lib/examples/aas_sample.lyx

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   7 \newcommand{\vdag}{(v)^\dagger}
   8 \newcommand{\myemail}{skywalker@galaxy.far.far.away}
   9 \slugcomment{Not to appear in Nonlearned J., 45.}
  10 \shorttitle{Djorgovski et al.}
  11 \shortauthors{Collapsed Cores in Globular Clusters}
  12 \end_preamble
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  66 \end_header
  67
  68 \begin_body
  69
  70 \begin_layout Title
  71 Collapsed Cores in Globular Clusters,  Gauge-Boson Couplings, and AASTeX
  72  Examples
  73 \end_layout
  74
  75 \begin_layout Author
  76 S.
  77  Djorgovski
  78 \begin_inset Flex altaffilmark
  79 status open
  80
  81 \begin_layout Plain Layout
  82 1,2,3
  83 \end_layout
  84
  85 \end_inset
  86
  87  and Ivan R.
  88  King
  89 \begin_inset Flex altaffilmark
  90 status collapsed
  91
  92 \begin_layout Plain Layout
  93 1
  94 \end_layout
  95
  96 \end_inset
  97
  98
  99 \end_layout
 100
 101 \begin_layout Affiliation
 102 Astronomy Department, University of California, Berkeley, CA 94720
 103 \end_layout
 104
 105 \begin_layout Author
 106 C.
 107  D.
 108  Biemesderfer
 109 \begin_inset Flex altaffilmark
 110 status collapsed
 111
 112 \begin_layout Plain Layout
 113 4,5
 114 \end_layout
 115
 116 \end_inset
 117
 118
 119 \end_layout
 120
 121 \begin_layout Affiliation
 122 National Optical Astronomy Observatories, Tucson, AZ 85719
 123 \end_layout
 124
 125 \begin_layout Email
 126 aastex-help@aas.org
 127 \end_layout
 128
 129 \begin_layout And
 130
 131 \end_layout
 132
 133 \begin_layout Author
 134 R.
 135  J.
 136  Hanisch
 137 \begin_inset Flex altaffilmark
 138 status collapsed
 139
 140 \begin_layout Plain Layout
 141 5
 142 \end_layout
 143
 144 \end_inset
 145
 146
 147 \end_layout
 148
 149 \begin_layout Affiliation
 150 Space Telescope Science Institute, Baltimore, MD 21218
 151 \end_layout
 152
 153 \begin_layout Altaffilation
 154 1
 155 \begin_inset ERT
 156 status collapsed
 157
 158 \begin_layout Plain Layout
 159
 160 }{
 161 \end_layout
 162
 163 \end_inset
 164
 165 Visiting Astronomer, Cerro Tololo Inter-American Observatory.
 166  CTIO is operated by AURA, Inc.
 167 \begin_inset space \space{}
 168 \end_inset
 169
 170 under contract to the National Science Foundation.
 171 \end_layout
 172
 173 \begin_layout Altaffilation
 174 2
 175 \begin_inset ERT
 176 status collapsed
 177
 178 \begin_layout Plain Layout
 179
 180 }{
 181 \end_layout
 182
 183 \end_inset
 184
 185 Society of Fellows, Harvard University.
 186 \end_layout
 187
 188 \begin_layout Altaffilation
 189 3
 190 \begin_inset ERT
 191 status collapsed
 192
 193 \begin_layout Plain Layout
 194
 195 }{
 196 \end_layout
 197
 198 \end_inset
 199
 200 present address: Center for Astrophysics, 60 Garden Street, Cambridge, MA
 201  02138
 202 \end_layout
 203
 204 \begin_layout Altaffilation
 205 4
 206 \begin_inset ERT
 207 status collapsed
 208
 209 \begin_layout Plain Layout
 210
 211 }{
 212 \end_layout
 213
 214 \end_inset
 215
 216 Visiting Programmer, Space Telescope Science Institute
 217 \end_layout
 218
 219 \begin_layout Altaffilation
 220 5
 221 \begin_inset ERT
 222 status collapsed
 223
 224 \begin_layout Plain Layout
 225
 226 }{
 227 \end_layout
 228
 229 \end_inset
 230
 231 Patron, Alonso's Bar and Grill
 232 \end_layout
 233
 234 \begin_layout Abstract
 235 This is a preliminary report on surface photometry of the major fraction
 236  of known globular clusters, to see which of them show the signs of a collapsed
 237  core.
 238  We also explore some diversionary mathematics and recreational tables.
 239
 240 \end_layout
 241
 242 \begin_layout Keywords
 243 clusters: globular, peanut---bosons: bozos
 244 \end_layout
 245
 246 \begin_layout Section
 247 Introduction
 248 \end_layout
 249
 250 \begin_layout Standard
 251 A focal problem today in the dynamics of globular clusters is core collapse.
 252  It has been predicted by theory for decades
 253 \begin_inset ERT
 254 status collapsed
 255
 256 \begin_layout Plain Layout
 257
 258
 259 \backslash
 260 citep{hen61,lyn68,spi85}
 261 \end_layout
 262
 263 \end_inset
 264
 265 , but observation has been less alert to the phenomenon.
 266  For many years the central brightness peak in M15
 267 \begin_inset ERT
 268 status collapsed
 269
 270 \begin_layout Plain Layout
 271
 272
 273 \backslash
 274 citep{kin75,new78}
 275 \end_layout
 276
 277 \end_inset
 278
 279  seemed a unique anomaly.
 280  Then
 281 \begin_inset ERT
 282 status collapsed
 283
 284 \begin_layout Plain Layout
 285
 286
 287 \backslash
 288 citet{aur82}
 289 \end_layout
 290
 291 \end_inset
 292
 293  suggested a central peak in NGC 6397, and a limited photographic survey
 294  of ours
 295 \begin_inset ERT
 296 status collapsed
 297
 298 \begin_layout Plain Layout
 299
 300
 301 \backslash
 302 citep[Paper I]{djo84}
 303 \end_layout
 304
 305 \end_inset
 306
 307  found three more cases, including NGC 6624, whose sharp center had often
 308  been remarked on
 309 \begin_inset ERT
 310 status collapsed
 311
 312 \begin_layout Plain Layout
 313
 314
 315 \backslash
 316 citep{can78}
 317 \end_layout
 318
 319 \end_inset
 320
 321 .
 322
 323 \end_layout
 324
 325 \begin_layout Section
 326 Observations
 327 \end_layout
 328
 329 \begin_layout Standard
 330 All our observations were short direct exposures with CCD's.
 331  At Lick Observatory we used a TI 500
 332 \begin_inset Formula $\times$
 333 \end_inset
 334
 335 500 chip and a GEC 575
 336 \begin_inset Formula $\times$
 337 \end_inset
 338
 339 385, on the 1-m Nickel reflector.
 340  The only filter available at Lick was red.
 341  At CTIO we used a GEC 575
 342 \begin_inset Formula $\times$
 343 \end_inset
 344
 345 385, with
 346 \begin_inset Formula $B,V,$
 347 \end_inset
 348
 349  and
 350 \begin_inset Formula $R$
 351 \end_inset
 352
 353  filters, and an RCA 512
 354 \begin_inset Formula $\times$
 355 \end_inset
 356
 357 320, with
 358 \begin_inset Formula $U,B,V,R,$
 359 \end_inset
 360
 361  and
 362 \begin_inset Formula $I$
 363 \end_inset
 364
 365  filters, on the 1.5-m reflector.
 366  In the CTIO observations we tried to concentrate on the shortest practicable
 367  wavelengths; but faintness, reddening, and poor short-wavelength sensitivity
 368  often kept us from observing in
 369 \begin_inset Formula $U$
 370 \end_inset
 371
 372  or even in
 373 \begin_inset Formula $B$
 374 \end_inset
 375
 376 .
 377  All four cameras had scales of the order of 0.4 arcsec/pixel, and our field
 378  sizes were around 3 arcmin.
 379 \end_layout
 380
 381 \begin_layout Standard
 382 The CCD images are unfortunately not always suitable, for very poor clusters
 383  or for clusters with large cores.
 384  Since the latter are easily studied by other means, we augmented our own
 385  CCD profiles by collecting from the literature a number of star-count profiles
 386
 387 \begin_inset ERT
 388 status collapsed
 389
 390 \begin_layout Plain Layout
 391
 392
 393 \backslash
 394 citep{kin68,pet76,har84,ort85}
 395 \end_layout
 396
 397 \end_inset
 398
 399 , as well as photoelectric profiles
 400 \begin_inset ERT
 401 status collapsed
 402
 403 \begin_layout Plain Layout
 404
 405
 406 \backslash
 407 citep{kin66,kin75}
 408 \end_layout
 409
 410 \end_inset
 411
 412  and electronographic profiles
 413 \begin_inset ERT
 414 status collapsed
 415
 416 \begin_layout Plain Layout
 417
 418
 419 \backslash
 420 citep{kro84}
 421 \end_layout
 422
 423 \end_inset
 424
 425 .
 426  In a few cases we judged normality by eye estimates on one of the Sky Surveys.
 427 \end_layout
 428
 429 \begin_layout Section
 430 Helicity Amplitudes
 431 \end_layout
 432
 433 \begin_layout Standard
 434 It has been realized that helicity amplitudes provide a convenient means
 435  for Feynman diagram
 436 \begin_inset Foot
 437 status collapsed
 438
 439 \begin_layout Plain Layout
 440 Footnotes can be inserted like this.
 441 \end_layout
 442
 443 \end_inset
 444
 445  evaluations.
 446  These amplitude-level techniques are particularly convenient for calculations
 447  involving many Feynman diagrams, where the usual trace techniques for the
 448  amplitude squared becomes unwieldy.
 449  Our calculations use the helicity techniques developed by other authors
 450
 451 \begin_inset CommandInset citation
 452 LatexCommand cite
 453 key "hag86"
 454
 455 \end_inset
 456
 457 ; we briefly summarize below.
 458 \end_layout
 459
 460 \begin_layout Subsection
 461 Formalism
 462 \end_layout
 463
 464 \begin_layout Standard
 465 \begin_inset CommandInset label
 466 LatexCommand label
 467 name "bozomath"
 468
 469 \end_inset
 470
 471
 472 \end_layout
 473
 474 \begin_layout Standard
 475 A tree-level amplitude in
 476 \begin_inset Formula $e^{+}e^{-}$
 477 \end_inset
 478
 479  collisions can be expressed in terms of fermion strings of the form
 480 \begin_inset Formula
 481 \begin{equation}
 482 \bar{v}(p_{2},\sigma_{2})P_{-\tau}\hat{a}_{1}\hat{a}_{2}\cdots\hat{a}_{n}u(p_{1},\sigma_{1}),
 483 \end{equation}
 484
 485 \end_inset
 486
 487  where
 488 \begin_inset Formula $p$
 489 \end_inset
 490
 491  and
 492 \begin_inset Formula $\sigma$
 493 \end_inset
 494
 495  label the initial
 496 \begin_inset Formula $e^{\pm}$
 497 \end_inset
 498
 499  four-momenta and helicities
 500 \begin_inset Formula $(\sigma=\pm1)$
 501 \end_inset
 502
 503 ,
 504 \begin_inset Formula $\hat{a}_{i}=a_{i}^{\mu}\gamma_{\nu}$
 505 \end_inset
 506
 507  and
 508 \begin_inset Formula $P_{\tau}=\frac{1}{2}(1+\tau\gamma_{5})$
 509 \end_inset
 510
 511  is a chirality projection operator
 512 \begin_inset Formula $(\tau=\pm1)$
 513 \end_inset
 514
 515 .
 516  The
 517 \begin_inset Formula $a_{i}^{\mu}$
 518 \end_inset
 519
 520  may be formed from particle four-momenta, gauge-boson polarization vectors
 521  or fermion strings with an uncontracted Lorentz index associated with final-sta
 522 te fermions.
 523 \end_layout
 524
 525 \begin_layout NoteToEditor
 526 Figures 1 and 2 should appear side-by-side in print
 527 \end_layout
 528
 529 \begin_layout Standard
 530 In the chiral representation the
 531 \begin_inset Formula $\gamma$
 532 \end_inset
 533
 534  matrices are expressed in terms of
 535 \begin_inset Formula $2\times2$
 536 \end_inset
 537
 538  Pauli matrices
 539 \begin_inset Formula $\sigma$
 540 \end_inset
 541
 542  and the unit matrix 1 as
 543 \begin_inset Formula
 544 \begin{eqnarray*}
 545 \gamma^{\mu} & = & \left(\begin{array}{cc}
 546 0 & \sigma_{+}^{\mu}\\
 547 \sigma_{-}^{\mu} & 0
 548 \end{array}\right),\gamma^{5}=\left(\begin{array}{cc}
 549 -1 & 0\\
 550 0 & 1
 551 \end{array}\right),\\
 552 \sigma_{\pm}^{\mu} & = & ({\textbf{1}},\pm\sigma),
 553 \end{eqnarray*}
 554
 555 \end_inset
 556
 557  giving
 558 \begin_inset Formula
 559 \begin{equation}
 560 \hat{a}=\left(\begin{array}{cc}
 561 0 & (\hat{a})_{+}\\
 562 (\hat{a})_{-} & 0
 563 \end{array}\right),(\hat{a})_{\pm}=a_{\mu}\sigma_{\pm}^{\mu},
 564 \end{equation}
 565
 566 \end_inset
 567
 568  The spinors are expressed in terms of two-component Weyl spinors as
 569 \begin_inset Formula
 570 \begin{equation}
 571 u=\left(\begin{array}{c}
 572 (u)_{-}\\
 573 (u)_{+}
 574 \end{array}\right),v={\textbf{(}}\vdag_{+}{\textbf{,}}\vdag_{-}{\textbf{)}}.
 575 \end{equation}
 576
 577 \end_inset
 578
 579
 580 \end_layout
 581
 582 \begin_layout Standard
 583 The Weyl spinors are given in terms of helicity eigenstates
 584 \begin_inset Formula $\chi_{\lambda}(p)$
 585 \end_inset
 586
 587  with
 588 \begin_inset Formula $\lambda=\pm1$
 589 \end_inset
 590
 591  by
 592 \end_layout
 593
 594 \begin_layout MathLetters
 595 \begin_inset Formula
 596 \begin{eqnarray}
 597 u(p,\lambda)_{\pm} & = & (E\pm\lambda|{\textbf{p}}|)^{1/2}\chi_{\lambda}(p),\\
 598 v(p,\lambda)_{\pm} & = & \pm\lambda(E\mp\lambda|{\textbf{p}}|)^{1/2}\chi_{-\lambda}(p)
 599 \end{eqnarray}
 600
 601 \end_inset
 602
 603
 604 \end_layout
 605
 606 \begin_layout Section
 607 Floating material and so forth
 608 \end_layout
 609
 610 \begin_layout Standard
 611 Consider a task that computes profile parameters for a modified Lorentzian
 612  of the form
 613 \begin_inset Formula
 614 \begin{equation}
 615 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
 616 \end{equation}
 617
 618 \end_inset
 619
 620  where
 621 \begin_inset Formula
 622 \[
 623 d_{1}=\sqrt{\left(\begin{array}{c}
 624 \frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 625 \frac{y_{1}}{R_{min}}\end{array}\right)^{2}}
 626 \]
 627
 628 \end_inset
 629
 630
 631 \begin_inset Formula
 632 \[
 633 d_{2}=\sqrt{\left(\begin{array}{c}
 634 \frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 635 \case{y_{1}}{PR_{min}}\end{array}\right)^{2}}
 636 \]
 637
 638 \end_inset
 639
 640
 641 \begin_inset Formula
 642 \[
 643 x_{1}=(x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta
 644 \]
 645
 646 \end_inset
 647
 648
 649 \begin_inset Formula
 650 \[
 651 y_{1}=-(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta
 652 \]
 653
 654 \end_inset
 655
 656
 657 \end_layout
 658
 659 \begin_layout Standard
 660 In these expressions
 661 \begin_inset Formula $x_{0}$
 662 \end_inset
 663
 664 ,
 665 \begin_inset Formula $y_{0}$
 666 \end_inset
 667
 668  is the star center, and
 669 \begin_inset Formula $\Theta$
 670 \end_inset
 671
 672  is the angle with the
 673 \begin_inset Formula $x$
 674 \end_inset
 675
 676  axis.
 677  Results of this task are shown in table
 678 \begin_inset space ~
 679 \end_inset
 680
 681
 682 \begin_inset CommandInset ref
 683 LatexCommand ref
 684 reference "tbl-2"
 685
 686 \end_inset
 687
 688 .
 689  It is not clear how these sorts of analyses may affect determination of
 690
 691 \begin_inset Formula $M_{\sun}$
 692 \end_inset
 693
 694 , but the assumption is that the alternate results should be less than 90°
 695  out of phase with previous values.
 696  We have no observations of
 697 \begin_inset ERT
 698 status collapsed
 699
 700 \begin_layout Plain Layout
 701
 702
 703 \backslash
 704 ion{Ca}{2}
 705 \end_layout
 706
 707 \end_inset
 708
 709 .
 710  Roughly
 711 \begin_inset ERT
 712 status collapsed
 713
 714 \begin_layout Plain Layout
 715
 716
 717 \backslash
 718 slantfrac{4}{5}
 719 \end_layout
 720
 721 \end_inset
 722
 723  of the electronically submitted abstracts for AAS meetings are error-free.
 724 \end_layout
 725
 726 \begin_layout Acknowledgements
 727
 728 \end_layout
 729
 730 \begin_layout Standard
 731 We are grateful to V.
 732  Barger, T.
 733  Han, and R.
 734  J.
 735  N.
 736  Phillips for doing the math in section
 737 \begin_inset space ~
 738 \end_inset
 739
 740
 741 \begin_inset CommandInset ref
 742 LatexCommand ref
 743 reference "bozomath"
 744
 745 \end_inset
 746
 747 .
 748  More information on the AASTeX macros package are available at
 749 \begin_inset Flex URL
 750 status collapsed
 751
 752 \begin_layout Plain Layout
 753
 754 http://www.aas.org/publications/aastex
 755 \end_layout
 756
 757 \end_inset
 758
 759  or the
 760 \begin_inset ERT
 761 status collapsed
 762
 763 \begin_layout Plain Layout
 764
 765
 766 \backslash
 767 anchor{ftp://www.aas.org/pubs/}{AAS ftp site}
 768 \end_layout
 769
 770 \end_inset
 771
 772 .
 773 \end_layout
 774
 775 \begin_layout Appendix
 776
 777 \end_layout
 778
 779 \begin_layout Section
 780 Appendicial material
 781 \end_layout
 782
 783 \begin_layout Standard
 784 Consider once again a task that computes profile parameters for a modified
 785  Lorentzian of the form
 786 \begin_inset Formula
 787 \begin{equation}
 788 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
 789 \end{equation}
 790
 791 \end_inset
 792
 793  where
 794 \end_layout
 795
 796 \begin_layout MathLetters
 797 \begin_inset Formula
 798 \[
 799 d_{1}=\frac{3}{4}\sqrt{\left(\begin{array}{c}
 800 \frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 801 \frac{y_{1}}{R_{min}}\end{array}\right)^{2}}
 802 \]
 803
 804 \end_inset
 805
 806
 807 \begin_inset Formula
 808 \begin{equation}
 809 d_{2}=\case{3}{4}\sqrt{\left(\begin{array}{c}
 810 \frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 811 \case{y_{1}}{PR_{min}}\end{array}\right)^{2}}
 812 \end{equation}
 813
 814 \end_inset
 815
 816
 817 \begin_inset Formula
 818 \begin{eqnarray}
 819 x_{1} & = & (x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta\\
 820 y_{1} & = & -(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta
 821 \end{eqnarray}
 822
 823 \end_inset
 824
 825
 826 \end_layout
 827
 828 \begin_layout Standard
 829 For completeness, here is one last equation.
 830
 831 \begin_inset Formula
 832 \begin{equation}
 833 e=mc^{2}
 834 \end{equation}
 835
 836 \end_inset
 837
 838
 839 \end_layout
 840
 841 \begin_layout References
 842 \labelwidthstring References
 843 \begin_inset CommandInset bibitem
 844 LatexCommand bibitem
 845 label "Auri\\`ere(1982)"
 846 key "aur82"
 847
 848 \end_inset
 849
 850 Aurière, M.
 851  1982,
 852 \begin_inset ERT
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1013 King, I.
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1038
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1042
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1064
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1066
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1068 \backslash
1069 pasp
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1071
1072 \end_inset
1073
1074 , 96, 198
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1086 Lynden-Bell, D., and Wood, R.
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1092
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1094 \backslash
1095 mnras
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1097
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1102
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1120
1121
1122 \backslash
1123 apjs
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1125
1126 \end_inset
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1128 , 37, 27
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1140 Ortolani, S., Rosino, L., and Sandage, A.
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1142 \begin_inset ERT
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1146
1147
1148 \backslash
1149 aj
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1151
1152 \end_inset
1153
1154 , 90, 473
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1164 \end_inset
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1166 Peterson, C.
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1175 \backslash
1176 aj
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1178
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1181 , 81, 617
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1742
1743 \end_inset
1744 </cell>
1745 <cell alignment="right" valignment="top" usebox="none">
1746 \begin_inset Text
1747
1748 \begin_layout Plain Layout
1749 0.9
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1751
1752 \end_inset
1753 </cell>
1754 <cell alignment="right" valignment="top" usebox="none">
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1756
1757 \begin_layout Plain Layout
1758 0.3
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1760
1761 \end_inset
1762 </cell>
1763 <cell alignment="right" valignment="top" usebox="none">
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1765
1766 \begin_layout Plain Layout
1767 60
1768 \end_layout
1769
1770 \end_inset
1771 </cell>
1772 <cell alignment="right" valignment="top" usebox="none">
1773 \begin_inset Text
1774
1775 \begin_layout Plain Layout
1776 3.4
1777 \end_layout
1778
1779 \end_inset
1780 </cell>
1781 <cell alignment="right" valignment="top" usebox="none">
1782 \begin_inset Text
1783
1784 \begin_layout Plain Layout
1785 1.622
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1787
1788 \end_inset
1789 </cell>
1790 <cell alignment="right" valignment="top" usebox="none">
1791 \begin_inset Text
1792
1793 \begin_layout Plain Layout
1794 1.551
1795 \end_layout
1796
1797 \end_inset
1798 </cell>
1799 <cell alignment="right" valignment="top" usebox="none">
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1801
1802 \begin_layout Plain Layout
1803 2.159
1804 \end_layout
1805
1806 \end_inset
1807 </cell>
1808 <cell alignment="right" valignment="top" usebox="none">
1809 \begin_inset Text
1810
1811 \begin_layout Plain Layout
1812 6.7
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1814
1815 \end_inset
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1819
1820 \begin_layout Plain Layout
1821 7.3
1822 \end_layout
1823
1824 \end_inset
1825 </cell>
1826 <cell alignment="right" valignment="top" usebox="none">
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1828
1829 \begin_layout Plain Layout
1830 -40.272
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1832
1833 \end_inset
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1837
1838 \begin_layout Plain Layout
1839 4
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1841
1842 \end_inset
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1849 \begin_layout Plain Layout
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1852
1853 \end_inset
1854 </cell>
1855 <cell alignment="right" valignment="top" usebox="none">
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1857
1858 \begin_layout Plain Layout
1859 32733.8
1860 \end_layout
1861
1862 \end_inset
1863 </cell>
1864 <cell alignment="right" valignment="top" usebox="none">
1865 \begin_inset Text
1866
1867 \begin_layout Plain Layout
1868 -1.2
1869 \begin_inset Flex tablenotemark
1870 status open
1871
1872 \begin_layout Plain Layout
1873 c
1874 \end_layout
1875
1876 \end_inset
1877
1878
1879 \end_layout
1880
1881 \end_inset
1882 </cell>
1883 <cell alignment="right" valignment="top" usebox="none">
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1885
1886 \begin_layout Plain Layout
1887 -0.5
1888 \end_layout
1889
1890 \end_inset
1891 </cell>
1892 <cell alignment="right" valignment="top" usebox="none">
1893 \begin_inset Text
1894
1895 \begin_layout Plain Layout
1896 41
1897 \end_layout
1898
1899 \end_inset
1900 </cell>
1901 <cell alignment="right" valignment="top" usebox="none">
1902 \begin_inset Text
1903
1904 \begin_layout Plain Layout
1905 54.8
1906 \end_layout
1907
1908 \end_inset
1909 </cell>
1910 <cell alignment="right" valignment="top" usebox="none">
1911 \begin_inset Text
1912
1913 \begin_layout Plain Layout
1914 2.282
1915 \end_layout
1916
1917 \end_inset
1918 </cell>
1919 <cell alignment="right" valignment="top" usebox="none">
1920 \begin_inset Text
1921
1922 \begin_layout Plain Layout
1923 2.156
1924 \end_layout
1925
1926 \end_inset
1927 </cell>
1928 <cell alignment="right" valignment="top" usebox="none">
1929 \begin_inset Text
1930
1931 \begin_layout Plain Layout
1932 4.313
1933 \end_layout
1934
1935 \end_inset
1936 </cell>
1937 <cell alignment="right" valignment="top" usebox="none">
1938 \begin_inset Text
1939
1940 \begin_layout Plain Layout
1941 117.4
1942 \end_layout
1943
1944 \end_inset
1945 </cell>
1946 <cell alignment="right" valignment="top" usebox="none">
1947 \begin_inset Text
1948
1949 \begin_layout Plain Layout
1950 78.2
1951 \end_layout
1952
1953 \end_inset
1954 </cell>
1955 <cell alignment="right" valignment="top" usebox="none">
1956 \begin_inset Text
1957
1958 \begin_layout Plain Layout
1959 -35.847
1960 \end_layout
1961
1962 \end_inset
1963 </cell>
1964 <cell alignment="right" valignment="top" usebox="none">
1965 \begin_inset Text
1966
1967 \begin_layout Plain Layout
1968 5,6
1969 \end_layout
1970
1971 \end_inset
1972 </cell>
1973 </row>
1974 <row>
1975 <cell alignment="center" valignment="top" usebox="none">
1976 \begin_inset Text
1977
1978 \begin_layout Plain Layout
1979  5
1980 \end_layout
1981
1982 \end_inset
1983 </cell>
1984 <cell alignment="right" valignment="top" usebox="none">
1985 \begin_inset Text
1986
1987 \begin_layout Plain Layout
1988  9607.4
1989 \end_layout
1990
1991 \end_inset
1992 </cell>
1993 <cell alignment="right" valignment="top" usebox="none">
1994 \begin_inset Text
1995
1996 \begin_layout Plain Layout
1997 -0.4
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1999
2000 \end_inset
2001 </cell>
2002 <cell alignment="right" valignment="top" usebox="none">
2003 \begin_inset Text
2004
2005 \begin_layout Plain Layout
2006 -0.4
2007 \end_layout
2008
2009 \end_inset
2010 </cell>
2011 <cell alignment="right" valignment="top" usebox="none">
2012 \begin_inset Text
2013
2014 \begin_layout Plain Layout
2015 60
2016 \end_layout
2017
2018 \end_inset
2019 </cell>
2020 <cell alignment="right" valignment="top" usebox="none">
2021 \begin_inset Text
2022
2023 \begin_layout Plain Layout
2024 1.4
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2026
2027 \end_inset
2028 </cell>
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2031
2032 \begin_layout Plain Layout
2033 1.669
2034 \begin_inset Flex tablenotemark
2035 status collapsed
2036
2037 \begin_layout Plain Layout
2038 c
2039 \end_layout
2040
2041 \end_inset
2042
2043
2044 \end_layout
2045
2046 \end_inset
2047 </cell>
2048 <cell alignment="right" valignment="top" usebox="none">
2049 \begin_inset Text
2050
2051 \begin_layout Plain Layout
2052 1.574
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2054
2055 \end_inset
2056 </cell>
2057 <cell alignment="right" valignment="top" usebox="none">
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2060 \begin_layout Plain Layout
2061 2.343
2062 \end_layout
2063
2064 \end_inset
2065 </cell>
2066 <cell alignment="right" valignment="top" usebox="none">
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2068
2069 \begin_layout Plain Layout
2070 8.0
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2072
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2074 </cell>
2075 <cell alignment="right" valignment="top" usebox="none">
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2079 8.9
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2081
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2086
2087 \begin_layout Plain Layout
2088 -33.417
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2095
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2097 7
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2100 \end_inset
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2103 <row>
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2116 \begin_layout Plain Layout
2117 31638.6
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2119
2120 \end_inset
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2125 \begin_layout Plain Layout
2126 1.6
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2128
2129 \end_inset
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2132 \begin_inset Text
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2134 \begin_layout Plain Layout
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2137
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2142
2143 \begin_layout Plain Layout
2144 39
2145 \end_layout
2146
2147 \end_inset
2148 </cell>
2149 <cell alignment="right" valignment="top" usebox="none">
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2151
2152 \begin_layout Plain Layout
2153 315.2
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2155
2156 \end_inset
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2158 <cell alignment="right" valignment="top" usebox="none">
2159 \begin_inset Text
2160
2161 \begin_layout Plain Layout
2162  3.433
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2164
2165 \end_inset
2166 </cell>
2167 <cell alignment="right" valignment="top" usebox="none">
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2169
2170 \begin_layout Plain Layout
2171 3.075
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2173
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2178
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2182
2183 \end_inset
2184 </cell>
2185 <cell alignment="right" valignment="top" usebox="none">
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2188 \begin_layout Plain Layout
2189 92.1
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2191
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2193 </cell>
2194 <cell alignment="right" valignment="top" usebox="none">
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2198 25.3
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2200
2201 \end_inset
2202 </cell>
2203 <cell alignment="right" valignment="top" usebox="none">
2204 \begin_inset Text
2205
2206 \begin_layout Plain Layout
2207 -12.052
2208 \end_layout
2209
2210 \end_inset
2211 </cell>
2212 <cell alignment="right" valignment="top" usebox="none">
2213 \begin_inset Text
2214
2215 \begin_layout Plain Layout
2216 8
2217 \end_layout
2218
2219 \end_inset
2220 </cell>
2221 </row>
2222 </lyxtabular>
2223
2224 \end_inset
2225
2226
2227 \end_layout
2228
2229 \begin_layout Table note
2230 a
2231 \begin_inset ERT
2232 status collapsed
2233
2234 \begin_layout Plain Layout
2235
2236 }{
2237 \end_layout
2238
2239 \end_inset
2240
2241 Sample footnote for table
2242 \begin_inset space ~
2243 \end_inset
2244
2245
2246 \begin_inset CommandInset ref
2247 LatexCommand ref
2248 reference "tbl-2"
2249
2250 \end_inset
2251
2252  that was generated with the LaTeX table environment
2253 \end_layout
2254
2255 \begin_layout Table note
2256 b
2257 \begin_inset ERT
2258 status collapsed
2259
2260 \begin_layout Plain Layout
2261
2262 }{
2263 \end_layout
2264
2265 \end_inset
2266
2267 Yet another sample footnote for table
2268 \begin_inset space ~
2269 \end_inset
2270
2271
2272 \begin_inset CommandInset ref
2273 LatexCommand ref
2274 reference "tbl-2"
2275
2276 \end_inset
2277
2278
2279 \end_layout
2280
2281 \begin_layout Table note
2282 c
2283 \begin_inset ERT
2284 status collapsed
2285
2286 \begin_layout Plain Layout
2287
2288 }{
2289 \end_layout
2290
2291 \end_inset
2292
2293 Another sample footnote for table
2294 \begin_inset space ~
2295 \end_inset
2296
2297
2298 \begin_inset CommandInset ref
2299 LatexCommand ref
2300 reference "tbl-2"
2301
2302 \end_inset
2303
2304
2305 \end_layout
2306
2307 \begin_layout TableComments
2308 We can also attach a long-ish paragraph of explanatory material to a table.
2309  Use
2310 \backslash
2311 tablerefs to append a list of references.
2312  The following references were from a different table: I've patched them
2313  in here to show how they look, but don't take them too seriously---I certainly
2314  have not.
2315 \end_layout
2316
2317 \begin_layout TableRefs
2318 (1) Barbuy, Spite, & Spite 1985; (2) Bond 1980; (3) Carbon et al.
2319  1987; (4) Hobbs & Duncan 1987; (5) Gilroy et al.
2320  1988: (6) Gratton & Ortolani 1986; (7) Gratton & Sneden 1987; (8) Gratton
2321  & Sneden (1988); (9) Gratton & Sneden 1991; (10) Kraft et al.
2322  1982; (11) LCL, or Laird, 1990; (12) Leep & Wallerstein 1981; (13) Luck
2323  & Bond 1981; (14) Luck & Bond 1985; (15) Magain 1987; (16) Magain 1989;
2324  (17) Peterson 1981; (18) Peterson, Kurucz, & Carney 1990; (19) RMB; (20)
2325  Schuster & Nissen 1988; (21) Schuster & Nissen 1989b; (22) Spite et al.
2326  1984; (23) Spite & Spite 1986; (24) Hobbs & Thorburn 1991; (25) Hobbs et
2327  al.
2328  1991; (26) Olsen 1983.
2329 \end_layout
2330
2331 \end_inset
2332
2333
2334 \end_layout
2335
2336 \begin_layout Standard
2337 \begin_inset ERT
2338 status collapsed
2339
2340 \begin_layout Plain Layout
2341
2342 % LyX can load deluxetable files verbatim.
2343  To see this in action, uncomment the following
2344 \end_layout
2345
2346 \end_inset
2347
2348
2349 \end_layout
2350
2351 \begin_layout Standard
2352 \begin_inset ERT
2353 status collapsed
2354
2355 \begin_layout Plain Layout
2356
2357 % line (delete the
2358 \end_layout
2359
2360 \end_inset
2361
2362
2363 \begin_inset Quotes eld
2364 \end_inset
2365
2366
2367 \begin_inset ERT
2368 status collapsed
2369
2370 \begin_layout Plain Layout
2371
2372 %
2373 \end_layout
2374
2375 \end_inset
2376
2377
2378 \begin_inset Quotes erd
2379 \end_inset
2380
2381
2382 \begin_inset ERT
2383 status collapsed
2384
2385 \begin_layout Plain Layout
2386
2387 ) and copy the file table.tex from the AASTeX 5.0 distribution into
2388 \end_layout
2389
2390 \end_inset
2391
2392
2393 \end_layout
2394
2395 \begin_layout Standard
2396 \begin_inset ERT
2397 status collapsed
2398
2399 \begin_layout Plain Layout
2400
2401 % the same directory as this file.
2402 \end_layout
2403
2404 \end_inset
2405
2406
2407 \end_layout
2408
2409 \begin_layout Standard
2410 \begin_inset ERT
2411 status collapsed
2412
2413 \begin_layout Plain Layout
2414
2415 %
2416 \end_layout
2417
2418 \end_inset
2419
2420
2421 \begin_inset CommandInset include
2422 LatexCommand input
2423 filename "table"
2424
2425 \end_inset
2426
2427
2428 \end_layout
2429
2430 \end_body
2431 \end_document