[Paper I]{djo84} found three more +cases, \objectname{NGC 6624}, \objectname[M 15]{NGC 7078}, and +\object[Cl 1938-341]{Terzan 8}), 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 random {\it Chandra} data set \dataset{ADS/Sa.ASCA\#X/86008020} 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 or configurations can be provided +%% in parentheses, after the keyword, but they will not be verified. + +{\it 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{deluxetable}{ccrrrrrrrrcrl} +\tabletypesize{\scriptsize} +\rotate +\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} + +%% 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 + +\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'm 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'. |