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lyx_mirror/lib/examples/aas_sample.lyx
Jean-Marc Lasgouttes 970386d4a8 update file formats 
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2003-01-17 13:50:11 +00:00

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#LyX 1.3 created this file. For more info see http://www.lyx.org/
\lyxformat 221
\textclass aastex
\begin_preamble
\newcommand{\vdag}{(v)^\dagger}
\newcommand{\myemail}{skywalker@galaxy.far.far.away}
\slugcomment{Not to appear in Nonlearned J., 45.}
\shorttitle{Djorgovski et al.}
\shortauthors{Collapsed Cores in Globular Clusters}
\end_preamble
\language english
\inputencoding default
\fontscheme default
\graphics default
\paperfontsize default
\spacing single
\papersize Default
\paperpackage a4
\use_geometry 0
\use_amsmath 0
\use_natbib 0
\use_numerical_citations 0
\paperorientation portrait
\secnumdepth 3
\tocdepth 3
\paragraph_separation indent
\defskip medskip
\quotes_language english
\quotes_times 2
\papercolumns 1
\papersides 1
\paperpagestyle default
\layout Title
Collapsed Cores in Globular Clusters, Gauge-Boson Couplings, and AASTeX
Examples
\layout Author
S.
Djorgovski
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
altaffilmark{1,2,3}
\end_inset
and Ivan R.
King
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
altaffilmark{1}
\end_inset
\layout Affiliation
Astronomy Department, University of California, Berkeley, CA 94720
\layout Author
C.
D.
Biemesderfer
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
altaffilmark{4,5}
\end_inset
\layout Affiliation
National Optical Astronomy Observatories, Tucson, AZ 85719
\layout Email
aastex-help@aas.org
\layout And
\layout Author
R.
J.
Hanisch
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
altaffilmark{5}
\end_inset
\layout Affiliation
Space Telescope Science Institute, Baltimore, MD 21218
\layout Standard
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
altaffiltext{1}{Visiting Astronomer, Cerro Tololo Inter-American Observatory.
CTIO is operated by AURA, Inc.
\backslash
under contract to the National Science Foundation.}
\layout Standard
\backslash
altaffiltext{2}{Society of Fellows, Harvard University.}
\layout Standard
\backslash
altaffiltext{3}{present address: Center for Astrophysics, 60 Garden Street,
Cambridge, MA 02138}
\layout Standard
\backslash
altaffiltext{4}{Visiting Programmer, Space Telescope Science Institute}
\layout Standard
\backslash
altaffiltext{5}{Patron, Alonso's Bar and Grill}
\end_inset
\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
clusters: globular, peanut---bosons: bozos
\layout Section
Introduction
\layout Standard
A focal problem today in the dynamics of globular clusters is core collapse.
It has been predicted by theory for decades
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
citep{hen61,lyn68,spi85}
\end_inset
, but observation has been less alert to the phenomenon.
For many years the central brightness peak in M15
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
citep{kin75,new78}
\end_inset
seemed a unique anomaly.
Then
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
citet{aur82}
\end_inset
suggested a central peak in NGC 6397, and a limited photographic survey
of ours
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
citep[Paper I]{djo84}
\end_inset
found three more cases, including NGC 6624, whose sharp center had often
been remarked on
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
citep{can78}
\end_inset
.
\layout Section
Observations
\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
500 chip and a GEC 575
\begin_inset Formula \( \times \)
\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
385, with
\begin_inset Formula \( B,V, \)
\end_inset
and
\begin_inset Formula \( R \)
\end_inset
filters, and an RCA 512
\begin_inset Formula \( \times \)
\end_inset
320, with
\begin_inset Formula \( U,B,V,R, \)
\end_inset
and
\begin_inset Formula \( I \)
\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
or even in
\begin_inset Formula \( B \)
\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
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
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
citep{kin68,pet76,har84,ort85}
\end_inset
, as well as photoelectric profiles
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
citep{kin66,kin75}
\end_inset
and electronographic profiles
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
citep{kro84}
\end_inset
.
In a few cases we judged normality by eye estimates on one of the Sky Surveys.
\layout Section
Helicity Amplitudes
\layout Standard
It has been realized that helicity amplitudes provide a convenient means
for Feynman diagram
\begin_inset Foot
collapsed true
\layout Standard
Footnotes can be inserted like this.
\end_inset
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
\begin_inset LatexCommand \cite{hag86}
\end_inset
; we briefly summarize below.
\layout Subsection
Formalism
\layout Standard
\begin_inset LatexCommand \label{bozomath}
\end_inset
\layout Standard
A tree-level amplitude in
\begin_inset Formula \( e^{+}e^{-} \)
\end_inset
collisions can be expressed in terms of fermion strings of the form
\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
where
\begin_inset Formula \( p \)
\end_inset
and
\begin_inset Formula \( \sigma \)
\end_inset
label the initial
\begin_inset Formula \( e^{\pm } \)
\end_inset
four-momenta and helicities
\begin_inset Formula \( (\sigma =\pm 1) \)
\end_inset
,
\begin_inset Formula \( \hat{a}_{i}=a^{\mu }_{i}\gamma _{\nu } \)
\end_inset
and
\begin_inset Formula \( P_{\tau }=\frac{1}{2}(1+\tau \gamma _{5}) \)
\end_inset
is a chirality projection operator
\begin_inset Formula \( (\tau =\pm1 ) \)
\end_inset
.
The
\begin_inset Formula \( a^{\mu }_{i} \)
\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
Figures 1 and 2 should appear side-by-side in print
\layout Standard
In the chiral representation the
\begin_inset Formula \( \gamma \)
\end_inset
matrices are expressed in terms of
\begin_inset Formula \( 2\times 2 \)
\end_inset
Pauli matrices
\begin_inset Formula \( \sigma \)
\end_inset
and the unit matrix 1 as
\begin_inset Formula \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 } & = & ({\textbf {1}},\pm \sigma ),\nonumber
\end{eqnarray}
\end_inset
giving
\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
The spinors are expressed in terms of two-component Weyl spinors as
\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
\layout Standard
The Weyl spinors are given in terms of helicity eigenstates
\begin_inset Formula \( \chi _{\lambda }(p) \)
\end_inset
with
\begin_inset Formula \( \lambda =\pm1 \)
\end_inset
by
\layout MathLetters
\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
\layout Section
Floating material and so forth
\layout Standard
Consider a task that computes profile parameters for a modified Lorentzian
of the form
\begin_inset Formula \begin{equation}
I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
\end{equation}
\end_inset
where
\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
\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
\begin_inset Formula \[
x_{1}=(x-x_{0})\cos \Theta +(y-y_{0})\sin \Theta \]
\end_inset
\begin_inset Formula \[
y_{1}=-(x-x_{0})\sin \Theta +(y-y_{0})\cos \Theta \]
\end_inset
\layout Standard
In these expressions
\begin_inset Formula \( x_{0} \)
\end_inset
,
\begin_inset Formula \( y_{0} \)
\end_inset
is the star center, and
\begin_inset Formula \( \Theta \)
\end_inset
is the angle with the
\begin_inset Formula \( x \)
\end_inset
axis.
Results of this task are shown in table\SpecialChar ~
\begin_inset LatexCommand \ref{tbl-2}
\end_inset
.
It is not clear how these sorts of analyses may affect determination of
\begin_inset Formula \( M_{\sun } \)
\end_inset
, but the assumption is that the alternate results should be less than 90
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
degr
\backslash
\end_inset
out of phase with previous values.
We have no observations of
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
ion{Ca}{2}
\end_inset
.
Roughly
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
slantfrac{4}{5}
\end_inset
of the electronically submitted abstracts for AAS meetings are error-free.
\layout Acknowledgements
\layout Standard
We are grateful to V.
Barger, T.
Han, and R.
J.
N.
Phillips for doing the math in section\SpecialChar ~
\begin_inset LatexCommand \ref{bozomath}
\end_inset
.
More information on the AASTeX macros package are available at
\begin_inset LatexCommand \url{http://www.aas.org/publications/aastex}
\end_inset
or the
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
anchor{ftp://www.aas.org/pubs/}{AAS ftp site}
\end_inset
.
\layout Appendix
\layout Section
Appendicial material
\layout Standard
Consider once again a task that computes profile parameters for a modified
Lorentzian of the form
\begin_inset Formula \begin{equation}
I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
\end{equation}
\end_inset
where
\layout MathLetters
\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
\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}
\case {y_{1}}{PR_{min}}
\end{array}\right) ^{2}}
\end{equation}
\end_inset
\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
\layout Standard
For completeness, here is one last equation.
\begin_inset Formula \begin{equation}
e=mc^{2}
\end{equation}
\end_inset
\layout References
\bibitem [Auri\`ere(1982)]{aur82}
Auri\i \`{e}
re, M.
1982,
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
aap
\end_inset
, 109, 301
\layout References
\bibitem [Canizares et al.(1978)]{can78}
Canizares, C.
R., Grindlay, J.
E., Hiltner, W.
A., Liller, W., and McClintock, J.
E.
1978,
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
apj
\end_inset
, 224, 39
\layout References
\bibitem [Djorgovski and King(1984)]{djo84}
Djorgovski, S., and King, I.
R.
1984,
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
apjl
\end_inset
, 277, L49
\layout References
\bibitem [Hagiwara and Zeppenfeld(1986)]{hag86}
Hagiwara, K., and Zeppenfeld, D.
1986, Nucl.Phys., 274, 1
\layout References
\bibitem [Harris and van den Bergh(1984)]{har84}
Harris, W.
E., and van den Bergh, S.
1984,
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
aj
\end_inset
, 89, 1816
\layout References
\bibitem [H\`enon(1961)]{hen61}
H\i \'{e}
non, M.
1961, Ann.d'Ap., 24, 369
\layout References
\bibitem [King(1966)]{kin66}
King, I.
R.
1966,
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
aj
\end_inset
, 71, 276
\layout References
\bibitem [King(1975)]{kin75}
King, I.
R.
1975, Dynamics of Stellar Systems, A.
Hayli, Dordrecht: Reidel, 1975, 99
\layout References
\bibitem [King et al.(1968)]{kin68}
King, I.
R., Hedemann, E., Hodge, S.
M., and White, R.
E.
1968,
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
aj
\end_inset
, 73, 456
\layout References
\bibitem [Kron et al.(1984)]{kro84}
Kron, G.
E., Hewitt, A.
V., and Wasserman, L.
H.
1984,
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
pasp
\end_inset
, 96, 198
\layout References
\bibitem [Lynden-Bell and Wood(1968)]{lyn68}
Lynden-Bell, D., and Wood, R.
1968,
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
mnras
\end_inset
, 138, 495
\layout References
\bibitem [Newell and O'Neil(1978)]{new78}
Newell, E.
B., and O'Neil, E.
J.
1978,
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
apjs
\end_inset
, 37, 27
\layout References
\bibitem [Ortolani et al.(1985)]{ort85}
Ortolani, S., Rosino, L., and Sandage, A.
1985,
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
aj
\end_inset
, 90, 473
\layout References
\bibitem [Peterson(1976)]{pet76}
Peterson, C.
J.
1976,
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
aj
\end_inset
, 81, 617
\layout References
\bibitem [Spitzer(1985)]{spi85}
Spitzer, L.
1985, Dynamics of Star Clusters, J.
Goodman and P.
Hut, Dordrecht: Reidel, 109
\layout Standard
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
clearpage
\end_inset
\layout FigCaption
\begin_inset LatexCommand \label{fig1}
\end_inset
This is the first figure and it uses sgi9259.eps as its EPS figure file.
\layout FigCaption
\begin_inset LatexCommand \label{fig2}
\end_inset
This is an example of a long figure caption that must be set as a paragraph.
The processor has to buffer the text of the caption, so it is good not
to be too wordy, but that would make for poor communication as well.
\layout FigCaption
\begin_inset LatexCommand \label{fig3}
\end_inset
This figure has no associated EPS file, so the optional parameter is omitted.
\layout Standard
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
clearpage
\end_inset
\layout Standard
\begin_inset Float table
wide false
collapsed false
\layout Caption
\added_space_bottom medskip
Terribly relevant tabular information.
\begin_inset LatexCommand \label{tbl-2}
\end_inset
\layout Standard
\begin_inset Tabular
<lyxtabular version="3" rows="7" columns="13">
<features endhead="-1" endfirsthead="-1" endfoot="-1" endlastfoot="-1">
<column alignment="center" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="center" valignment="top" width="0pt">
<row>
<cell alignment="center" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
Star
\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
Height
\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
\begin_inset Formula \( d_{x} \)
\end_inset
\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
\begin_inset Formula \( d_{y} \)
\end_inset
\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
\begin_inset Formula \( n \)
\end_inset
\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
\begin_inset Formula \( \chi ^{2} \)
\end_inset
\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
\begin_inset Formula \( R_{maj} \)
\end_inset
\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
\begin_inset Formula \( R_{min} \)
\end_inset
\end_inset
</cell>
<cell multicolumn="1" alignment="center" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
\begin_inset Formula \( P \)
\end_inset
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
tablenotemark{a}
\end_inset
\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
\begin_inset Formula \( PR_{maj} \)
\end_inset
\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
\begin_inset Formula \( PR_{min} \)
\end_inset
\end_inset
</cell>
<cell multicolumn="1" alignment="center" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
\begin_inset Formula \( \Theta \)
\end_inset
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
tablenotemark{b}
\end_inset
\end_inset
</cell>
<cell alignment="center" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
Ref.
\end_inset
</cell>
</row>
<row>
<cell alignment="center" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
tableline
\backslash
tableline
\end_inset
1
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
33472.5
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
-0.1
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
0.4
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
53
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
27.4
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
2.065
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
1.940
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
3.900
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
68.3
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
116.2
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
-27.639
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
1,2
\end_inset
</cell>
</row>
<row>
<cell alignment="center" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
2
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
27802.4
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
-0.3
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
-0.2
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
60
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
3.7
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
1.628
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
1.510
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
2.156
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
6.8
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
7.5
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
-26.764
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
3
\end_inset
</cell>
</row>
<row>
<cell alignment="center" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
3
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
29210.6
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</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
0.9
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
0.3
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
60
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
3.4
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
1.622
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
1.551
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
2.159
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</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
6.7
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
7.3
\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
-40.272
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</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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4
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<row>
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\begin_inset Text
\layout Standard
4
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</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
32733.8
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
-1.2
\begin_inset ERT
status Collapsed
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\backslash
tablenotemark{c}
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\end_inset
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<cell alignment="right" valignment="top" usebox="none">
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-0.5
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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41
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
54.8
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
2.282
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</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
2.156
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</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
4.313
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</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
117.4
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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78.2
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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-35.847
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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5,6
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<row>
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\begin_inset Text
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5
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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9607.4
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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-0.4
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
-0.4
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</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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60
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</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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1.4
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<cell alignment="right" valignment="top" usebox="none">
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\layout Standard
1.669
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status Collapsed
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tablenotemark{c}
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1.574
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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2.343
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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8.0
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<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
\layout Standard
8.9
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</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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-33.417
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</cell>
<cell alignment="right" valignment="top" usebox="none">
\begin_inset Text
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7
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<row>
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\begin_inset Text
\layout Standard
6
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</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
31638.6
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</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
1.6
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</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
0.1
\end_inset
</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
39
\end_inset
</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
315.2
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</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
3.433
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</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
3.075
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</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
7.488
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</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
92.1
\end_inset
</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
25.3
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</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
-12.052
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</cell>
<cell alignment="right" valignment="top" bottomline="true" usebox="none">
\begin_inset Text
\layout Standard
8
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</cell>
</row>
</lyxtabular>
\end_inset
\layout Standard
\begin_inset ERT
status Collapsed
\layout Standard
\backslash
tablenotetext{a}{Sample footnote for table~
\backslash
ref{tbl-2} that was generated with the
\backslash
LaTeX
\backslash
table environment}
\layout Standard
\backslash
tablenotetext{b}{Yet another sample footnote for table~
\backslash
ref{tbl-2}}
\layout Standard
\backslash
tablenotetext{c}{Another sample footnote for table~
\backslash
ref{tbl-2}}
\end_inset
\layout TableComments
We can also attach a long-ish paragraph of explanatory material to a table.
Use
\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
(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_inset
\layout Standard
\begin_inset ERT
status Collapsed
\layout Standard
% LyX can load deluxetable files verbatim.
To see this in action, uncomment the following
\end_inset
\layout Standard
\begin_inset ERT
status Collapsed
\layout Standard
% line (delete the
\end_inset
\begin_inset Quotes eld
\end_inset
\begin_inset ERT
status Collapsed
\layout Standard
%
\end_inset
\begin_inset Quotes erd
\end_inset
\begin_inset ERT
status Collapsed
\layout Standard
) and copy the file table.tex from the AASTeX 5.0 distribution into
\end_inset
\layout Standard
\begin_inset ERT
status Collapsed
\layout Standard
% the same directory as this file.
\end_inset
\layout Standard
\begin_inset ERT
status Collapsed
\layout Standard
%
\end_inset
\begin_inset Include \input{table}
\end_inset
\the_end
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