lyx_mirror/lib/examples/aas_sample.lyx

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#This file was created by <mike> Sun Jul 25 23:59:27 1999
#LyX 1.0 (C) 1995-1999 Matthias Ettrich and the LyX Team
\lyxformat 2.15
\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
\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
\latex latex
\latex default
Examples
\layout Author
S.
Djorgovski
\latex latex
\backslash
altaffilmark{1,2,3}
\latex default
and Ivan R.
King
\latex latex
\backslash
altaffilmark{1}
\layout Affiliation
Astronomy Department, University of California, Berkeley, CA 94720
\layout Author
C.
D.
Biemesderfer
\latex latex
\backslash
altaffilmark{4,5}
\layout Affiliation
National Optical Astronomy Observatories, Tucson, AZ 85719
\layout Email
aastex-help@aas.org
\layout And
\layout Author
R.
J.
Hanisch
\latex latex
\backslash
altaffilmark{5}
\layout Affiliation
Space Telescope Science Institute, Baltimore, MD 21218
\layout Standard
\latex latex
\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
\latex latex
\backslash
altaffiltext{2}{Society of Fellows, Harvard University.}
\layout Standard
\latex latex
\backslash
altaffiltext{3}{present address: Center for Astrophysics, 60 Garden Street,
Cambridge, MA 02138}
\layout Standard
\latex latex
\backslash
altaffiltext{4}{Visiting Programmer, Space Telescope Science Institute}
\layout Standard
\latex latex
\backslash
altaffiltext{5}{Patron, Alonso's Bar and Grill}
\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
\latex latex
\backslash
citep{hen61,lyn68,spi85}
\latex default
, but observation has been less alert to the phenomenon.
For many years the central brightness peak in M15
\latex latex
\backslash
citep{kin75,new78}
\latex default
seemed a unique anomaly.
Then
\latex latex
\backslash
citet{aur82}
\latex default
suggested a central peak in NGC 6397, and a limited photographic survey
of ours
\latex latex
\backslash
citep[Paper I]{djo84}
\latex default
found three more cases, including NGC 6624, whose sharp center had often
been remarked on
\latex latex
\backslash
citep{can78}
\latex default
.
\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
\latex latex
\backslash
citep{kin68,pet76,har84,ort85}
\latex default
, as well as photoelectric profiles
\latex latex
\backslash
citep{kin66,kin75}
\latex default
and electronographic profiles
\latex latex
\backslash
citep{kro84}
\latex default
.
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_float footnote
\layout Standard
Footnotes can be inserted like this.
\end_float
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
\protected_separator
\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
\latex latex
\backslash
degr
\backslash
\latex default
out of phase with previous values.
We have no observations of
\latex latex
\backslash
ion{Ca}{2}
\latex default
.
Roughly
\latex latex
\backslash
slantfrac{4}{5}
\latex default
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
\protected_separator
\begin_inset LatexCommand \ref{bozomath}
\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
\latex default
or the
\latex latex
\backslash
anchor{ftp://www.aas.org/pubs/}{AAS ftp site}
\latex default
.
\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,
\latex latex
\backslash
aap
\latex default
, 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,
\latex latex
\backslash
apj
\latex default
, 224, 39
\layout References
\bibitem [Djorgovski and King(1984)]{djo84}
Djorgovski, S., and King, I.
R.
1984,
\latex latex
\backslash
apjl
\latex default
, 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,
\latex latex
\backslash
aj
\latex default
, 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,
\latex latex
\backslash
aj
\latex default
, 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,
\latex latex
\backslash
aj
\latex default
, 73, 456
\layout References
\bibitem [Kron et al.(1984)]{kro84}
Kron, G.
E., Hewitt, A.
V., and Wasserman, L.
H.
1984,
\latex latex
\backslash
pasp
\latex default
, 96, 198
\layout References
\bibitem [Lynden-Bell and Wood(1968)]{lyn68}
Lynden-Bell, D., and Wood, R.
1968,
\latex latex
\backslash
mnras
\latex default
, 138, 495
\layout References
\bibitem [Newell and O'Neil(1978)]{new78}
Newell, E.
B., and O'Neil, E.
J.
1978,
\latex latex
\backslash
apjs
\latex default
, 37, 27
\layout References
\bibitem [Ortolani et al.(1985)]{ort85}
Ortolani, S., Rosino, L., and Sandage, A.
1985,
\latex latex
\backslash
aj
\latex default
, 90, 473
\layout References
\bibitem [Peterson(1976)]{pet76}
Peterson, C.
J.
1976,
\latex latex
\backslash
aj
\latex default
, 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
\latex latex
\backslash
clearpage
\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
\latex latex
\backslash
clearpage
\layout Standard
\begin_float tab
\layout Caption
\added_space_bottom medskip
Terribly relevant tabular information.
\begin_inset LatexCommand \label{tbl-2}
\end_inset
\layout Standard
\LyXTable
multicol5
7 13 0 0 -1 -1 -1 -1
0 0 0 0
0 0 0 0
0 0 0 0
0 0 0 0
0 0 0 0
0 0 0 0
0 0 0 0
8 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
8 0 0 "" ""
0 8 1 1 0 0 0 "" ""
0 4 1 1 0 0 0 "" ""
0 4 1 1 0 0 0 "" ""
0 4 1 1 0 0 0 "" ""
0 4 1 1 0 0 0 "" ""
0 4 1 1 0 0 0 "" ""
0 4 1 1 0 0 0 "" ""
0 4 1 1 0 0 0 "" ""
1 8 0 0 0 0 0 "" ""
0 4 1 1 0 0 0 "" ""
0 4 1 1 0 0 0 "" ""
1 8 0 0 0 0 0 "" ""
0 8 0 0 0 0 0 "" ""
0 8 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 8 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 8 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 8 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 8 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 8 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
Star
\newline
Height
\newline
\begin_inset Formula \( d_{x} \)
\end_inset
\newline
\begin_inset Formula \( d_{y} \)
\end_inset
\newline
\begin_inset Formula \( n \)
\end_inset
\newline
\begin_inset Formula \( \chi ^{2} \)
\end_inset
\newline
\begin_inset Formula \( R_{maj} \)
\end_inset
\newline
\begin_inset Formula \( R_{min} \)
\end_inset
\newline
\begin_inset Formula \( P \)
\end_inset
\latex latex
\backslash
tablenotemark{a}
\latex default
\newline
\begin_inset Formula \( PR_{maj} \)
\end_inset
\newline
\begin_inset Formula \( PR_{min} \)
\end_inset
\newline
\begin_inset Formula \( \Theta \)
\end_inset
\latex latex
\backslash
tablenotemark{b}
\latex default
\newline
Ref.
\newline
\latex latex
\backslash
tableline
\backslash
tableline
\latex default
1
\newline
33472.5
\newline
-0.1
\newline
0.4
\newline
53
\newline
27.4
\newline
2.065
\newline
1.940
\newline
3.900
\newline
68.3
\newline
116.2
\newline
-27.639
\newline
1,2
\newline
2
\newline
27802.4
\newline
-0.3
\newline
-0.2
\newline
60
\newline
3.7
\newline
1.628
\newline
1.510
\newline
2.156
\newline
6.8
\newline
7.5
\newline
-26.764
\newline
3
\newline
3
\newline
29210.6
\newline
0.9
\newline
0.3
\newline
60
\newline
3.4
\newline
1.622
\newline
1.551
\newline
2.159
\newline
6.7
\newline
7.3
\newline
-40.272
\newline
4
\newline
4
\newline
32733.8
\newline
-1.2
\latex latex
\backslash
tablenotemark{c}
\latex default
\newline
-0.5
\newline
41
\newline
54.8
\newline
2.282
\newline
2.156
\newline
4.313
\newline
117.4
\newline
78.2
\newline
-35.847
\newline
5,6
\newline
5
\newline
9607.4
\newline
-0.4
\newline
-0.4
\newline
60
\newline
1.4
\newline
1.669
\latex latex
\backslash
tablenotemark{c}
\latex default
\newline
1.574
\newline
2.343
\newline
8.0
\newline
8.9
\newline
-33.417
\newline
7
\newline
6
\newline
31638.6
\newline
1.6
\newline
0.1
\newline
39
\newline
315.2
\newline
3.433
\newline
3.075
\newline
7.488
\newline
92.1
\newline
25.3
\newline
-12.052
\newline
8
\layout Standard
\latex latex
\backslash
tablenotetext{a}{Sample footnote for table~
\backslash
ref{tbl-2} that was generated with the
\backslash
LaTeX
\backslash
table environment}
\layout Standard
\latex latex
\backslash
tablenotetext{b}{Yet another sample footnote for table~
\backslash
ref{tbl-2}}
\layout Standard
\latex latex
\backslash
tablenotetext{c}{Another sample footnote for table~
\backslash
ref{tbl-2}}
\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_float
\layout Standard
\latex latex
% LyX can load deluxetable files verbatim.
To see this in action, uncomment the following
\layout Standard
\latex latex
% line (delete the
\latex default
\begin_inset Quotes eld
\end_inset
\latex latex
%
\latex default
\begin_inset Quotes erd
\end_inset
\latex latex
) and copy the file table.tex from the AASTeX 5.0 distribution into
\layout Standard
\latex latex
% the same directory as this file.
\layout Standard
\latex latex
%
\begin_inset Include \input{table}
\end_inset
\the_end