X-Git-Url: https://git.lyx.org/gitweb/?a=blobdiff_plain;f=lib%2Fexamples%2Faas_sample.lyx;h=c77b86e9ad2fb1fc5c857b8f0a48205a0262a982;hb=e9d9f2e27bf7d8174022a8c9fffc94c981ab7c0f;hp=95d29d1b67ab81fa8b48a85511206ba8b294debf;hpb=27de1486ca34aaad446adb798d71a77d6f6304da;p=lyx.git diff --git a/lib/examples/aas_sample.lyx b/lib/examples/aas_sample.lyx index 95d29d1b67..c77b86e9ad 100644 --- a/lib/examples/aas_sample.lyx +++ b/lib/examples/aas_sample.lyx @@ -1,6 +1,7 @@ -#This file was created by Sun Jul 25 23:59:27 1999 -#LyX 1.0 (C) 1995-1999 Matthias Ettrich and the LyX Team -\lyxformat 2.15 +#LyX 1.5.0svn created this file. For more info see http://www.lyx.org/ +\lyxformat 245 +\begin_document +\begin_header \textclass aastex \begin_preamble \newcommand{\vdag}{(v)^\dagger} @@ -9,265 +10,406 @@ \shorttitle{Djorgovski et al.} \shortauthors{Collapsed Cores in Globular Clusters} \end_preamble -\language default +\language english \inputencoding default \fontscheme default \graphics default \paperfontsize default -\spacing single -\papersize Default -\paperpackage a4 -\use_geometry 0 +\spacing single +\papersize default +\use_geometry false \use_amsmath 0 +\cite_engine basic +\use_bibtopic false \paperorientation portrait \secnumdepth 3 \tocdepth 3 \paragraph_separation indent \defskip medskip \quotes_language english -\quotes_times 2 \papercolumns 1 \papersides 1 \paperpagestyle default +\tracking_changes false +\output_changes true +\end_header -\layout Title +\begin_body -Collapsed Cores in Globular Clusters, Gauge-Boson Couplings, and AASTeX -\latex latex - -\latex default +\begin_layout Title + +Collapsed Cores in Globular Clusters, Gauge-Boson Couplings, and AASTeX Examples -\layout Author +\end_layout + +\begin_layout Author S. Djorgovski -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash altaffilmark{1,2,3} -\latex default +\end_layout + +\end_inset + and Ivan R. King -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash altaffilmark{1} -\layout Affiliation +\end_layout + +\end_inset + + +\end_layout + +\begin_layout Affiliation Astronomy Department, University of California, Berkeley, CA 94720 -\layout Author +\end_layout + +\begin_layout Author C. D. Biemesderfer -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash altaffilmark{4,5} -\layout Affiliation +\end_layout + +\end_inset + + +\end_layout + +\begin_layout Affiliation National Optical Astronomy Observatories, Tucson, AZ 85719 -\layout Email +\end_layout + +\begin_layout Email aastex-help@aas.org -\layout And +\end_layout + +\begin_layout And + +\end_layout -\layout Author +\begin_layout Author R. J. Hanisch -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash altaffilmark{5} -\layout Affiliation +\end_layout + +\end_inset + + +\end_layout + +\begin_layout Affiliation Space Telescope Science Institute, Baltimore, MD 21218 -\layout Standard +\end_layout + +\begin_layout Standard -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash altaffiltext{1}{Visiting Astronomer, Cerro Tololo Inter-American Observatory. CTIO is operated by AURA, Inc. -\backslash +\backslash under contract to the National Science Foundation.} -\layout Standard +\end_layout + +\begin_layout Standard +\end_layout -\latex latex +\begin_layout Standard -\backslash +\backslash altaffiltext{2}{Society of Fellows, Harvard University.} -\layout Standard +\end_layout +\begin_layout Standard -\latex latex +\end_layout -\backslash +\begin_layout Standard + +\backslash altaffiltext{3}{present address: Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138} -\layout Standard +\end_layout + +\begin_layout Standard +\end_layout -\latex latex +\begin_layout Standard -\backslash +\backslash altaffiltext{4}{Visiting Programmer, Space Telescope Science Institute} -\layout Standard +\end_layout +\begin_layout Standard -\latex latex +\end_layout -\backslash +\begin_layout Standard + +\backslash altaffiltext{5}{Patron, Alonso's Bar and Grill} -\layout Abstract +\end_layout + +\end_inset + + +\end_layout + +\begin_layout 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. -\layout Keywords +\end_layout + +\begin_layout Keywords clusters: globular, peanut---bosons: bozos -\layout Section +\end_layout + +\begin_layout Section Introduction -\layout Standard +\end_layout + +\begin_layout Standard A focal problem today in the dynamics of globular clusters is core collapse. It has been predicted by theory for decades -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash citep{hen61,lyn68,spi85} -\latex default +\end_layout + +\end_inset + , but observation has been less alert to the phenomenon. For many years the central brightness peak in M15 -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash citep{kin75,new78} -\latex default +\end_layout + +\end_inset + seemed a unique anomaly. Then -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash citet{aur82} -\latex default +\end_layout + +\end_inset + suggested a central peak in NGC 6397, and a limited photographic survey of ours -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash citep[Paper I]{djo84} -\latex default +\end_layout + +\end_inset + found three more cases, including NGC 6624, whose sharp center had often been remarked on -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash citep{can78} -\latex default +\end_layout + +\end_inset + . -\layout Section +\end_layout + +\begin_layout Section Observations -\layout Standard +\end_layout + +\begin_layout Standard All our observations were short direct exposures with CCD's. At Lick Observatory we used a TI 500 \begin_inset Formula \( \times \) -\end_inset +\end_inset 500 chip and a GEC 575 \begin_inset Formula \( \times \) -\end_inset +\end_inset 385, on the 1-m Nickel reflector. The only filter available at Lick was red. At CTIO we used a GEC 575 \begin_inset Formula \( \times \) -\end_inset +\end_inset 385, with \begin_inset Formula \( B,V, \) -\end_inset +\end_inset and \begin_inset Formula \( R \) -\end_inset +\end_inset filters, and an RCA 512 \begin_inset Formula \( \times \) -\end_inset +\end_inset 320, with \begin_inset Formula \( U,B,V,R, \) -\end_inset +\end_inset and \begin_inset Formula \( I \) -\end_inset +\end_inset 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 \begin_inset Formula \( U \) -\end_inset +\end_inset or even in \begin_inset Formula \( B \) -\end_inset +\end_inset . All four cameras had scales of the order of 0.4 arcsec/pixel, and our field sizes were around 3 arcmin. -\layout Standard +\end_layout + +\begin_layout Standard 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 -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash citep{kin68,pet76,har84,ort85} -\latex default +\end_layout + +\end_inset + , as well as photoelectric profiles -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash citep{kin66,kin75} -\latex default +\end_layout + +\end_inset + and electronographic profiles -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash citep{kro84} -\latex default +\end_layout + +\end_inset + . In a few cases we judged normality by eye estimates on one of the Sky Surveys. -\layout Section +\end_layout + +\begin_layout Section Helicity Amplitudes -\layout Standard +\end_layout + +\begin_layout Standard It has been realized that helicity amplitudes provide a convenient means for Feynman diagram -\begin_float footnote -\layout Standard +\begin_inset Foot +status collapsed + +\begin_layout Standard Footnotes can be inserted like this. -\end_float +\end_layout + +\end_inset + evaluations. These amplitude-level techniques are particularly convenient for calculations involving many Feynman diagrams, where the usual trace techniques for the @@ -276,90 +418,98 @@ Footnotes can be inserted like this. \begin_inset LatexCommand \cite{hag86} -\end_inset +\end_inset ; we briefly summarize below. -\layout Subsection +\end_layout + +\begin_layout Subsection Formalism -\layout Standard +\end_layout + +\begin_layout Standard \begin_inset LatexCommand \label{bozomath} -\end_inset +\end_inset + +\end_layout -\layout Standard +\begin_layout Standard A tree-level amplitude in \begin_inset Formula \( e^{+}e^{-} \) -\end_inset +\end_inset collisions can be expressed in terms of fermion strings of the form -\begin_inset Formula -\begin{equation} +\begin_inset Formula \begin{equation} \bar{v}(p_{2},\sigma _{2})P_{-\tau }\hat{a}_{1}\hat{a}_{2}\cdots \hat{a}_{n}u(p_{1},\sigma _{1}), \end{equation} -\end_inset +\end_inset where \begin_inset Formula \( p \) -\end_inset +\end_inset and \begin_inset Formula \( \sigma \) -\end_inset +\end_inset label the initial \begin_inset Formula \( e^{\pm } \) -\end_inset +\end_inset four-momenta and helicities \begin_inset Formula \( (\sigma =\pm 1) \) -\end_inset +\end_inset , \begin_inset Formula \( \hat{a}_{i}=a^{\mu }_{i}\gamma _{\nu } \) -\end_inset +\end_inset and \begin_inset Formula \( P_{\tau }=\frac{1}{2}(1+\tau \gamma _{5}) \) -\end_inset +\end_inset is a chirality projection operator \begin_inset Formula \( (\tau =\pm1 ) \) -\end_inset +\end_inset . The \begin_inset Formula \( a^{\mu }_{i} \) -\end_inset +\end_inset may be formed from particle four-momenta, gauge-boson polarization vectors or fermion strings with an uncontracted Lorentz index associated with final-sta te fermions. -\layout NoteToEditor +\end_layout + +\begin_layout NoteToEditor Figures 1 and 2 should appear side-by-side in print -\layout Standard +\end_layout + +\begin_layout Standard In the chiral representation the \begin_inset Formula \( \gamma \) -\end_inset +\end_inset matrices are expressed in terms of \begin_inset Formula \( 2\times 2 \) -\end_inset +\end_inset Pauli matrices \begin_inset Formula \( \sigma \) -\end_inset +\end_inset and the unit matrix 1 as -\begin_inset Formula -\begin{eqnarray} +\begin_inset Formula \begin{eqnarray} \gamma ^{\mu } & = & \left( \begin{array}{cc} 0 & \sigma ^{\mu }_{+}\\ \sigma ^{\mu }_{-} & 0 @@ -367,229 +517,260 @@ In the chiral representation the -1 & 0\\ 0 & 1 \end{array}\right) ,\nonumber \\ -\sigma ^{\mu }_{\pm } & = & ({\textbf {1}},\pm \sigma ),\nonumber +\sigma ^{\mu }_{\pm } & = & ({\textbf {1}},\pm \sigma ),\nonumber \end{eqnarray} -\end_inset +\end_inset giving -\begin_inset Formula -\begin{equation} +\begin_inset Formula \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} -\end_inset +\end_inset The spinors are expressed in terms of two-component Weyl spinors as -\begin_inset Formula -\begin{equation} +\begin_inset Formula \begin{equation} u=\left( \begin{array}{c} (u)_{-}\\ (u)_{+} \end{array}\right) ,v={\textbf {(}}\vdag _{+}{\textbf {,}}\vdag _{-}{\textbf {)}}. \end{equation} -\end_inset +\end_inset -\layout Standard +\end_layout + +\begin_layout Standard The Weyl spinors are given in terms of helicity eigenstates \begin_inset Formula \( \chi _{\lambda }(p) \) -\end_inset +\end_inset with \begin_inset Formula \( \lambda =\pm1 \) -\end_inset +\end_inset by -\layout MathLetters +\end_layout + +\begin_layout MathLetters -\begin_inset Formula -\begin{eqnarray} +\begin_inset Formula \begin{eqnarray} u(p,\lambda )_{\pm } & = & (E\pm \lambda |{\textbf {p}}|)^{1/2}\chi _{\lambda }(p),\\ v(p,\lambda )_{\pm } & = & \pm \lambda (E\mp \lambda |{\textbf {p}}|)^{1/2}\chi _{-\lambda }(p) \end{eqnarray} -\end_inset +\end_inset -\layout Section +\end_layout + +\begin_layout Section Floating material and so forth -\layout Standard +\end_layout + +\begin_layout Standard Consider a task that computes profile parameters for a modified Lorentzian of the form -\begin_inset Formula -\begin{equation} +\begin_inset Formula \begin{equation} I=\frac{1}{1+d_{1}^{P(1+d_{2})}} \end{equation} -\end_inset +\end_inset where -\begin_inset Formula -\[ +\begin_inset Formula \[ d_{1}=\sqrt{\left( \begin{array}{c} \frac{x_{1}}{R_{maj}} \end{array}\right) ^{2}+\left( \begin{array}{c} \frac{y_{1}}{R_{min}} \end{array}\right) ^{2}}\] -\end_inset +\end_inset -\begin_inset Formula -\[ +\begin_inset Formula \[ d_{2}=\sqrt{\left( \begin{array}{c} \frac{x_{1}}{PR_{maj}} \end{array}\right) ^{2}+\left( \begin{array}{c} \case {y_{1}}{PR_{min}} \end{array}\right) ^{2}}\] -\end_inset +\end_inset -\begin_inset Formula -\[ +\begin_inset Formula \[ x_{1}=(x-x_{0})\cos \Theta +(y-y_{0})\sin \Theta \] -\end_inset +\end_inset -\begin_inset Formula -\[ +\begin_inset Formula \[ y_{1}=-(x-x_{0})\sin \Theta +(y-y_{0})\cos \Theta \] -\end_inset +\end_inset -\layout Standard +\end_layout + +\begin_layout Standard In these expressions \begin_inset Formula \( x_{0} \) -\end_inset +\end_inset , \begin_inset Formula \( y_{0} \) -\end_inset +\end_inset is the star center, and \begin_inset Formula \( \Theta \) -\end_inset +\end_inset is the angle with the \begin_inset Formula \( x \) -\end_inset +\end_inset axis. - Results of this task are shown in table -\protected_separator + Results of this task are shown in table\InsetSpace ~ \begin_inset LatexCommand \ref{tbl-2} -\end_inset +\end_inset . It is not clear how these sorts of analyses may affect determination of \begin_inset Formula \( M_{\sun } \) -\end_inset +\end_inset , but the assumption is that the alternate results should be less than 90 -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash degr -\backslash +\backslash -\latex default +\end_layout + +\end_inset + out of phase with previous values. We have no observations of -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash ion{Ca}{2} -\latex default +\end_layout + +\end_inset + . Roughly -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash slantfrac{4}{5} -\latex default +\end_layout + +\end_inset + of the electronically submitted abstracts for AAS meetings are error-free. -\layout Acknowledgements +\end_layout + +\begin_layout Acknowledgements + +\end_layout -\layout Standard +\begin_layout Standard We are grateful to V. Barger, T. Han, and R. J. N. - Phillips for doing the math in section -\protected_separator + Phillips for doing the math in section\InsetSpace ~ \begin_inset LatexCommand \ref{bozomath} -\end_inset +\end_inset . More information on the AASTeX macros package are available at -\latex latex \begin_inset LatexCommand \url{http://www.aas.org/publications/aastex} -\end_inset +\end_inset -\latex default or the -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash anchor{ftp://www.aas.org/pubs/}{AAS ftp site} -\latex default +\end_layout + +\end_inset + . -\layout Appendix +\end_layout + +\begin_layout Appendix -\layout Section +\end_layout + +\begin_layout Section Appendicial material -\layout Standard +\end_layout + +\begin_layout Standard Consider once again a task that computes profile parameters for a modified Lorentzian of the form -\begin_inset Formula -\begin{equation} +\begin_inset Formula \begin{equation} I=\frac{1}{1+d_{1}^{P(1+d_{2})}} \end{equation} -\end_inset +\end_inset where -\layout MathLetters +\end_layout +\begin_layout MathLetters -\begin_inset Formula -\[ + +\begin_inset Formula \[ d_{1}=\frac{3}{4}\sqrt{\left( \begin{array}{c} \frac{x_{1}}{R_{maj}} \end{array}\right) ^{2}+\left( \begin{array}{c} \frac{y_{1}}{R_{min}} \end{array}\right) ^{2}}\] -\end_inset +\end_inset -\begin_inset Formula -\begin{equation} +\begin_inset Formula \begin{equation} d_{2}=\case {3}{4}\sqrt{\left( \begin{array}{c} \frac{x_{1}}{PR_{maj}} \end{array}\right) ^{2}+\left( \begin{array}{c} @@ -597,43 +778,53 @@ d_{2}=\case {3}{4}\sqrt{\left( \begin{array}{c} \end{array}\right) ^{2}} \end{equation} -\end_inset +\end_inset -\begin_inset Formula -\begin{eqnarray} +\begin_inset Formula \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_inset +\end_inset + +\end_layout -\layout Standard +\begin_layout Standard For completeness, here is one last equation. -\begin_inset Formula -\begin{equation} +\begin_inset Formula \begin{equation} e=mc^{2} \end{equation} -\end_inset +\end_inset -\layout References +\end_layout + +\begin_layout References \bibitem [Auri\`ere(1982)]{aur82} Auri\i \`{e} re, M. 1982, -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash aap -\latex default +\end_layout + +\end_inset + , 109, 301 -\layout References +\end_layout + +\begin_layout References \bibitem [Canizares et al.(1978)]{can78} Canizares, C. @@ -642,67 +833,105 @@ Canizares, C. A., Liller, W., and McClintock, J. E. 1978, -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash apj -\latex default +\end_layout + +\end_inset + , 224, 39 -\layout References +\end_layout + +\begin_layout References \bibitem [Djorgovski and King(1984)]{djo84} Djorgovski, S., and King, I. R. 1984, -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash apjl -\latex default +\end_layout + +\end_inset + , 277, L49 -\layout References +\end_layout + +\begin_layout References \bibitem [Hagiwara and Zeppenfeld(1986)]{hag86} Hagiwara, K., and Zeppenfeld, D. 1986, Nucl.Phys., 274, 1 -\layout References +\end_layout + +\begin_layout References \bibitem [Harris and van den Bergh(1984)]{har84} Harris, W. E., and van den Bergh, S. 1984, -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash aj -\latex default +\end_layout + +\end_inset + , 89, 1816 -\layout References +\end_layout + +\begin_layout References \bibitem [H\`enon(1961)]{hen61} H\i \'{e} non, M. 1961, Ann.d'Ap., 24, 369 -\layout References +\end_layout + +\begin_layout References \bibitem [King(1966)]{kin66} King, I. R. 1966, -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash aj -\latex default +\end_layout + +\end_inset + , 71, 276 -\layout References +\end_layout + +\begin_layout References \bibitem [King(1975)]{kin75} King, I. R. 1975, Dynamics of Stellar Systems, A. Hayli, Dordrecht: Reidel, 1975, 99 -\layout References +\end_layout + +\begin_layout References \bibitem [King et al.(1968)]{kin68} King, I. @@ -710,13 +939,21 @@ King, I. M., and White, R. E. 1968, -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash aj -\latex default +\end_layout + +\end_inset + , 73, 456 -\layout References +\end_layout + +\begin_layout References \bibitem [Kron et al.(1984)]{kro84} Kron, G. @@ -724,529 +961,1314 @@ Kron, G. V., and Wasserman, L. H. 1984, -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash pasp -\latex default +\end_layout + +\end_inset + , 96, 198 -\layout References +\end_layout + +\begin_layout References \bibitem [Lynden-Bell and Wood(1968)]{lyn68} Lynden-Bell, D., and Wood, R. 1968, -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard -\backslash +\backslash mnras -\latex default +\end_layout + +\end_inset + , 138, 495 -\layout References +\end_layout + +\begin_layout References \bibitem [Newell and O'Neil(1978)]{new78} Newell, E. B., and O'Neil, E. 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-12.052 -\newline +\end_layout + +\end_inset + + +\begin_inset Text + +\begin_layout Standard + 8 -\layout Standard +\end_layout + +\end_inset + + + + +\end_inset + + +\end_layout + +\begin_layout Standard -\latex latex +\begin_inset ERT +status collapsed -\backslash +\begin_layout Standard + +\backslash tablenotetext{a}{Sample footnote for table~ -\backslash +\backslash ref{tbl-2} that was generated with the -\backslash +\backslash LaTeX -\backslash +\backslash table environment} -\layout Standard +\end_layout + +\begin_layout Standard +\end_layout -\latex latex +\begin_layout Standard -\backslash +\backslash tablenotetext{b}{Yet another sample footnote for table~ -\backslash +\backslash ref{tbl-2}} -\layout Standard +\end_layout +\begin_layout Standard -\latex latex +\end_layout -\backslash +\begin_layout Standard + +\backslash tablenotetext{c}{Another sample footnote for table~ -\backslash +\backslash ref{tbl-2}} -\layout TableComments +\end_layout + +\end_inset + + +\end_layout + +\begin_layout TableComments We can also attach a long-ish paragraph of explanatory material to a table. Use -\backslash +\backslash tablerefs to append a list of references. The following references were from a different table: I've patched them in here to show how they look, but don't take them too seriously---I certainly have not. -\layout TableRefs +\end_layout + +\begin_layout TableRefs (1) Barbuy, Spite, & Spite 1985; (2) Bond 1980; (3) Carbon et al. 1987; (4) Hobbs & Duncan 1987; (5) Gilroy et al. @@ -1259,47 +2281,106 @@ tablerefs to append a list of references. 1984; (23) Spite & Spite 1986; (24) Hobbs & Thorburn 1991; (25) Hobbs et al. 1991; (26) Olsen 1983. -\end_float -\layout Standard +\end_layout + +\end_inset + +\end_layout + +\begin_layout Standard -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard % LyX can load deluxetable files verbatim. To see this in action, uncomment the following -\layout Standard +\end_layout + +\end_inset + + +\end_layout +\begin_layout Standard -\latex latex + +\begin_inset ERT +status collapsed + +\begin_layout Standard % line (delete the -\latex default +\end_layout + +\end_inset + \begin_inset Quotes eld -\end_inset +\end_inset -\latex latex +\begin_inset ERT +status collapsed + +\begin_layout Standard % -\latex default +\end_layout + +\end_inset + \begin_inset Quotes erd -\end_inset +\end_inset + +\begin_inset ERT +status collapsed -\latex latex +\begin_layout Standard ) and copy the file table.tex from the AASTeX 5.0 distribution into -\layout Standard +\end_layout +\end_inset -\latex latex + +\end_layout + +\begin_layout Standard + + +\begin_inset ERT +status collapsed + +\begin_layout Standard % the same directory as this file. -\layout Standard +\end_layout + +\end_inset + + +\end_layout +\begin_layout Standard -\latex latex + +\begin_inset ERT +status collapsed + +\begin_layout Standard % +\end_layout + +\end_inset + + \begin_inset Include \input{table} -\end_inset +\end_inset + + +\end_layout -\the_end +\end_body +\end_document