lib/examples/aas_sample.lyx

   1 #LyX 1.6.0svn created this file. For more info see http://www.lyx.org/
   2 \lyxformat 341
   3 \begin_document
   4 \begin_header
   5 \textclass aastex
   6 \begin_preamble
   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
  13 \language english
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  43 \tracking_changes false
  44 \output_changes false
  45 \author ""
  46 \end_header
  47
  48 \begin_body
  49
  50 \begin_layout Title
  51 Collapsed Cores in Globular Clusters,  Gauge-Boson Couplings, and AASTeX
  52  Examples
  53 \end_layout
  54
  55 \begin_layout Author
  56 S.
  57  Djorgovski
  58 \begin_inset ERT
  59 status collapsed
  60
  61 \begin_layout Plain Layout
  62
  63
  64 \backslash
  65 altaffilmark{1,2,3}
  66 \end_layout
  67
  68 \end_inset
  69
  70  and Ivan R.
  71  King
  72 \begin_inset ERT
  73 status collapsed
  74
  75 \begin_layout Plain Layout
  76
  77
  78 \backslash
  79 altaffilmark{1}
  80 \end_layout
  81
  82 \end_inset
  83
  84
  85 \end_layout
  86
  87 \begin_layout Affiliation
  88 Astronomy Department, University of California, Berkeley, CA 94720
  89 \end_layout
  90
  91 \begin_layout Author
  92 C.
  93  D.
  94  Biemesderfer
  95 \begin_inset ERT
  96 status collapsed
  97
  98 \begin_layout Plain Layout
  99
 100
 101 \backslash
 102 altaffilmark{4,5}
 103 \end_layout
 104
 105 \end_inset
 106
 107
 108 \end_layout
 109
 110 \begin_layout Affiliation
 111 National Optical Astronomy Observatories, Tucson, AZ 85719
 112 \end_layout
 113
 114 \begin_layout Email
 115 aastex-help@aas.org
 116 \end_layout
 117
 118 \begin_layout And
 119
 120 \end_layout
 121
 122 \begin_layout Author
 123 R.
 124  J.
 125  Hanisch
 126 \begin_inset ERT
 127 status collapsed
 128
 129 \begin_layout Plain Layout
 130
 131
 132 \backslash
 133 altaffilmark{5}
 134 \end_layout
 135
 136 \end_inset
 137
 138
 139 \end_layout
 140
 141 \begin_layout Affiliation
 142 Space Telescope Science Institute, Baltimore, MD 21218
 143 \end_layout
 144
 145 \begin_layout Standard
 146 \begin_inset ERT
 147 status collapsed
 148
 149 \begin_layout Plain Layout
 150
 151
 152 \backslash
 153 altaffiltext{1}{Visiting Astronomer, Cerro Tololo Inter-American Observatory.
 154  CTIO is operated by AURA, Inc.
 155 \backslash
 156  under contract to the National Science Foundation.}
 157 \end_layout
 158
 159 \begin_layout Plain Layout
 160
 161 \end_layout
 162
 163 \begin_layout Plain Layout
 164
 165
 166 \backslash
 167 altaffiltext{2}{Society of Fellows, Harvard University.}
 168 \end_layout
 169
 170 \begin_layout Plain Layout
 171
 172 \end_layout
 173
 174 \begin_layout Plain Layout
 175
 176
 177 \backslash
 178 altaffiltext{3}{present address: Center for Astrophysics, 60 Garden Street,
 179  Cambridge, MA 02138}
 180 \end_layout
 181
 182 \begin_layout Plain Layout
 183
 184 \end_layout
 185
 186 \begin_layout Plain Layout
 187
 188
 189 \backslash
 190 altaffiltext{4}{Visiting Programmer, Space Telescope Science Institute}
 191
 192 \end_layout
 193
 194 \begin_layout Plain Layout
 195
 196 \end_layout
 197
 198 \begin_layout Plain Layout
 199
 200
 201 \backslash
 202 altaffiltext{5}{Patron, Alonso's Bar and Grill}
 203 \end_layout
 204
 205 \end_inset
 206
 207
 208 \end_layout
 209
 210 \begin_layout Abstract
 211 This is a preliminary report on surface photometry of the major fraction
 212  of known globular clusters, to see which of them show the signs of a collapsed
 213  core.
 214  We also explore some diversionary mathematics and recreational tables.
 215
 216 \end_layout
 217
 218 \begin_layout Keywords
 219 clusters: globular, peanut---bosons: bozos
 220 \end_layout
 221
 222 \begin_layout Section
 223 Introduction
 224 \end_layout
 225
 226 \begin_layout Standard
 227 A focal problem today in the dynamics of globular clusters is core collapse.
 228  It has been predicted by theory for decades
 229 \begin_inset ERT
 230 status collapsed
 231
 232 \begin_layout Plain Layout
 233
 234
 235 \backslash
 236 citep{hen61,lyn68,spi85}
 237 \end_layout
 238
 239 \end_inset
 240
 241 , but observation has been less alert to the phenomenon.
 242  For many years the central brightness peak in M15
 243 \begin_inset ERT
 244 status collapsed
 245
 246 \begin_layout Plain Layout
 247
 248
 249 \backslash
 250 citep{kin75,new78}
 251 \end_layout
 252
 253 \end_inset
 254
 255  seemed a unique anomaly.
 256  Then
 257 \begin_inset ERT
 258 status collapsed
 259
 260 \begin_layout Plain Layout
 261
 262
 263 \backslash
 264 citet{aur82}
 265 \end_layout
 266
 267 \end_inset
 268
 269  suggested a central peak in NGC 6397, and a limited photographic survey
 270  of ours
 271 \begin_inset ERT
 272 status collapsed
 273
 274 \begin_layout Plain Layout
 275
 276
 277 \backslash
 278 citep[Paper I]{djo84}
 279 \end_layout
 280
 281 \end_inset
 282
 283  found three more cases, including NGC 6624, whose sharp center had often
 284  been remarked on
 285 \begin_inset ERT
 286 status collapsed
 287
 288 \begin_layout Plain Layout
 289
 290
 291 \backslash
 292 citep{can78}
 293 \end_layout
 294
 295 \end_inset
 296
 297 .
 298
 299 \end_layout
 300
 301 \begin_layout Section
 302 Observations
 303 \end_layout
 304
 305 \begin_layout Standard
 306 All our observations were short direct exposures with CCD's.
 307  At Lick Observatory we used a TI 500
 308 \begin_inset Formula $\times$
 309 \end_inset
 310
 311 500 chip and a GEC 575
 312 \begin_inset Formula $\times$
 313 \end_inset
 314
 315 385, on the 1-m Nickel reflector.
 316  The only filter available at Lick was red.
 317  At CTIO we used a GEC 575
 318 \begin_inset Formula $\times$
 319 \end_inset
 320
 321 385, with
 322 \begin_inset Formula $B,V,$
 323 \end_inset
 324
 325  and
 326 \begin_inset Formula $R$
 327 \end_inset
 328
 329  filters, and an RCA 512
 330 \begin_inset Formula $\times$
 331 \end_inset
 332
 333 320, with
 334 \begin_inset Formula $U,B,V,R,$
 335 \end_inset
 336
 337  and
 338 \begin_inset Formula $I$
 339 \end_inset
 340
 341  filters, on the 1.5-m reflector.
 342  In the CTIO observations we tried to concentrate on the shortest practicable
 343  wavelengths; but faintness, reddening, and poor short-wavelength sensitivity
 344  often kept us from observing in
 345 \begin_inset Formula $U$
 346 \end_inset
 347
 348  or even in
 349 \begin_inset Formula $B$
 350 \end_inset
 351
 352 .
 353  All four cameras had scales of the order of 0.4 arcsec/pixel, and our field
 354  sizes were around 3 arcmin.
 355 \end_layout
 356
 357 \begin_layout Standard
 358 The CCD images are unfortunately not always suitable, for very poor clusters
 359  or for clusters with large cores.
 360  Since the latter are easily studied by other means, we augmented our own
 361  CCD profiles by collecting from the literature a number of star-count profiles
 362
 363 \begin_inset ERT
 364 status collapsed
 365
 366 \begin_layout Plain Layout
 367
 368
 369 \backslash
 370 citep{kin68,pet76,har84,ort85}
 371 \end_layout
 372
 373 \end_inset
 374
 375 , as well as photoelectric profiles
 376 \begin_inset ERT
 377 status collapsed
 378
 379 \begin_layout Plain Layout
 380
 381
 382 \backslash
 383 citep{kin66,kin75}
 384 \end_layout
 385
 386 \end_inset
 387
 388  and electronographic profiles
 389 \begin_inset ERT
 390 status collapsed
 391
 392 \begin_layout Plain Layout
 393
 394
 395 \backslash
 396 citep{kro84}
 397 \end_layout
 398
 399 \end_inset
 400
 401 .
 402  In a few cases we judged normality by eye estimates on one of the Sky Surveys.
 403 \end_layout
 404
 405 \begin_layout Section
 406 Helicity Amplitudes
 407 \end_layout
 408
 409 \begin_layout Standard
 410 It has been realized that helicity amplitudes provide a convenient means
 411  for Feynman diagram
 412 \begin_inset Foot
 413 status collapsed
 414
 415 \begin_layout Plain Layout
 416 Footnotes can be inserted like this.
 417 \end_layout
 418
 419 \end_inset
 420
 421  evaluations.
 422  These amplitude-level techniques are particularly convenient for calculations
 423  involving many Feynman diagrams, where the usual trace techniques for the
 424  amplitude squared becomes unwieldy.
 425  Our calculations use the helicity techniques developed by other authors
 426
 427 \begin_inset CommandInset citation
 428 LatexCommand cite
 429 key "hag86"
 430
 431 \end_inset
 432
 433 ; we briefly summarize below.
 434 \end_layout
 435
 436 \begin_layout Subsection
 437 Formalism
 438 \end_layout
 439
 440 \begin_layout Standard
 441 \begin_inset CommandInset label
 442 LatexCommand label
 443 name "bozomath"
 444
 445 \end_inset
 446
 447
 448 \end_layout
 449
 450 \begin_layout Standard
 451 A tree-level amplitude in
 452 \begin_inset Formula $e^{+}e^{-}$
 453 \end_inset
 454
 455  collisions can be expressed in terms of fermion strings of the form
 456 \begin_inset Formula \begin{equation}
 457 \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}
 458
 459 \end_inset
 460
 461  where
 462 \begin_inset Formula $p$
 463 \end_inset
 464
 465  and
 466 \begin_inset Formula $\sigma$
 467 \end_inset
 468
 469  label the initial
 470 \begin_inset Formula $e^{\pm}$
 471 \end_inset
 472
 473  four-momenta and helicities
 474 \begin_inset Formula $(\sigma=\pm1)$
 475 \end_inset
 476
 477 ,
 478 \begin_inset Formula $\hat{a}_{i}=a_{i}^{\mu}\gamma_{\nu}$
 479 \end_inset
 480
 481  and
 482 \begin_inset Formula $P_{\tau}=\frac{1}{2}(1+\tau\gamma_{5})$
 483 \end_inset
 484
 485  is a chirality projection operator
 486 \begin_inset Formula $(\tau=\pm1)$
 487 \end_inset
 488
 489 .
 490  The
 491 \begin_inset Formula $a_{i}^{\mu}$
 492 \end_inset
 493
 494  may be formed from particle four-momenta, gauge-boson polarization vectors
 495  or fermion strings with an uncontracted Lorentz index associated with final-sta
 496 te fermions.
 497 \end_layout
 498
 499 \begin_layout NoteToEditor
 500 Figures 1 and 2 should appear side-by-side in print
 501 \end_layout
 502
 503 \begin_layout Standard
 504 In the chiral representation the
 505 \begin_inset Formula $\gamma$
 506 \end_inset
 507
 508  matrices are expressed in terms of
 509 \begin_inset Formula $2\times2$
 510 \end_inset
 511
 512  Pauli matrices
 513 \begin_inset Formula $\sigma$
 514 \end_inset
 515
 516  and the unit matrix 1 as
 517 \begin_inset Formula \begin{eqnarray*}
 518 \gamma^{\mu} & = & \left(\begin{array}{cc}
 519 0 & \sigma_{+}^{\mu}\\
 520 \sigma_{-}^{\mu} & 0\end{array}\right),\gamma^{5}=\left(\begin{array}{cc}
 521 -1 & 0\\
 522 0 & 1\end{array}\right),\\
 523 \sigma_{\pm}^{\mu} & = & ({\textbf{1}},\pm\sigma),\end{eqnarray*}
 524
 525 \end_inset
 526
 527  giving
 528 \begin_inset Formula \begin{equation}
 529 \hat{a}=\left(\begin{array}{cc}
 530 0 & (\hat{a})_{+}\\
 531 (\hat{a})_{-} & 0\end{array}\right),(\hat{a})_{\pm}=a_{\mu}\sigma_{\pm}^{\mu},\end{equation}
 532
 533 \end_inset
 534
 535  The spinors are expressed in terms of two-component Weyl spinors as
 536 \begin_inset Formula \begin{equation}
 537 u=\left(\begin{array}{c}
 538 (u)_{-}\\
 539 (u)_{+}\end{array}\right),v={\textbf{(}}\vdag_{+}{\textbf{,}}\vdag_{-}{\textbf{)}}.\end{equation}
 540
 541 \end_inset
 542
 543
 544 \end_layout
 545
 546 \begin_layout Standard
 547 The Weyl spinors are given in terms of helicity eigenstates
 548 \begin_inset Formula $\chi_{\lambda}(p)$
 549 \end_inset
 550
 551  with
 552 \begin_inset Formula $\lambda=\pm1$
 553 \end_inset
 554
 555  by
 556 \end_layout
 557
 558 \begin_layout MathLetters
 559 \begin_inset Formula \begin{eqnarray}
 560 u(p,\lambda)_{\pm} & = & (E\pm\lambda|{\textbf{p}}|)^{1/2}\chi_{\lambda}(p),\\
 561 v(p,\lambda)_{\pm} & = & \pm\lambda(E\mp\lambda|{\textbf{p}}|)^{1/2}\chi_{-\lambda}(p)\end{eqnarray}
 562
 563 \end_inset
 564
 565
 566 \end_layout
 567
 568 \begin_layout Section
 569 Floating material and so forth
 570 \end_layout
 571
 572 \begin_layout Standard
 573 Consider a task that computes profile parameters for a modified Lorentzian
 574  of the form
 575 \begin_inset Formula \begin{equation}
 576 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}\end{equation}
 577
 578 \end_inset
 579
 580  where
 581 \begin_inset Formula \[
 582 d_{1}=\sqrt{\left(\begin{array}{c}
 583 \frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 584 \frac{y_{1}}{R_{min}}\end{array}\right)^{2}}\]
 585
 586 \end_inset
 587
 588
 589 \begin_inset Formula \[
 590 d_{2}=\sqrt{\left(\begin{array}{c}
 591 \frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 592 \case{y_{1}}{PR_{min}}\end{array}\right)^{2}}\]
 593
 594 \end_inset
 595
 596
 597 \begin_inset Formula \[
 598 x_{1}=(x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta\]
 599
 600 \end_inset
 601
 602
 603 \begin_inset Formula \[
 604 y_{1}=-(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta\]
 605
 606 \end_inset
 607
 608
 609 \end_layout
 610
 611 \begin_layout Standard
 612 In these expressions
 613 \begin_inset Formula $x_{0}$
 614 \end_inset
 615
 616 ,
 617 \begin_inset Formula $y_{0}$
 618 \end_inset
 619
 620  is the star center, and
 621 \begin_inset Formula $\Theta$
 622 \end_inset
 623
 624  is the angle with the
 625 \begin_inset Formula $x$
 626 \end_inset
 627
 628  axis.
 629  Results of this task are shown in table
 630 \begin_inset space ~
 631 \end_inset
 632
 633
 634 \begin_inset CommandInset ref
 635 LatexCommand ref
 636 reference "tbl-2"
 637
 638 \end_inset
 639
 640 .
 641  It is not clear how these sorts of analyses may affect determination of
 642
 643 \begin_inset Formula $M_{\sun}$
 644 \end_inset
 645
 646 , but the assumption is that the alternate results should be less than 90
 647 \begin_inset ERT
 648 status collapsed
 649
 650 \begin_layout Plain Layout
 651
 652
 653 \backslash
 654 degr
 655 \backslash
 656
 657 \end_layout
 658
 659 \end_inset
 660
 661 out of phase with previous values.
 662  We have no observations of
 663 \begin_inset ERT
 664 status collapsed
 665
 666 \begin_layout Plain Layout
 667
 668
 669 \backslash
 670 ion{Ca}{2}
 671 \end_layout
 672
 673 \end_inset
 674
 675 .
 676  Roughly
 677 \begin_inset ERT
 678 status collapsed
 679
 680 \begin_layout Plain Layout
 681
 682
 683 \backslash
 684 slantfrac{4}{5}
 685 \end_layout
 686
 687 \end_inset
 688
 689  of the electronically submitted abstracts for AAS meetings are error-free.
 690 \end_layout
 691
 692 \begin_layout Acknowledgements
 693
 694 \end_layout
 695
 696 \begin_layout Standard
 697 We are grateful to V.
 698  Barger, T.
 699  Han, and R.
 700  J.
 701  N.
 702  Phillips for doing the math in section
 703 \begin_inset space ~
 704 \end_inset
 705
 706
 707 \begin_inset CommandInset ref
 708 LatexCommand ref
 709 reference "bozomath"
 710
 711 \end_inset
 712
 713 .
 714  More information on the AASTeX macros package are available at
 715 \begin_inset Flex URL
 716 status collapsed
 717
 718 \begin_layout Plain Layout
 719
 720 http://www.aas.org/publications/aastex
 721 \end_layout
 722
 723 \end_inset
 724
 725  or the
 726 \begin_inset ERT
 727 status collapsed
 728
 729 \begin_layout Plain Layout
 730
 731
 732 \backslash
 733 anchor{ftp://www.aas.org/pubs/}{AAS ftp site}
 734 \end_layout
 735
 736 \end_inset
 737
 738 .
 739 \end_layout
 740
 741 \begin_layout Appendix
 742
 743 \end_layout
 744
 745 \begin_layout Section
 746 Appendicial material
 747 \end_layout
 748
 749 \begin_layout Standard
 750 Consider once again a task that computes profile parameters for a modified
 751  Lorentzian of the form
 752 \begin_inset Formula \begin{equation}
 753 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}\end{equation}
 754
 755 \end_inset
 756
 757  where
 758 \end_layout
 759
 760 \begin_layout MathLetters
 761 \begin_inset Formula \[
 762 d_{1}=\frac{3}{4}\sqrt{\left(\begin{array}{c}
 763 \frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 764 \frac{y_{1}}{R_{min}}\end{array}\right)^{2}}\]
 765
 766 \end_inset
 767
 768
 769 \begin_inset Formula \begin{equation}
 770 d_{2}=\case{3}{4}\sqrt{\left(\begin{array}{c}
 771 \frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 772 \case{y_{1}}{PR_{min}}\end{array}\right)^{2}}\end{equation}
 773
 774 \end_inset
 775
 776
 777 \begin_inset Formula \begin{eqnarray}
 778 x_{1} & = & (x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta\\
 779 y_{1} & = & -(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta\end{eqnarray}
 780
 781 \end_inset
 782
 783
 784 \end_layout
 785
 786 \begin_layout Standard
 787 For completeness, here is one last equation.
 788
 789 \begin_inset Formula \begin{equation}
 790 e=mc^{2}\end{equation}
 791
 792 \end_inset
 793
 794
 795 \end_layout
 796
 797 \begin_layout References
 798 \begin_inset CommandInset bibitem
 799 LatexCommand bibitem
 800 label "Auri\\`ere(1982)"
 801 key "aur82"
 802
 803 \end_inset
 804
 805 Aurière, M.
 806  1982,
 807 \begin_inset ERT
 808 status collapsed
 809
 810 \begin_layout Plain Layout
 811
 812
 813 \backslash
 814 aap
 815 \end_layout
 816
 817 \end_inset
 818
 819 , 109, 301
 820 \end_layout
 821
 822 \begin_layout References
 823 \begin_inset CommandInset bibitem
 824 LatexCommand bibitem
 825 label "Canizares et al.(1978)"
 826 key "can78"
 827
 828 \end_inset
 829
 830 Canizares, C.
 831  R., Grindlay, J.
 832  E., Hiltner, W.
 833  A., Liller, W., and McClintock, J.
 834  E.
 835  1978,
 836 \begin_inset ERT
 837 status collapsed
 838
 839 \begin_layout Plain Layout
 840
 841
 842 \backslash
 843 apj
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 859 Djorgovski, S., and King, I.
 860  R.
 861  1984,
 862 \begin_inset ERT
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 864
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 938 \begin_inset ERT
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 940
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 943
 944 \backslash
 945 aj
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 961 King, I.
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 985
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 987 aj
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1001 \end_inset
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1003 Kron, G.
1004  E., Hewitt, A.
1005  V., and Wasserman, L.
1006  H.
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1009 status collapsed
1010
1011 \begin_layout Plain Layout
1012
1013
1014 \backslash
1015 pasp
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1017
1018 \end_inset
1019
1020 , 96, 198
1021 \end_layout
1022
1023 \begin_layout References
1024 \begin_inset CommandInset bibitem
1025 LatexCommand bibitem
1026 label "Lynden-Bell and Wood(1968)"
1027 key "lyn68"
1028
1029 \end_inset
1030
1031 Lynden-Bell, D., and Wood, R.
1032  1968,
1033 \begin_inset ERT
1034 status collapsed
1035
1036 \begin_layout Plain Layout
1037
1038
1039 \backslash
1040 mnras
1041 \end_layout
1042
1043 \end_inset
1044
1045 , 138, 495
1046 \end_layout
1047
1048 \begin_layout References
1049 \begin_inset CommandInset bibitem
1050 LatexCommand bibitem
1051 label "Newell and O'Neil(1978)"
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1053
1054 \end_inset
1055
1056 Newell, E.
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1058  J.
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1060 \begin_inset ERT
1061 status collapsed
1062
1063 \begin_layout Plain Layout
1064
1065
1066 \backslash
1067 apjs
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1069
1070 \end_inset
1071
1072 , 37, 27
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1074
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1076 \begin_inset CommandInset bibitem
1077 LatexCommand bibitem
1078 label "Ortolani et al.(1985)"
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1081 \end_inset
1082
1083 Ortolani, S., Rosino, L., and Sandage, A.
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1085 \begin_inset ERT
1086 status collapsed
1087
1088 \begin_layout Plain Layout
1089
1090
1091 \backslash
1092 aj
1093 \end_layout
1094
1095 \end_inset
1096
1097 , 90, 473
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1099
1100 \begin_layout References
1101 \begin_inset CommandInset bibitem
1102 LatexCommand bibitem
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1105
1106 \end_inset
1107
1108 Peterson, C.
1109  J.
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1111 \begin_inset ERT
1112 status collapsed
1113
1114 \begin_layout Plain Layout
1115
1116
1117 \backslash
1118 aj
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1120
1121 \end_inset
1122
1123 , 81, 617
1124 \end_layout
1125
1126 \begin_layout References
1127 \begin_inset CommandInset bibitem
1128 LatexCommand bibitem
1129 label "Spitzer(1985)"
1130 key "spi85"
1131
1132 \end_inset
1133
1134 Spitzer, L.
1135  1985, Dynamics of Star Clusters, J.
1136  Goodman and P.
1137  Hut, Dordrecht: Reidel, 109
1138 \end_layout
1139
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1143
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1148 clearpage
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1150
1151 \end_inset
1152
1153
1154 \end_layout
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1158 LatexCommand label
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1161 \end_inset
1162
1163 This is the first figure and it uses sgi9259.eps as its EPS figure file.
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1168 LatexCommand label
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1172
1173 This is an example of a long figure caption that must be set as a paragraph.
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1176
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1181 LatexCommand label
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1185
1186 This figure has no associated EPS file, so the optional parameter is omitted.
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1218 LatexCommand label
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1221 \end_inset
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1223
1224 \end_layout
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1226 \end_inset
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1228
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1372
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1420
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1454
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1741 \end_layout
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 1.622
1750 \end_layout
1751
1752 \end_inset
1753 </cell>
1754 <cell alignment="right" valignment="top" usebox="none">
1755 \begin_inset Text
1756
1757 \begin_layout Plain Layout
1758 1.551
1759 \end_layout
1760
1761 \end_inset
1762 </cell>
1763 <cell alignment="right" valignment="top" usebox="none">
1764 \begin_inset Text
1765
1766 \begin_layout Plain Layout
1767 2.159
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 6.7
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 7.3
1786 \end_layout
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 -40.272
1795 \end_layout
1796
1797 \end_inset
1798 </cell>
1799 <cell alignment="right" valignment="top" usebox="none">
1800 \begin_inset Text
1801
1802 \begin_layout Plain Layout
1803 4
1804 \end_layout
1805
1806 \end_inset
1807 </cell>
1808 </row>
1809 <row>
1810 <cell alignment="center" valignment="top" usebox="none">
1811 \begin_inset Text
1812
1813 \begin_layout Plain Layout
1814  4
1815 \end_layout
1816
1817 \end_inset
1818 </cell>
1819 <cell alignment="right" valignment="top" usebox="none">
1820 \begin_inset Text
1821
1822 \begin_layout Plain Layout
1823 32733.8
1824 \end_layout
1825
1826 \end_inset
1827 </cell>
1828 <cell alignment="right" valignment="top" usebox="none">
1829 \begin_inset Text
1830
1831 \begin_layout Plain Layout
1832 -1.2
1833 \begin_inset ERT
1834 status collapsed
1835
1836 \begin_layout Plain Layout
1837
1838
1839 \backslash
1840 tablenotemark{c}
1841 \end_layout
1842
1843 \end_inset
1844
1845
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 -0.5
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 41
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 54.8
1873 \end_layout
1874
1875 \end_inset
1876 </cell>
1877 <cell alignment="right" valignment="top" usebox="none">
1878 \begin_inset Text
1879
1880 \begin_layout Plain Layout
1881 2.282
1882 \end_layout
1883
1884 \end_inset
1885 </cell>
1886 <cell alignment="right" valignment="top" usebox="none">
1887 \begin_inset Text
1888
1889 \begin_layout Plain Layout
1890 2.156
1891 \end_layout
1892
1893 \end_inset
1894 </cell>
1895 <cell alignment="right" valignment="top" usebox="none">
1896 \begin_inset Text
1897
1898 \begin_layout Plain Layout
1899 4.313
1900 \end_layout
1901
1902 \end_inset
1903 </cell>
1904 <cell alignment="right" valignment="top" usebox="none">
1905 \begin_inset Text
1906
1907 \begin_layout Plain Layout
1908 117.4
1909 \end_layout
1910
1911 \end_inset
1912 </cell>
1913 <cell alignment="right" valignment="top" usebox="none">
1914 \begin_inset Text
1915
1916 \begin_layout Plain Layout
1917 78.2
1918 \end_layout
1919
1920 \end_inset
1921 </cell>
1922 <cell alignment="right" valignment="top" usebox="none">
1923 \begin_inset Text
1924
1925 \begin_layout Plain Layout
1926 -35.847
1927 \end_layout
1928
1929 \end_inset
1930 </cell>
1931 <cell alignment="right" valignment="top" usebox="none">
1932 \begin_inset Text
1933
1934 \begin_layout Plain Layout
1935 5,6
1936 \end_layout
1937
1938 \end_inset
1939 </cell>
1940 </row>
1941 <row>
1942 <cell alignment="center" valignment="top" usebox="none">
1943 \begin_inset Text
1944
1945 \begin_layout Plain Layout
1946  5
1947 \end_layout
1948
1949 \end_inset
1950 </cell>
1951 <cell alignment="right" valignment="top" usebox="none">
1952 \begin_inset Text
1953
1954 \begin_layout Plain Layout
1955  9607.4
1956 \end_layout
1957
1958 \end_inset
1959 </cell>
1960 <cell alignment="right" valignment="top" usebox="none">
1961 \begin_inset Text
1962
1963 \begin_layout Plain Layout
1964 -0.4
1965 \end_layout
1966
1967 \end_inset
1968 </cell>
1969 <cell alignment="right" valignment="top" usebox="none">
1970 \begin_inset Text
1971
1972 \begin_layout Plain Layout
1973 -0.4
1974 \end_layout
1975
1976 \end_inset
1977 </cell>
1978 <cell alignment="right" valignment="top" usebox="none">
1979 \begin_inset Text
1980
1981 \begin_layout Plain Layout
1982 60
1983 \end_layout
1984
1985 \end_inset
1986 </cell>
1987 <cell alignment="right" valignment="top" usebox="none">
1988 \begin_inset Text
1989
1990 \begin_layout Plain Layout
1991 1.4
1992 \end_layout
1993
1994 \end_inset
1995 </cell>
1996 <cell alignment="right" valignment="top" usebox="none">
1997 \begin_inset Text
1998
1999 \begin_layout Plain Layout
2000 1.669
2001 \begin_inset ERT
2002 status collapsed
2003
2004 \begin_layout Plain Layout
2005
2006
2007 \backslash
2008 tablenotemark{c}
2009 \end_layout
2010
2011 \end_inset
2012
2013
2014 \end_layout
2015
2016 \end_inset
2017 </cell>
2018 <cell alignment="right" valignment="top" usebox="none">
2019 \begin_inset Text
2020
2021 \begin_layout Plain Layout
2022 1.574
2023 \end_layout
2024
2025 \end_inset
2026 </cell>
2027 <cell alignment="right" valignment="top" usebox="none">
2028 \begin_inset Text
2029
2030 \begin_layout Plain Layout
2031 2.343
2032 \end_layout
2033
2034 \end_inset
2035 </cell>
2036 <cell alignment="right" valignment="top" usebox="none">
2037 \begin_inset Text
2038
2039 \begin_layout Plain Layout
2040 8.0
2041 \end_layout
2042
2043 \end_inset
2044 </cell>
2045 <cell alignment="right" valignment="top" usebox="none">
2046 \begin_inset Text
2047
2048 \begin_layout Plain Layout
2049 8.9
2050 \end_layout
2051
2052 \end_inset
2053 </cell>
2054 <cell alignment="right" valignment="top" usebox="none">
2055 \begin_inset Text
2056
2057 \begin_layout Plain Layout
2058 -33.417
2059 \end_layout
2060
2061 \end_inset
2062 </cell>
2063 <cell alignment="right" valignment="top" usebox="none">
2064 \begin_inset Text
2065
2066 \begin_layout Plain Layout
2067 7
2068 \end_layout
2069
2070 \end_inset
2071 </cell>
2072 </row>
2073 <row>
2074 <cell alignment="center" valignment="top" usebox="none">
2075 \begin_inset Text
2076
2077 \begin_layout Plain Layout
2078  6
2079 \end_layout
2080
2081 \end_inset
2082 </cell>
2083 <cell alignment="right" valignment="top" usebox="none">
2084 \begin_inset Text
2085
2086 \begin_layout Plain Layout
2087 31638.6
2088 \end_layout
2089
2090 \end_inset
2091 </cell>
2092 <cell alignment="right" valignment="top" usebox="none">
2093 \begin_inset Text
2094
2095 \begin_layout Plain Layout
2096 1.6
2097 \end_layout
2098
2099 \end_inset
2100 </cell>
2101 <cell alignment="right" valignment="top" usebox="none">
2102 \begin_inset Text
2103
2104 \begin_layout Plain Layout
2105 0.1
2106 \end_layout
2107
2108 \end_inset
2109 </cell>
2110 <cell alignment="right" valignment="top" usebox="none">
2111 \begin_inset Text
2112
2113 \begin_layout Plain Layout
2114 39
2115 \end_layout
2116
2117 \end_inset
2118 </cell>
2119 <cell alignment="right" valignment="top" usebox="none">
2120 \begin_inset Text
2121
2122 \begin_layout Plain Layout
2123 315.2
2124 \end_layout
2125
2126 \end_inset
2127 </cell>
2128 <cell alignment="right" valignment="top" usebox="none">
2129 \begin_inset Text
2130
2131 \begin_layout Plain Layout
2132  3.433
2133 \end_layout
2134
2135 \end_inset
2136 </cell>
2137 <cell alignment="right" valignment="top" usebox="none">
2138 \begin_inset Text
2139
2140 \begin_layout Plain Layout
2141 3.075
2142 \end_layout
2143
2144 \end_inset
2145 </cell>
2146 <cell alignment="right" valignment="top" usebox="none">
2147 \begin_inset Text
2148
2149 \begin_layout Plain Layout
2150 7.488
2151 \end_layout
2152
2153 \end_inset
2154 </cell>
2155 <cell alignment="right" valignment="top" usebox="none">
2156 \begin_inset Text
2157
2158 \begin_layout Plain Layout
2159 92.1
2160 \end_layout
2161
2162 \end_inset
2163 </cell>
2164 <cell alignment="right" valignment="top" usebox="none">
2165 \begin_inset Text
2166
2167 \begin_layout Plain Layout
2168 25.3
2169 \end_layout
2170
2171 \end_inset
2172 </cell>
2173 <cell alignment="right" valignment="top" usebox="none">
2174 \begin_inset Text
2175
2176 \begin_layout Plain Layout
2177 -12.052
2178 \end_layout
2179
2180 \end_inset
2181 </cell>
2182 <cell alignment="right" valignment="top" usebox="none">
2183 \begin_inset Text
2184
2185 \begin_layout Plain Layout
2186 8
2187 \end_layout
2188
2189 \end_inset
2190 </cell>
2191 </row>
2192 </lyxtabular>
2193
2194 \end_inset
2195
2196
2197 \end_layout
2198
2199 \begin_layout Plain Layout
2200 \begin_inset ERT
2201 status collapsed
2202
2203 \begin_layout Plain Layout
2204
2205
2206 \backslash
2207 tablenotetext{a}{Sample footnote for table~
2208 \backslash
2209 ref{tbl-2} that was generated with the
2210 \backslash
2211 LaTeX
2212 \backslash
2213  table environment}
2214 \end_layout
2215
2216 \begin_layout Plain Layout
2217
2218 \end_layout
2219
2220 \begin_layout Plain Layout
2221
2222
2223 \backslash
2224 tablenotetext{b}{Yet another sample footnote for table~
2225 \backslash
2226 ref{tbl-2}}
2227 \end_layout
2228
2229 \begin_layout Plain Layout
2230
2231 \end_layout
2232
2233 \begin_layout Plain Layout
2234
2235
2236 \backslash
2237 tablenotetext{c}{Another sample footnote for table~
2238 \backslash
2239 ref{tbl-2}}
2240 \end_layout
2241
2242 \end_inset
2243
2244
2245 \end_layout
2246
2247 \begin_layout TableComments
2248 We can also attach a long-ish paragraph of explanatory material to a table.
2249  Use
2250 \backslash
2251 tablerefs to append a list of references.
2252  The following references were from a different table: I've patched them
2253  in here to show how they look, but don't take them too seriously---I certainly
2254  have not.
2255 \end_layout
2256
2257 \begin_layout TableRefs
2258 (1) Barbuy, Spite, & Spite 1985; (2) Bond 1980; (3) Carbon et al.
2259  1987; (4) Hobbs & Duncan 1987; (5) Gilroy et al.
2260  1988: (6) Gratton & Ortolani 1986; (7) Gratton & Sneden 1987; (8) Gratton
2261  & Sneden (1988); (9) Gratton & Sneden 1991; (10) Kraft et al.
2262  1982; (11) LCL, or Laird, 1990; (12) Leep & Wallerstein 1981; (13) Luck
2263  & Bond 1981; (14) Luck & Bond 1985; (15) Magain 1987; (16) Magain 1989;
2264  (17) Peterson 1981; (18) Peterson, Kurucz, & Carney 1990; (19) RMB; (20)
2265  Schuster & Nissen 1988; (21) Schuster & Nissen 1989b; (22) Spite et al.
2266  1984; (23) Spite & Spite 1986; (24) Hobbs & Thorburn 1991; (25) Hobbs et
2267  al.
2268  1991; (26) Olsen 1983.
2269 \end_layout
2270
2271 \end_inset
2272
2273
2274 \end_layout
2275
2276 \begin_layout Standard
2277 \begin_inset ERT
2278 status collapsed
2279
2280 \begin_layout Plain Layout
2281
2282 % LyX can load deluxetable files verbatim.
2283  To see this in action, uncomment the following
2284 \end_layout
2285
2286 \end_inset
2287
2288
2289 \end_layout
2290
2291 \begin_layout Standard
2292 \begin_inset ERT
2293 status collapsed
2294
2295 \begin_layout Plain Layout
2296
2297 % line (delete the
2298 \end_layout
2299
2300 \end_inset
2301
2302
2303 \begin_inset Quotes eld
2304 \end_inset
2305
2306
2307 \begin_inset ERT
2308 status collapsed
2309
2310 \begin_layout Plain Layout
2311
2312 %
2313 \end_layout
2314
2315 \end_inset
2316
2317
2318 \begin_inset Quotes erd
2319 \end_inset
2320
2321
2322 \begin_inset ERT
2323 status collapsed
2324
2325 \begin_layout Plain Layout
2326
2327 ) and copy the file table.tex from the AASTeX 5.0 distribution into
2328 \end_layout
2329
2330 \end_inset
2331
2332
2333 \end_layout
2334
2335 \begin_layout Standard
2336 \begin_inset ERT
2337 status collapsed
2338
2339 \begin_layout Plain Layout
2340
2341 % the same directory as this file.
2342 \end_layout
2343
2344 \end_inset
2345
2346
2347 \end_layout
2348
2349 \begin_layout Standard
2350 \begin_inset ERT
2351 status collapsed
2352
2353 \begin_layout Plain Layout
2354
2355 %
2356 \end_layout
2357
2358 \end_inset
2359
2360
2361 \begin_inset CommandInset include
2362 LatexCommand input
2363 filename "table"
2364
2365 \end_inset
2366
2367
2368 \end_layout
2369
2370 \end_body
2371 \end_document