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8 \begin_preamble
9 \newcommand{\myemail}{skywalker@galaxy.far.far.away}
10 %\slugcomment{Not to appear in Nonlearned J., 45.}
11 \shorttitle{Djorgovski et al.}
12 \shortauthors{Collapsed Cores in Globular Clusters}
13 \end_preamble
14 \use_default_options true
15 \maintain_unincluded_children no
16 \language english
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93 \begin_body
94
95 \begin_layout Standard
96 \begin_inset Note Note
97 status open
98
99 \begin_layout Plain Layout
100 \noindent
101 \align left
102 Sample document for contributions to journals of the American Astronomical
103  Society (AAS).
104  Please consult the 
105 \begin_inset CommandInset href
106 LatexCommand href
107 name "AASTeX user guide"
108 target "http://journals.aas.org/authors/aastex/aasguide.html"
109 literal "false"
110
111 \end_inset
112
113  for details on how to use AASTeX.
114  
115 \end_layout
116
117 \begin_layout Plain Layout
118 \noindent
119 \align left
120 An up-to-date sample LaTeX article using AASTeX is available under 
121 \begin_inset Flex URL
122 status open
123
124 \begin_layout Plain Layout
125
126 http://journals.aas.org/authors/aastex/aastex.html#_download
127 \end_layout
128
129 \end_inset
130
131 .
132 \end_layout
133
134 \end_inset
135
136
137 \begin_inset Note Note
138 status open
139
140 \begin_layout Plain Layout
141 \noindent
142 \align left
143 The AASTeX document class uses a different name since version 6.0 (2016/02/16).
144  Depending on the version installed on your system, set the document class
145  to American Astronomical Society (AASTeX v.
146  6) or American Astronomical Society (AASTeX v.
147  5).
148  
149 \end_layout
150
151 \begin_layout Plain Layout
152 \noindent
153 \align left
154 New features (cf.
155  
156 \begin_inset Flex URL
157 status collapsed
158
159 \begin_layout Plain Layout
160
161 http://journals.aas.org/authors/aastex/revisionhistory.html
162 \end_layout
163
164 \end_inset
165
166 ) are only partially supported by LyX (see 
167 \begin_inset Flex URL
168 status collapsed
169
170 \begin_layout Plain Layout
171
172 https://www.lyx.org/trac/ticket/10027
173 \end_layout
174
175 \end_inset
176
177 ).
178 \end_layout
179
180 \end_inset
181
182
183 \end_layout
184
185 \begin_layout Title
186 Collapsed Cores in Globular Clusters,  Gauge-Boson Couplings, and AAS\SpecialChar TeX
187  Examples
188 \end_layout
189
190 \begin_layout Author
191 S.
192  Djorgovski and Ivan R.
193  King
194 \end_layout
195
196 \begin_layout Affiliation
197 Astronomy Department, University of California, Berkeley, CA 94720
198 \end_layout
199
200 \begin_layout Altaffilation
201 Visiting Astronomer
202 \begin_inset Newline newline
203 \end_inset
204
205  Cerro Tololo Inter-American Observatory.
206 \begin_inset Newline newline
207 \end_inset
208
209 CTIO is operated by AURA Inc.
210 \begin_inset space \space{}
211 \end_inset
212
213 under contract to the National Science Foundation.
214 \end_layout
215
216 \begin_layout Altaffilation
217 Society of Fellows, Harvard University.
218 \end_layout
219
220 \begin_layout Altaffilation
221 present address: Center for Astrophysics
222 \begin_inset Newline newline
223 \end_inset
224
225 60 Garden Street, Cambridge, MA 02138
226 \end_layout
227
228 \begin_layout Author
229 C.
230  D.
231  Biemesderfer
232 \end_layout
233
234 \begin_layout Affiliation
235 National Optical Astronomy Observatories, Tucson, AZ 85719
236 \end_layout
237
238 \begin_layout Altaffilation
239 Visiting Programmer, Space Telescope Science Institute
240 \end_layout
241
242 \begin_layout Altaffilation
243 Patron, Alonso's Bar and Grill
244 \end_layout
245
246 \begin_layout Email
247 aastex-help@aas.org
248 \end_layout
249
250 \begin_layout Author
251 R.
252  J.
253  Hanisch
254 \end_layout
255
256 \begin_layout Affiliation
257 Space Telescope Science Institute, Baltimore, MD 21218
258 \end_layout
259
260 \begin_layout Altaffilation
261 Patron, Alonso's Bar and Grill
262 \end_layout
263
264 \begin_layout Abstract
265 This is a preliminary report on surface photometry of the major fraction
266  of known globular clusters, to see which of them show the signs of a collapsed
267  core.
268  We also explore some diversionary mathematics and recreational tables.
269  
270 \end_layout
271
272 \begin_layout Keywords
273 clusters: globular, peanut—bosons: bozos
274 \end_layout
275
276 \begin_layout Section
277 Introduction
278 \end_layout
279
280 \begin_layout Standard
281 A focal problem today in the dynamics of globular clusters is core collapse.
282  It has been predicted by theory for decades 
283 \begin_inset CommandInset citation
284 LatexCommand citep
285 key "hen61,lyn68,spi85"
286 literal "false"
287
288 \end_inset
289
290 , but observation has been less alert to the phenomenon.
291  For many years the central brightness peak in M15 
292 \begin_inset CommandInset citation
293 LatexCommand citep
294 key "kin75,new78"
295 literal "false"
296
297 \end_inset
298
299  seemed a unique anomaly.
300  Then 
301 \begin_inset CommandInset citation
302 LatexCommand citep
303 key "aur82"
304 literal "false"
305
306 \end_inset
307
308  suggested a central peak in NGC 6397, and a limited photographic survey
309  of ours 
310 \begin_inset CommandInset citation
311 LatexCommand citep
312 after "Paper I"
313 key "djo84"
314 literal "false"
315
316 \end_inset
317
318  found three more cases, including NGC 6624, whose sharp center had often
319  been remarked on 
320 \begin_inset CommandInset citation
321 LatexCommand citep
322 key "can78"
323 literal "false"
324
325 \end_inset
326
327 .
328  
329 \end_layout
330
331 \begin_layout Section
332 Observations
333 \end_layout
334
335 \begin_layout Standard
336 All our observations were short direct exposures with CCD's.
337  At Lick Observatory we used a TI 500
338 \begin_inset Formula $\times$
339 \end_inset
340
341 500 chip and a GEC 575
342 \begin_inset Formula $\times$
343 \end_inset
344
345 385, on the 1-m Nickel reflector.
346  The only filter available at Lick was red.
347  At CTIO we used a GEC 575
348 \begin_inset Formula $\times$
349 \end_inset
350
351 385, with 
352 \begin_inset Formula $B,V,$
353 \end_inset
354
355  and 
356 \begin_inset Formula $R$
357 \end_inset
358
359  filters, and an RCA 512
360 \begin_inset Formula $\times$
361 \end_inset
362
363 320, with 
364 \begin_inset Formula $U,B,V,R,$
365 \end_inset
366
367  and 
368 \begin_inset Formula $I$
369 \end_inset
370
371  filters, on the 1.5-m reflector.
372  In the CTIO observations we tried to concentrate on the shortest practicable
373  wavelengths; but faintness, reddening, and poor short-wavelength sensitivity
374  often kept us from observing in 
375 \begin_inset Formula $U$
376 \end_inset
377
378  or even in 
379 \begin_inset Formula $B$
380 \end_inset
381
382 .
383  All four cameras had scales of the order of 0.4 arcsec/pixel, and our field
384  sizes were around 3 arcmin.
385 \end_layout
386
387 \begin_layout Standard
388 The CCD images are unfortunately not always suitable, for very poor clusters
389  or for clusters with large cores.
390  Since the latter are easily studied by other means, we augmented our own
391  CCD profiles by collecting from the literature a number of star-count profiles
392  
393 \begin_inset CommandInset citation
394 LatexCommand citep
395 key "kin68,pet76,har84,ort85"
396 literal "false"
397
398 \end_inset
399
400 , as well as photoelectric profiles 
401 \begin_inset CommandInset citation
402 LatexCommand citep
403 key "kin66,kin75"
404 literal "false"
405
406 \end_inset
407
408  and electronographic profiles 
409 \begin_inset CommandInset citation
410 LatexCommand citep
411 key "kro84"
412 literal "false"
413
414 \end_inset
415
416 .
417  In a few cases we judged normality by eye estimates on one of the Sky Surveys.
418 \end_layout
419
420 \begin_layout Section
421 Helicity Amplitudes
422 \end_layout
423
424 \begin_layout Standard
425 It has been realized that helicity amplitudes provide a convenient means
426  for Feynman diagram
427 \begin_inset Foot
428 status collapsed
429
430 \begin_layout Plain Layout
431 Footnotes can be inserted like this.
432 \end_layout
433
434 \end_inset
435
436  evaluations.
437  These amplitude-level techniques are particularly convenient for calculations
438  involving many Feynman diagrams, where the usual trace techniques for the
439  amplitude squared becomes unwieldy.
440  Our calculations use the helicity techniques developed by other authors
441  
442 \begin_inset CommandInset citation
443 LatexCommand cite
444 key "hag86"
445 literal "true"
446
447 \end_inset
448
449 ; we briefly summarize below.
450 \end_layout
451
452 \begin_layout Subsection
453 Formalism
454 \end_layout
455
456 \begin_layout Standard
457 \begin_inset CommandInset label
458 LatexCommand label
459 name "bozomath"
460
461 \end_inset
462
463
464 \end_layout
465
466 \begin_layout Standard
467 A tree-level amplitude in 
468 \begin_inset Formula $e^{+}e^{-}$
469 \end_inset
470
471  collisions can be expressed in terms of fermion strings of the form 
472 \begin_inset Formula 
473 \begin{equation}
474 \bar{v}(p_{2},\sigma_{2})P_{-\tau}\hat{a}_{1}\hat{a}_{2}\cdots\hat{a}_{n}u(p_{1},\sigma_{1}),
475 \end{equation}
476
477 \end_inset
478
479  where 
480 \begin_inset Formula $p$
481 \end_inset
482
483  and 
484 \begin_inset Formula $\sigma$
485 \end_inset
486
487  label the initial 
488 \begin_inset Formula $e^{\pm}$
489 \end_inset
490
491  four-momenta and helicities 
492 \begin_inset Formula $(\sigma=\pm1)$
493 \end_inset
494
495
496 \begin_inset Formula $\hat{a}_{i}=a_{i}^{\mu}\gamma_{\nu}$
497 \end_inset
498
499  and 
500 \begin_inset Formula $P_{\tau}=\frac{1}{2}(1+\tau\gamma_{5})$
501 \end_inset
502
503  is a chirality projection operator 
504 \begin_inset Formula $(\tau=\pm1)$
505 \end_inset
506
507 .
508  The 
509 \begin_inset Formula $a_{i}^{\mu}$
510 \end_inset
511
512  may be formed from particle four-momenta, gauge-boson polarization vectors
513  or fermion strings with an uncontracted Lorentz index associated with final-sta
514 te fermions.
515 \end_layout
516
517 \begin_layout NoteToEditor
518 Figures 1 and 2 should appear side-by-side in print
519 \end_layout
520
521 \begin_layout Standard
522 In the chiral representation the 
523 \begin_inset Formula $\gamma$
524 \end_inset
525
526  matrices are expressed in terms of 
527 \begin_inset Formula $2\times2$
528 \end_inset
529
530  Pauli matrices 
531 \begin_inset Formula $\sigma$
532 \end_inset
533
534  and the unit matrix 1 as 
535 \begin_inset Formula 
536 \begin{eqnarray*}
537 \gamma^{\mu} & = & \left(\begin{array}{cc}
538 0 & \sigma_{+}^{\mu}\\
539 \sigma_{-}^{\mu} & 0
540 \end{array}\right),\gamma^{5}=\left(\begin{array}{cc}
541 -1 & 0\\
542 0 & 1
543 \end{array}\right),\\
544 \sigma_{\pm}^{\mu} & = & ({\textbf{1}},\pm\sigma),
545 \end{eqnarray*}
546
547 \end_inset
548
549  giving 
550 \begin_inset Formula 
551 \begin{equation}
552 \hat{a}=\left(\begin{array}{cc}
553 0 & (\hat{a})_{+}\\
554 (\hat{a})_{-} & 0
555 \end{array}\right),(\hat{a})_{\pm}=a_{\mu}\sigma_{\pm}^{\mu},
556 \end{equation}
557
558 \end_inset
559
560  The spinors are expressed in terms of two-component Weyl spinors as 
561 \begin_inset Formula 
562 \begin{equation}
563 u=\left(\begin{array}{c}
564 (u)_{-}\\
565 (u)_{+}
566 \end{array}\right),v={\textbf{(}}\vdag_{+}{\textbf{,}}\vdag_{-}{\textbf{)}}.
567 \end{equation}
568
569 \end_inset
570
571
572 \end_layout
573
574 \begin_layout Standard
575 The Weyl spinors are given in terms of helicity eigenstates 
576 \begin_inset Formula $\chi_{\lambda}(p)$
577 \end_inset
578
579  with 
580 \begin_inset Formula $\lambda=\pm1$
581 \end_inset
582
583  by 
584 \end_layout
585
586 \begin_layout MathLetters
587 \begin_inset Formula 
588 \begin{eqnarray}
589 u(p,\lambda)_{\pm} & = & (E\pm\lambda|{\textbf{p}}|)^{1/2}\chi_{\lambda}(p),\\
590 v(p,\lambda)_{\pm} & = & \pm\lambda(E\mp\lambda|{\textbf{p}}|)^{1/2}\chi_{-\lambda}(p)
591 \end{eqnarray}
592
593 \end_inset
594
595
596 \end_layout
597
598 \begin_layout Section
599 Floating material and so forth
600 \end_layout
601
602 \begin_layout Standard
603 Consider a task that computes profile parameters for a modified Lorentzian
604  of the form 
605 \begin_inset Formula 
606 \begin{equation}
607 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
608 \end{equation}
609
610 \end_inset
611
612  where 
613 \begin_inset Formula 
614 \[
615 d_{1}=\sqrt{\left(\begin{array}{c}
616 \frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
617 \frac{y_{1}}{R_{min}}\end{array}\right)^{2}}
618 \]
619
620 \end_inset
621
622
623 \begin_inset Formula 
624 \[
625 d_{2}=\sqrt{\left(\begin{array}{c}
626 \frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
627 \case{y_{1}}{PR_{min}}\end{array}\right)^{2}}
628 \]
629
630 \end_inset
631
632
633 \begin_inset Formula 
634 \[
635 x_{1}=(x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta
636 \]
637
638 \end_inset
639
640
641 \begin_inset Formula 
642 \[
643 y_{1}=-(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta
644 \]
645
646 \end_inset
647
648
649 \end_layout
650
651 \begin_layout Standard
652 In these expressions 
653 \begin_inset Formula $x_{0}$
654 \end_inset
655
656 ,
657 \begin_inset Formula $y_{0}$
658 \end_inset
659
660  is the star center, and 
661 \begin_inset Formula $\Theta$
662 \end_inset
663
664  is the angle with the 
665 \begin_inset Formula $x$
666 \end_inset
667
668  axis.
669  Results of this task are shown in table
670 \begin_inset space ~
671 \end_inset
672
673
674 \begin_inset CommandInset ref
675 LatexCommand ref
676 reference "tbl-2"
677
678 \end_inset
679
680 .
681  It is not clear how these sorts of analyses may affect determination of
682  
683 \begin_inset Formula $M_{\text{\sun}}$
684 \end_inset
685
686 , but the assumption is that the alternate results should be less than 90°
687  out of phase with previous values.
688  We have no observations of 
689 \begin_inset Preview
690
691 \begin_layout Standard
692 \begin_inset ERT
693 status open
694
695 \begin_layout Plain Layout
696
697
698 \backslash
699 ion{Ca}{2}
700 \end_layout
701
702 \end_inset
703
704
705 \end_layout
706
707 \end_inset
708
709 .
710  Roughly 
711 \begin_inset Formula $\nicefrac{4}{5}$
712 \end_inset
713
714  of the electronically submitted abstracts for AAS meetings are error-free.
715  
716 \end_layout
717
718 \begin_layout Acknowledgements
719 We are grateful to V.
720  Barger, T.
721  Han, and R.
722  J.
723  N.
724  Phillips for doing the math in section
725 \begin_inset space ~
726 \end_inset
727
728
729 \begin_inset CommandInset ref
730 LatexCommand ref
731 reference "bozomath"
732
733 \end_inset
734
735 .
736  More information on the AAS\SpecialChar TeX
737  macros package are available at 
738 \begin_inset Flex URL
739 status collapsed
740
741 \begin_layout Plain Layout
742
743 http://www.aas.org/publications/aastex
744 \end_layout
745
746 \end_inset
747
748  or the 
749 \begin_inset CommandInset href
750 LatexCommand href
751 name "AAS ftp site"
752 target "ftp://www.aas.org/pubs/AAS ftp site"
753 literal "false"
754
755 \end_inset
756
757 .
758 \end_layout
759
760 \begin_layout Software
761 IRAF, AIPS, Astropy, ...
762 \end_layout
763
764 \begin_layout Appendix
765
766 \end_layout
767
768 \begin_layout Bibliography
769 \begin_inset CommandInset bibitem
770 LatexCommand bibitem
771 label "Auri\\`ere(1982)"
772 key "aur82"
773 literal "true"
774
775 \end_inset
776
777 Aurière, M.
778  1982, 
779 \begin_inset ERT
780 status collapsed
781
782 \begin_layout Plain Layout
783
784
785 \backslash
786 aap
787 \end_layout
788
789 \end_inset
790
791 , 109, 301 
792 \end_layout
793
794 \begin_layout Bibliography
795 \begin_inset CommandInset bibitem
796 LatexCommand bibitem
797 label "Canizares et al.(1978)"
798 key "can78"
799 literal "true"
800
801 \end_inset
802
803 Canizares, C.
804  R., Grindlay, J.
805  E., Hiltner, W.
806  A., Liller, W., and McClintock, J.
807  E.
808  1978, 
809 \begin_inset ERT
810 status collapsed
811
812 \begin_layout Plain Layout
813
814
815 \backslash
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868 Hagiwara, K., and Zeppenfeld, D.
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929
930 \backslash
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948 King, I.
949  R.
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963 King, I.
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965  M., and White, R.
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1003 \backslash
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1009 , 96, 198 
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1038
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1083 Ortolani, S., Rosino, L., and Sandage, A.
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1095 \end_inset
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1097 , 90, 473 
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1109 Peterson, C.
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1122 \end_inset
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1124 , 81, 617 
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1136 Spitzer, L.
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1728 \end_inset
1729 </cell>
1730 <cell alignment="right" valignment="top" usebox="none">
1731 \begin_inset Text
1732
1733 \begin_layout Plain Layout
1734 -40.272
1735 \end_layout
1736
1737 \end_inset
1738 </cell>
1739 <cell alignment="right" valignment="top" usebox="none">
1740 \begin_inset Text
1741
1742 \begin_layout Plain Layout
1743 4
1744 \end_layout
1745
1746 \end_inset
1747 </cell>
1748 </row>
1749 <row>
1750 <cell alignment="center" valignment="top" usebox="none">
1751 \begin_inset Text
1752
1753 \begin_layout Plain Layout
1754  4 
1755 \end_layout
1756
1757 \end_inset
1758 </cell>
1759 <cell alignment="right" valignment="top" usebox="none">
1760 \begin_inset Text
1761
1762 \begin_layout Plain Layout
1763 32733.8 
1764 \end_layout
1765
1766 \end_inset
1767 </cell>
1768 <cell alignment="right" valignment="top" usebox="none">
1769 \begin_inset Text
1770
1771 \begin_layout Plain Layout
1772 -1.2
1773 \begin_inset Flex tablenotemark
1774 status open
1775
1776 \begin_layout Plain Layout
1777 c
1778 \end_layout
1779
1780 \end_inset
1781
1782
1783 \end_layout
1784
1785 \end_inset
1786 </cell>
1787 <cell alignment="right" valignment="top" usebox="none">
1788 \begin_inset Text
1789
1790 \begin_layout Plain Layout
1791 -0.5 
1792 \end_layout
1793
1794 \end_inset
1795 </cell>
1796 <cell alignment="right" valignment="top" usebox="none">
1797 \begin_inset Text
1798
1799 \begin_layout Plain Layout
1800 41 
1801 \end_layout
1802
1803 \end_inset
1804 </cell>
1805 <cell alignment="right" valignment="top" usebox="none">
1806 \begin_inset Text
1807
1808 \begin_layout Plain Layout
1809 54.8 
1810 \end_layout
1811
1812 \end_inset
1813 </cell>
1814 <cell alignment="right" valignment="top" usebox="none">
1815 \begin_inset Text
1816
1817 \begin_layout Plain Layout
1818 2.282 
1819 \end_layout
1820
1821 \end_inset
1822 </cell>
1823 <cell alignment="right" valignment="top" usebox="none">
1824 \begin_inset Text
1825
1826 \begin_layout Plain Layout
1827 2.156 
1828 \end_layout
1829
1830 \end_inset
1831 </cell>
1832 <cell alignment="right" valignment="top" usebox="none">
1833 \begin_inset Text
1834
1835 \begin_layout Plain Layout
1836 4.313 
1837 \end_layout
1838
1839 \end_inset
1840 </cell>
1841 <cell alignment="right" valignment="top" usebox="none">
1842 \begin_inset Text
1843
1844 \begin_layout Plain Layout
1845 117.4 
1846 \end_layout
1847
1848 \end_inset
1849 </cell>
1850 <cell alignment="right" valignment="top" usebox="none">
1851 \begin_inset Text
1852
1853 \begin_layout Plain Layout
1854 78.2 
1855 \end_layout
1856
1857 \end_inset
1858 </cell>
1859 <cell alignment="right" valignment="top" usebox="none">
1860 \begin_inset Text
1861
1862 \begin_layout Plain Layout
1863 -35.847
1864 \end_layout
1865
1866 \end_inset
1867 </cell>
1868 <cell alignment="right" valignment="top" usebox="none">
1869 \begin_inset Text
1870
1871 \begin_layout Plain Layout
1872 5,6
1873 \end_layout
1874
1875 \end_inset
1876 </cell>
1877 </row>
1878 <row>
1879 <cell alignment="center" valignment="top" usebox="none">
1880 \begin_inset Text
1881
1882 \begin_layout Plain Layout
1883  5 
1884 \end_layout
1885
1886 \end_inset
1887 </cell>
1888 <cell alignment="right" valignment="top" usebox="none">
1889 \begin_inset Text
1890
1891 \begin_layout Plain Layout
1892  9607.4 
1893 \end_layout
1894
1895 \end_inset
1896 </cell>
1897 <cell alignment="right" valignment="top" usebox="none">
1898 \begin_inset Text
1899
1900 \begin_layout Plain Layout
1901 -0.4 
1902 \end_layout
1903
1904 \end_inset
1905 </cell>
1906 <cell alignment="right" valignment="top" usebox="none">
1907 \begin_inset Text
1908
1909 \begin_layout Plain Layout
1910 -0.4 
1911 \end_layout
1912
1913 \end_inset
1914 </cell>
1915 <cell alignment="right" valignment="top" usebox="none">
1916 \begin_inset Text
1917
1918 \begin_layout Plain Layout
1919 60 
1920 \end_layout
1921
1922 \end_inset
1923 </cell>
1924 <cell alignment="right" valignment="top" usebox="none">
1925 \begin_inset Text
1926
1927 \begin_layout Plain Layout
1928 1.4 
1929 \end_layout
1930
1931 \end_inset
1932 </cell>
1933 <cell alignment="right" valignment="top" usebox="none">
1934 \begin_inset Text
1935
1936 \begin_layout Plain Layout
1937 1.669
1938 \begin_inset Flex tablenotemark
1939 status collapsed
1940
1941 \begin_layout Plain Layout
1942 c
1943 \end_layout
1944
1945 \end_inset
1946
1947
1948 \end_layout
1949
1950 \end_inset
1951 </cell>
1952 <cell alignment="right" valignment="top" usebox="none">
1953 \begin_inset Text
1954
1955 \begin_layout Plain Layout
1956 1.574 
1957 \end_layout
1958
1959 \end_inset
1960 </cell>
1961 <cell alignment="right" valignment="top" usebox="none">
1962 \begin_inset Text
1963
1964 \begin_layout Plain Layout
1965 2.343 
1966 \end_layout
1967
1968 \end_inset
1969 </cell>
1970 <cell alignment="right" valignment="top" usebox="none">
1971 \begin_inset Text
1972
1973 \begin_layout Plain Layout
1974 8.0 
1975 \end_layout
1976
1977 \end_inset
1978 </cell>
1979 <cell alignment="right" valignment="top" usebox="none">
1980 \begin_inset Text
1981
1982 \begin_layout Plain Layout
1983 8.9 
1984 \end_layout
1985
1986 \end_inset
1987 </cell>
1988 <cell alignment="right" valignment="top" usebox="none">
1989 \begin_inset Text
1990
1991 \begin_layout Plain Layout
1992 -33.417
1993 \end_layout
1994
1995 \end_inset
1996 </cell>
1997 <cell alignment="right" valignment="top" usebox="none">
1998 \begin_inset Text
1999
2000 \begin_layout Plain Layout
2001 7
2002 \end_layout
2003
2004 \end_inset
2005 </cell>
2006 </row>
2007 <row>
2008 <cell alignment="center" valignment="top" usebox="none">
2009 \begin_inset Text
2010
2011 \begin_layout Plain Layout
2012  6 
2013 \end_layout
2014
2015 \end_inset
2016 </cell>
2017 <cell alignment="right" valignment="top" usebox="none">
2018 \begin_inset Text
2019
2020 \begin_layout Plain Layout
2021 31638.6 
2022 \end_layout
2023
2024 \end_inset
2025 </cell>
2026 <cell alignment="right" valignment="top" usebox="none">
2027 \begin_inset Text
2028
2029 \begin_layout Plain Layout
2030 1.6 
2031 \end_layout
2032
2033 \end_inset
2034 </cell>
2035 <cell alignment="right" valignment="top" usebox="none">
2036 \begin_inset Text
2037
2038 \begin_layout Plain Layout
2039 0.1 
2040 \end_layout
2041
2042 \end_inset
2043 </cell>
2044 <cell alignment="right" valignment="top" usebox="none">
2045 \begin_inset Text
2046
2047 \begin_layout Plain Layout
2048 39 
2049 \end_layout
2050
2051 \end_inset
2052 </cell>
2053 <cell alignment="right" valignment="top" usebox="none">
2054 \begin_inset Text
2055
2056 \begin_layout Plain Layout
2057 315.2 
2058 \end_layout
2059
2060 \end_inset
2061 </cell>
2062 <cell alignment="right" valignment="top" usebox="none">
2063 \begin_inset Text
2064
2065 \begin_layout Plain Layout
2066  3.433 
2067 \end_layout
2068
2069 \end_inset
2070 </cell>
2071 <cell alignment="right" valignment="top" usebox="none">
2072 \begin_inset Text
2073
2074 \begin_layout Plain Layout
2075 3.075 
2076 \end_layout
2077
2078 \end_inset
2079 </cell>
2080 <cell alignment="right" valignment="top" usebox="none">
2081 \begin_inset Text
2082
2083 \begin_layout Plain Layout
2084 7.488 
2085 \end_layout
2086
2087 \end_inset
2088 </cell>
2089 <cell alignment="right" valignment="top" usebox="none">
2090 \begin_inset Text
2091
2092 \begin_layout Plain Layout
2093 92.1 
2094 \end_layout
2095
2096 \end_inset
2097 </cell>
2098 <cell alignment="right" valignment="top" usebox="none">
2099 \begin_inset Text
2100
2101 \begin_layout Plain Layout
2102 25.3 
2103 \end_layout
2104
2105 \end_inset
2106 </cell>
2107 <cell alignment="right" valignment="top" usebox="none">
2108 \begin_inset Text
2109
2110 \begin_layout Plain Layout
2111 -12.052 
2112 \end_layout
2113
2114 \end_inset
2115 </cell>
2116 <cell alignment="right" valignment="top" usebox="none">
2117 \begin_inset Text
2118
2119 \begin_layout Plain Layout
2120 8
2121 \end_layout
2122
2123 \end_inset
2124 </cell>
2125 </row>
2126 </lyxtabular>
2127
2128 \end_inset
2129
2130
2131 \end_layout
2132
2133 \begin_layout Table note
2134 a
2135 \begin_inset ERT
2136 status collapsed
2137
2138 \begin_layout Plain Layout
2139
2140 }{
2141 \end_layout
2142
2143 \end_inset
2144
2145 Sample footnote for table
2146 \begin_inset space ~
2147 \end_inset
2148
2149
2150 \begin_inset CommandInset ref
2151 LatexCommand ref
2152 reference "tbl-2"
2153
2154 \end_inset
2155
2156  that was generated with the \SpecialChar LaTeX
2157  table environment
2158 \end_layout
2159
2160 \begin_layout Table note
2161 b
2162 \begin_inset ERT
2163 status collapsed
2164
2165 \begin_layout Plain Layout
2166
2167 }{
2168 \end_layout
2169
2170 \end_inset
2171
2172 Yet another sample footnote for table
2173 \begin_inset space ~
2174 \end_inset
2175
2176
2177 \begin_inset CommandInset ref
2178 LatexCommand ref
2179 reference "tbl-2"
2180
2181 \end_inset
2182
2183
2184 \end_layout
2185
2186 \begin_layout Table note
2187 c
2188 \begin_inset ERT
2189 status collapsed
2190
2191 \begin_layout Plain Layout
2192
2193 }{
2194 \end_layout
2195
2196 \end_inset
2197
2198 Another sample footnote for table
2199 \begin_inset space ~
2200 \end_inset
2201
2202
2203 \begin_inset CommandInset ref
2204 LatexCommand ref
2205 reference "tbl-2"
2206
2207 \end_inset
2208
2209
2210 \end_layout
2211
2212 \begin_layout TableComments
2213 We can also attach a long-ish paragraph of explanatory material to a table.
2214  Use 
2215 \backslash
2216 tablerefs to append a list of references.
2217  The following references were from a different table: I've patched them
2218  in here to show how they look, but don't take them too seriously—I certainly
2219  have not.
2220 \end_layout
2221
2222 \begin_layout TableRefs
2223 (1) Barbuy, Spite, & Spite 1985; (2) Bond 1980; (3) Carbon et al.
2224  1987; (4) Hobbs & Duncan 1987; (5) Gilroy et al.
2225  1988: (6) Gratton & Ortolani 1986; (7) Gratton & Sneden 1987; (8) Gratton
2226  & Sneden (1988); (9) Gratton & Sneden 1991; (10) Kraft et al.
2227  1982; (11) LCL, or Laird, 1990; (12) Leep & Wallerstein 1981; (13) Luck
2228  & Bond 1981; (14) Luck & Bond 1985; (15) Magain 1987; (16) Magain 1989;
2229  (17) Peterson 1981; (18) Peterson, Kurucz, & Carney 1990; (19) RMB; (20)
2230  Schuster & Nissen 1988; (21) Schuster & Nissen 1989b; (22) Spite et al.
2231  1984; (23) Spite & Spite 1986; (24) Hobbs & Thorburn 1991; (25) Hobbs et
2232  al.
2233  1991; (26) Olsen 1983.
2234 \end_layout
2235
2236 \end_inset
2237
2238
2239 \end_layout
2240
2241 \begin_layout Standard
2242 \begin_inset Note Note
2243 status open
2244
2245 \begin_layout Plain Layout
2246 LyX can load deluxetable files verbatim.
2247  To see this in action, dissolve the following Note and copy the file table.tex
2248  from the AASTeX 5.0 distribution into the same directory as this file.
2249 \end_layout
2250
2251 \end_inset
2252
2253
2254 \end_layout
2255
2256 \begin_layout Standard
2257 \begin_inset Note Note
2258 status open
2259
2260 \begin_layout Plain Layout
2261 \begin_inset CommandInset include
2262 LatexCommand input
2263 filename "table"
2264 literal "true"
2265
2266 \end_inset
2267
2268
2269 \end_layout
2270
2271 \end_inset
2272
2273
2274 \end_layout
2275
2276 \end_body
2277 \end_document