lib/examples/aas_sample.lyx

   1 #LyX 1.3 created this file. For more info see http://www.lyx.org/
   2 \lyxformat 221
   3 \textclass aastex
   4 \begin_preamble
   5 \newcommand{\vdag}{(v)^\dagger}
   6 \newcommand{\myemail}{skywalker@galaxy.far.far.away}
   7 \slugcomment{Not to appear in Nonlearned J., 45.}
   8 \shorttitle{Djorgovski et al.}
   9 \shortauthors{Collapsed Cores in Globular Clusters}
  10 \end_preamble
  11 \language english
  12 \inputencoding default
  13 \fontscheme default
  14 \graphics default
  15 \paperfontsize default
  16 \spacing single
  17 \papersize Default
  18 \paperpackage a4
  19 \use_geometry 0
  20 \use_amsmath 0
  21 \use_natbib 0
  22 \use_numerical_citations 0
  23 \paperorientation portrait
  24 \secnumdepth 3
  25 \tocdepth 3
  26 \paragraph_separation indent
  27 \defskip medskip
  28 \quotes_language english
  29 \quotes_times 2
  30 \papercolumns 1
  31 \papersides 1
  32 \paperpagestyle default
  33
  34 \layout Title
  35
  36 Collapsed Cores in Globular Clusters,  Gauge-Boson Couplings, and AASTeX
  37 Examples
  38 \layout Author
  39
  40 S.
  41  Djorgovski
  42 \begin_inset ERT
  43 status Collapsed
  44
  45 \layout Standard
  46
  47 \backslash
  48 altaffilmark{1,2,3}
  49 \end_inset
  50
  51  and Ivan R.
  52  King
  53 \begin_inset ERT
  54 status Collapsed
  55
  56 \layout Standard
  57
  58 \backslash
  59 altaffilmark{1}
  60 \end_inset
  61
  62
  63 \layout Affiliation
  64
  65 Astronomy Department, University of California, Berkeley, CA 94720
  66 \layout Author
  67
  68 C.
  69  D.
  70  Biemesderfer
  71 \begin_inset ERT
  72 status Collapsed
  73
  74 \layout Standard
  75
  76 \backslash
  77 altaffilmark{4,5}
  78 \end_inset
  79
  80
  81 \layout Affiliation
  82
  83 National Optical Astronomy Observatories, Tucson, AZ 85719
  84 \layout Email
  85
  86 aastex-help@aas.org
  87 \layout And
  88
  89 \layout Author
  90
  91 R.
  92  J.
  93  Hanisch
  94 \begin_inset ERT
  95 status Collapsed
  96
  97 \layout Standard
  98
  99 \backslash
 100 altaffilmark{5}
 101 \end_inset
 102
 103
 104 \layout Affiliation
 105
 106 Space Telescope Science Institute, Baltimore, MD 21218
 107 \layout Standard
 108
 109
 110 \begin_inset ERT
 111 status Collapsed
 112
 113 \layout Standard
 114
 115 \backslash
 116 altaffiltext{1}{Visiting Astronomer, Cerro Tololo Inter-American Observatory.
 117  CTIO is operated by AURA, Inc.
 118 \backslash
 119  under contract to the National Science Foundation.}
 120 \layout Standard
 121
 122 \backslash
 123 altaffiltext{2}{Society of Fellows, Harvard University.}
 124 \layout Standard
 125
 126 \backslash
 127 altaffiltext{3}{present address: Center for Astrophysics, 60 Garden Street,
 128  Cambridge, MA 02138}
 129 \layout Standard
 130
 131 \backslash
 132 altaffiltext{4}{Visiting Programmer, Space Telescope Science Institute}
 133
 134 \layout Standard
 135
 136 \backslash
 137 altaffiltext{5}{Patron, Alonso's Bar and Grill}
 138 \end_inset
 139
 140
 141 \layout Abstract
 142
 143 This is a preliminary report on surface photometry of the major fraction
 144  of known globular clusters, to see which of them show the signs of a collapsed
 145  core.
 146  We also explore some diversionary mathematics and recreational tables.
 147
 148 \layout Keywords
 149
 150 clusters: globular, peanut---bosons: bozos
 151 \layout Section
 152
 153 Introduction
 154 \layout Standard
 155
 156 A focal problem today in the dynamics of globular clusters is core collapse.
 157  It has been predicted by theory for decades
 158 \begin_inset ERT
 159 status Collapsed
 160
 161 \layout Standard
 162
 163 \backslash
 164 citep{hen61,lyn68,spi85}
 165 \end_inset
 166
 167 , but observation has been less alert to the phenomenon.
 168  For many years the central brightness peak in M15
 169 \begin_inset ERT
 170 status Collapsed
 171
 172 \layout Standard
 173
 174 \backslash
 175 citep{kin75,new78}
 176 \end_inset
 177
 178  seemed a unique anomaly.
 179  Then
 180 \begin_inset ERT
 181 status Collapsed
 182
 183 \layout Standard
 184
 185 \backslash
 186 citet{aur82}
 187 \end_inset
 188
 189  suggested a central peak in NGC 6397, and a limited photographic survey
 190  of ours
 191 \begin_inset ERT
 192 status Collapsed
 193
 194 \layout Standard
 195
 196 \backslash
 197 citep[Paper I]{djo84}
 198 \end_inset
 199
 200  found three more cases, including NGC 6624, whose sharp center had often
 201  been remarked on
 202 \begin_inset ERT
 203 status Collapsed
 204
 205 \layout Standard
 206
 207 \backslash
 208 citep{can78}
 209 \end_inset
 210
 211 .
 212
 213 \layout Section
 214
 215 Observations
 216 \layout Standard
 217
 218 All our observations were short direct exposures with CCD's.
 219  At Lick Observatory we used a TI 500
 220 \begin_inset Formula \( \times  \)
 221 \end_inset
 222
 223 500 chip and a GEC 575
 224 \begin_inset Formula \( \times  \)
 225 \end_inset
 226
 227 385, on the 1-m Nickel reflector.
 228  The only filter available at Lick was red.
 229  At CTIO we used a GEC 575
 230 \begin_inset Formula \( \times  \)
 231 \end_inset
 232
 233 385, with
 234 \begin_inset Formula \( B,V, \)
 235 \end_inset
 236
 237  and
 238 \begin_inset Formula \( R \)
 239 \end_inset
 240
 241  filters, and an RCA 512
 242 \begin_inset Formula \( \times  \)
 243 \end_inset
 244
 245 320, with
 246 \begin_inset Formula \( U,B,V,R, \)
 247 \end_inset
 248
 249  and
 250 \begin_inset Formula \( I \)
 251 \end_inset
 252
 253  filters, on the 1.5-m reflector.
 254  In the CTIO observations we tried to concentrate on the shortest practicable
 255  wavelengths; but faintness, reddening, and poor short-wavelength sensitivity
 256  often kept us from observing in
 257 \begin_inset Formula \( U \)
 258 \end_inset
 259
 260  or even in
 261 \begin_inset Formula \( B \)
 262 \end_inset
 263
 264 .
 265  All four cameras had scales of the order of 0.4 arcsec/pixel, and our field
 266  sizes were around 3 arcmin.
 267 \layout Standard
 268
 269 The CCD images are unfortunately not always suitable, for very poor clusters
 270  or for clusters with large cores.
 271  Since the latter are easily studied by other means, we augmented our own
 272  CCD profiles by collecting from the literature a number of star-count profiles
 273
 274 \begin_inset ERT
 275 status Collapsed
 276
 277 \layout Standard
 278
 279 \backslash
 280 citep{kin68,pet76,har84,ort85}
 281 \end_inset
 282
 283 , as well as photoelectric profiles
 284 \begin_inset ERT
 285 status Collapsed
 286
 287 \layout Standard
 288
 289 \backslash
 290 citep{kin66,kin75}
 291 \end_inset
 292
 293  and electronographic profiles
 294 \begin_inset ERT
 295 status Collapsed
 296
 297 \layout Standard
 298
 299 \backslash
 300 citep{kro84}
 301 \end_inset
 302
 303 .
 304  In a few cases we judged normality by eye estimates on one of the Sky Surveys.
 305 \layout Section
 306
 307 Helicity Amplitudes
 308 \layout Standard
 309
 310 It has been realized that helicity amplitudes provide a convenient means
 311  for Feynman diagram
 312 \begin_inset Foot
 313 collapsed true
 314
 315 \layout Standard
 316
 317 Footnotes can be inserted like this.
 318 \end_inset
 319
 320  evaluations.
 321  These amplitude-level techniques are particularly convenient for calculations
 322  involving many Feynman diagrams, where the usual trace techniques for the
 323  amplitude squared becomes unwieldy.
 324  Our calculations use the helicity techniques developed by other authors
 325
 326 \begin_inset LatexCommand \cite{hag86}
 327
 328 \end_inset
 329
 330 ; we briefly summarize below.
 331 \layout Subsection
 332
 333 Formalism
 334 \layout Standard
 335
 336
 337 \begin_inset LatexCommand \label{bozomath}
 338
 339 \end_inset
 340
 341
 342 \layout Standard
 343
 344 A tree-level amplitude in
 345 \begin_inset Formula \( e^{+}e^{-} \)
 346 \end_inset
 347
 348  collisions can be expressed in terms of fermion strings of the form
 349 \begin_inset Formula \begin{equation}
 350 \bar{v}(p_{2},\sigma _{2})P_{-\tau }\hat{a}_{1}\hat{a}_{2}\cdots \hat{a}_{n}u(p_{1},\sigma _{1}),
 351 \end{equation}
 352
 353 \end_inset
 354
 355  where
 356 \begin_inset Formula \( p \)
 357 \end_inset
 358
 359  and
 360 \begin_inset Formula \( \sigma  \)
 361 \end_inset
 362
 363  label the initial
 364 \begin_inset Formula \( e^{\pm } \)
 365 \end_inset
 366
 367  four-momenta and helicities
 368 \begin_inset Formula \( (\sigma =\pm 1) \)
 369 \end_inset
 370
 371 ,
 372 \begin_inset Formula \( \hat{a}_{i}=a^{\mu }_{i}\gamma _{\nu } \)
 373 \end_inset
 374
 375  and
 376 \begin_inset Formula \( P_{\tau }=\frac{1}{2}(1+\tau \gamma _{5}) \)
 377 \end_inset
 378
 379  is a chirality projection operator
 380 \begin_inset Formula \( (\tau =\pm1 ) \)
 381 \end_inset
 382
 383 .
 384  The
 385 \begin_inset Formula \( a^{\mu }_{i} \)
 386 \end_inset
 387
 388  may be formed from particle four-momenta, gauge-boson polarization vectors
 389  or fermion strings with an uncontracted Lorentz index associated with final-sta
 390 te fermions.
 391 \layout NoteToEditor
 392
 393 Figures 1 and 2 should appear side-by-side in print
 394 \layout Standard
 395
 396 In the chiral representation the
 397 \begin_inset Formula \( \gamma  \)
 398 \end_inset
 399
 400  matrices are expressed in terms of
 401 \begin_inset Formula \( 2\times 2 \)
 402 \end_inset
 403
 404  Pauli matrices
 405 \begin_inset Formula \( \sigma  \)
 406 \end_inset
 407
 408  and the unit matrix 1 as
 409 \begin_inset Formula \begin{eqnarray}
 410 \gamma ^{\mu } & = & \left( \begin{array}{cc}
 411 0 & \sigma ^{\mu }_{+}\\
 412 \sigma ^{\mu }_{-} & 0
 413 \end{array}\right) ,\gamma ^{5}=\left( \begin{array}{cc}
 414 -1 & 0\\
 415 0 & 1
 416 \end{array}\right) ,\nonumber \\
 417 \sigma ^{\mu }_{\pm } & = & ({\textbf {1}},\pm \sigma ),\nonumber
 418 \end{eqnarray}
 419
 420 \end_inset
 421
 422  giving
 423 \begin_inset Formula \begin{equation}
 424 \hat{a}=\left( \begin{array}{cc}
 425 0 & (\hat{a})_{+}\\
 426 (\hat{a})_{-} & 0
 427 \end{array}\right) ,(\hat{a})_{\pm }=a_{\mu }\sigma ^{\mu }_{\pm },
 428 \end{equation}
 429
 430 \end_inset
 431
 432  The spinors are expressed in terms of two-component Weyl spinors as
 433 \begin_inset Formula \begin{equation}
 434 u=\left( \begin{array}{c}
 435 (u)_{-}\\
 436 (u)_{+}
 437 \end{array}\right) ,v={\textbf {(}}\vdag _{+}{\textbf {,}}\vdag _{-}{\textbf {)}}.
 438 \end{equation}
 439
 440 \end_inset
 441
 442
 443 \layout Standard
 444
 445 The Weyl spinors are given in terms of helicity eigenstates
 446 \begin_inset Formula \( \chi _{\lambda }(p) \)
 447 \end_inset
 448
 449  with
 450 \begin_inset Formula \( \lambda =\pm1  \)
 451 \end_inset
 452
 453  by
 454 \layout MathLetters
 455
 456
 457 \begin_inset Formula \begin{eqnarray}
 458 u(p,\lambda )_{\pm } & = & (E\pm \lambda |{\textbf {p}}|)^{1/2}\chi _{\lambda }(p),\\
 459 v(p,\lambda )_{\pm } & = & \pm \lambda (E\mp \lambda |{\textbf {p}}|)^{1/2}\chi _{-\lambda }(p)
 460 \end{eqnarray}
 461
 462 \end_inset
 463
 464
 465 \layout Section
 466
 467 Floating material and so forth
 468 \layout Standard
 469
 470 Consider a task that computes profile parameters for a modified Lorentzian
 471  of the form
 472 \begin_inset Formula \begin{equation}
 473 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
 474 \end{equation}
 475
 476 \end_inset
 477
 478  where
 479 \begin_inset Formula \[
 480 d_{1}=\sqrt{\left( \begin{array}{c}
 481 \frac{x_{1}}{R_{maj}}
 482 \end{array}\right) ^{2}+\left( \begin{array}{c}
 483 \frac{y_{1}}{R_{min}}
 484 \end{array}\right) ^{2}}\]
 485
 486 \end_inset
 487
 488
 489 \begin_inset Formula \[
 490 d_{2}=\sqrt{\left( \begin{array}{c}
 491 \frac{x_{1}}{PR_{maj}}
 492 \end{array}\right) ^{2}+\left( \begin{array}{c}
 493 \case {y_{1}}{PR_{min}}
 494 \end{array}\right) ^{2}}\]
 495
 496 \end_inset
 497
 498
 499 \begin_inset Formula \[
 500 x_{1}=(x-x_{0})\cos \Theta +(y-y_{0})\sin \Theta \]
 501
 502 \end_inset
 503
 504
 505 \begin_inset Formula \[
 506 y_{1}=-(x-x_{0})\sin \Theta +(y-y_{0})\cos \Theta \]
 507
 508 \end_inset
 509
 510
 511 \layout Standard
 512
 513 In these expressions
 514 \begin_inset Formula \( x_{0} \)
 515 \end_inset
 516
 517 ,
 518 \begin_inset Formula \( y_{0} \)
 519 \end_inset
 520
 521  is the star center, and
 522 \begin_inset Formula \( \Theta  \)
 523 \end_inset
 524
 525  is the angle with the
 526 \begin_inset Formula \( x \)
 527 \end_inset
 528
 529  axis.
 530  Results of this task are shown in table\SpecialChar ~
 531
 532 \begin_inset LatexCommand \ref{tbl-2}
 533
 534 \end_inset
 535
 536 .
 537  It is not clear how these sorts of analyses may affect determination of
 538
 539 \begin_inset Formula \( M_{\sun } \)
 540 \end_inset
 541
 542 , but the assumption is that the alternate results should be less than 90
 543 \begin_inset ERT
 544 status Collapsed
 545
 546 \layout Standard
 547
 548 \backslash
 549 degr
 550 \backslash
 551
 552 \end_inset
 553
 554 out of phase with previous values.
 555  We have no observations of
 556 \begin_inset ERT
 557 status Collapsed
 558
 559 \layout Standard
 560
 561 \backslash
 562 ion{Ca}{2}
 563 \end_inset
 564
 565 .
 566  Roughly
 567 \begin_inset ERT
 568 status Collapsed
 569
 570 \layout Standard
 571
 572 \backslash
 573 slantfrac{4}{5}
 574 \end_inset
 575
 576  of the electronically submitted abstracts for AAS meetings are error-free.
 577 \layout Acknowledgements
 578
 579 \layout Standard
 580
 581 We are grateful to V.
 582  Barger, T.
 583  Han, and R.
 584  J.
 585  N.
 586  Phillips for doing the math in section\SpecialChar ~
 587
 588 \begin_inset LatexCommand \ref{bozomath}
 589
 590 \end_inset
 591
 592 .
 593  More information on the AASTeX macros package are available at
 594
 595 \begin_inset LatexCommand \url{http://www.aas.org/publications/aastex}
 596
 597 \end_inset
 598
 599
 600  or the
 601 \begin_inset ERT
 602 status Collapsed
 603
 604 \layout Standard
 605
 606 \backslash
 607 anchor{ftp://www.aas.org/pubs/}{AAS ftp site}
 608 \end_inset
 609
 610 .
 611 \layout Appendix
 612
 613 \layout Section
 614
 615 Appendicial material
 616 \layout Standard
 617
 618 Consider once again a task that computes profile parameters for a modified
 619  Lorentzian of the form
 620 \begin_inset Formula \begin{equation}
 621 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
 622 \end{equation}
 623
 624 \end_inset
 625
 626  where
 627 \layout MathLetters
 628
 629
 630 \begin_inset Formula \[
 631 d_{1}=\frac{3}{4}\sqrt{\left( \begin{array}{c}
 632 \frac{x_{1}}{R_{maj}}
 633 \end{array}\right) ^{2}+\left( \begin{array}{c}
 634 \frac{y_{1}}{R_{min}}
 635 \end{array}\right) ^{2}}\]
 636
 637 \end_inset
 638
 639
 640 \begin_inset Formula \begin{equation}
 641 d_{2}=\case {3}{4}\sqrt{\left( \begin{array}{c}
 642 \frac{x_{1}}{PR_{maj}}
 643 \end{array}\right) ^{2}+\left( \begin{array}{c}
 644 \case {y_{1}}{PR_{min}}
 645 \end{array}\right) ^{2}}
 646 \end{equation}
 647
 648 \end_inset
 649
 650
 651 \begin_inset Formula \begin{eqnarray}
 652 x_{1} & = & (x-x_{0})\cos \Theta +(y-y_{0})\sin \Theta \\
 653 y_{1} & = & -(x-x_{0})\sin \Theta +(y-y_{0})\cos \Theta
 654 \end{eqnarray}
 655
 656 \end_inset
 657
 658
 659 \layout Standard
 660
 661 For completeness, here is one last equation.
 662
 663 \begin_inset Formula \begin{equation}
 664 e=mc^{2}
 665 \end{equation}
 666
 667 \end_inset
 668
 669
 670 \layout References
 671 \bibitem [Auri\`ere(1982)]{aur82}
 672
 673 Auri\i \`{e}
 674 re, M.
 675  1982,
 676 \begin_inset ERT
 677 status Collapsed
 678
 679 \layout Standard
 680
 681 \backslash
 682 aap
 683 \end_inset
 684
 685 , 109, 301
 686 \layout References
 687 \bibitem [Canizares et al.(1978)]{can78}
 688
 689 Canizares, C.
 690  R., Grindlay, J.
 691  E., Hiltner, W.
 692  A., Liller, W., and McClintock, J.
 693  E.
 694  1978,
 695 \begin_inset ERT
 696 status Collapsed
 697
 698 \layout Standard
 699
 700 \backslash
 701 apj
 702 \end_inset
 703
 704 , 224, 39
 705 \layout References
 706 \bibitem [Djorgovski and King(1984)]{djo84}
 707
 708 Djorgovski, S., and King, I.
 709  R.
 710  1984,
 711 \begin_inset ERT
 712 status Collapsed
 713
 714 \layout Standard
 715
 716 \backslash
 717 apjl
 718 \end_inset
 719
 720 , 277, L49
 721 \layout References
 722 \bibitem [Hagiwara and Zeppenfeld(1986)]{hag86}
 723
 724 Hagiwara, K., and Zeppenfeld, D.
 725  1986, Nucl.Phys., 274, 1
 726 \layout References
 727 \bibitem [Harris and van den Bergh(1984)]{har84}
 728
 729 Harris, W.
 730  E., and van den Bergh, S.
 731  1984,
 732 \begin_inset ERT
 733 status Collapsed
 734
 735 \layout Standard
 736
 737 \backslash
 738 aj
 739 \end_inset
 740
 741 , 89, 1816
 742 \layout References
 743 \bibitem [H\`enon(1961)]{hen61}
 744
 745 H\i \'{e}
 746 non, M.
 747  1961, Ann.d'Ap., 24, 369
 748 \layout References
 749 \bibitem [King(1966)]{kin66}
 750
 751 King, I.
 752  R.
 753  1966,
 754 \begin_inset ERT
 755 status Collapsed
 756
 757 \layout Standard
 758
 759 \backslash
 760 aj
 761 \end_inset
 762
 763 , 71, 276
 764 \layout References
 765 \bibitem [King(1975)]{kin75}
 766
 767 King, I.
 768  R.
 769  1975, Dynamics of Stellar Systems, A.
 770  Hayli, Dordrecht: Reidel, 1975, 99
 771 \layout References
 772 \bibitem [King et al.(1968)]{kin68}
 773
 774 King, I.
 775  R., Hedemann, E., Hodge, S.
 776  M., and White, R.
 777  E.
 778  1968,
 779 \begin_inset ERT
 780 status Collapsed
 781
 782 \layout Standard
 783
 784 \backslash
 785 aj
 786 \end_inset
 787
 788 , 73, 456
 789 \layout References
 790 \bibitem [Kron et al.(1984)]{kro84}
 791
 792 Kron, G.
 793  E., Hewitt, A.
 794  V., and Wasserman, L.
 795  H.
 796  1984,
 797 \begin_inset ERT
 798 status Collapsed
 799
 800 \layout Standard
 801
 802 \backslash
 803 pasp
 804 \end_inset
 805
 806 , 96, 198
 807 \layout References
 808 \bibitem [Lynden-Bell and Wood(1968)]{lyn68}
 809
 810 Lynden-Bell, D., and Wood, R.
 811  1968,
 812 \begin_inset ERT
 813 status Collapsed
 814
 815 \layout Standard
 816
 817 \backslash
 818 mnras
 819 \end_inset
 820
 821 , 138, 495
 822 \layout References
 823 \bibitem [Newell and O'Neil(1978)]{new78}
 824
 825 Newell, E.
 826  B., and O'Neil, E.
 827  J.
 828  1978,
 829 \begin_inset ERT
 830 status Collapsed
 831
 832 \layout Standard
 833
 834 \backslash
 835 apjs
 836 \end_inset
 837
 838 , 37, 27
 839 \layout References
 840 \bibitem [Ortolani et al.(1985)]{ort85}
 841
 842 Ortolani, S., Rosino, L., and Sandage, A.
 843  1985,
 844 \begin_inset ERT
 845 status Collapsed
 846
 847 \layout Standard
 848
 849 \backslash
 850 aj
 851 \end_inset
 852
 853 , 90, 473
 854 \layout References
 855 \bibitem [Peterson(1976)]{pet76}
 856
 857 Peterson, C.
 858  J.
 859  1976,
 860 \begin_inset ERT
 861 status Collapsed
 862
 863 \layout Standard
 864
 865 \backslash
 866 aj
 867 \end_inset
 868
 869 , 81, 617
 870 \layout References
 871 \bibitem [Spitzer(1985)]{spi85}
 872
 873 Spitzer, L.
 874  1985, Dynamics of Star Clusters, J.
 875  Goodman and P.
 876  Hut, Dordrecht: Reidel, 109
 877 \layout Standard
 878
 879
 880 \begin_inset ERT
 881 status Collapsed
 882
 883 \layout Standard
 884
 885 \backslash
 886 clearpage
 887 \end_inset
 888
 889
 890 \layout FigCaption
 891
 892
 893 \begin_inset LatexCommand \label{fig1}
 894
 895 \end_inset
 896
 897 This is the first figure and it uses sgi9259.eps as its EPS figure file.
 898 \layout FigCaption
 899
 900
 901 \begin_inset LatexCommand \label{fig2}
 902
 903 \end_inset
 904
 905 This is an example of a long figure caption that must be set as a paragraph.
 906   The processor has to buffer the text of the caption, so it is good not
 907  to be too wordy, but that would make for poor communication as well.
 908
 909 \layout FigCaption
 910
 911
 912 \begin_inset LatexCommand \label{fig3}
 913
 914 \end_inset
 915
 916 This figure has no associated EPS file, so the optional parameter is omitted.
 917
 918 \layout Standard
 919
 920
 921 \begin_inset ERT
 922 status Collapsed
 923
 924 \layout Standard
 925
 926 \backslash
 927 clearpage
 928 \end_inset
 929
 930
 931 \layout Standard
 932
 933 \begin_inset Float table
 934 wide false
 935 collapsed false
 936
 937 \layout Caption
 938 \added_space_bottom medskip
 939 Terribly relevant tabular information.
 940 \begin_inset LatexCommand \label{tbl-2}
 941
 942 \end_inset
 943
 944
 945 \layout Standard
 946
 947
 948 \begin_inset  Tabular
 949 <lyxtabular version="3" rows="7" columns="13">
 950 <features endhead="-1" endfirsthead="-1" endfoot="-1" endlastfoot="-1">
 951 <column alignment="center" valignment="top" width="0pt">
 952 <column alignment="right" valignment="top" width="0pt">
 953 <column alignment="right" valignment="top" width="0pt">
 954 <column alignment="right" valignment="top" width="0pt">
 955 <column alignment="right" valignment="top" width="0pt">
 956 <column alignment="right" valignment="top" width="0pt">
 957 <column alignment="right" valignment="top" width="0pt">
 958 <column alignment="right" valignment="top" width="0pt">
 959 <column alignment="right" valignment="top" width="0pt">
 960 <column alignment="right" valignment="top" width="0pt">
 961 <column alignment="right" valignment="top" width="0pt">
 962 <column alignment="right" valignment="top" width="0pt">
 963 <column alignment="center" valignment="top" width="0pt">
 964 <row>
 965 <cell alignment="center" valignment="top" topline="true" bottomline="true" usebox="none">
 966 \begin_inset Text
 967
 968 \layout Standard
 969
 970 Star
 971 \end_inset
 972 </cell>
 973 <cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
 974 \begin_inset Text
 975
 976 \layout Standard
 977
 978  Height
 979 \end_inset
 980 </cell>
 981 <cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
 982 \begin_inset Text
 983
 984 \layout Standard
 985
 986
 987 \begin_inset Formula \( d_{x} \)
 988 \end_inset
 989
 990
 991 \end_inset
 992 </cell>
 993 <cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
 994 \begin_inset Text
 995
 996 \layout Standard
 997
 998
 999 \begin_inset Formula \( d_{y} \)
1000 \end_inset
1001
1002
1003 \end_inset
1004 </cell>
1005 <cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
1006 \begin_inset Text
1007
1008 \layout Standard
1009
1010
1011 \begin_inset Formula \( n \)
1012 \end_inset
1013
1014
1015 \end_inset
1016 </cell>
1017 <cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
1018 \begin_inset Text
1019
1020 \layout Standard
1021
1022
1023 \begin_inset Formula \( \chi ^{2} \)
1024 \end_inset
1025
1026
1027 \end_inset
1028 </cell>
1029 <cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
1030 \begin_inset Text
1031
1032 \layout Standard
1033
1034
1035 \begin_inset Formula \( R_{maj} \)
1036 \end_inset
1037
1038
1039 \end_inset
1040 </cell>
1041 <cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
1042 \begin_inset Text
1043
1044 \layout Standard
1045
1046
1047 \begin_inset Formula \( R_{min} \)
1048 \end_inset
1049
1050
1051 \end_inset
1052 </cell>
1053 <cell multicolumn="1" alignment="center" valignment="top" usebox="none">
1054 \begin_inset Text
1055
1056 \layout Standard
1057
1058
1059 \begin_inset Formula \( P \)
1060 \end_inset
1061
1062
1063 \begin_inset ERT
1064 status Collapsed
1065
1066 \layout Standard
1067
1068 \backslash
1069 tablenotemark{a}
1070 \end_inset
1071
1072
1073 \end_inset
1074 </cell>
1075 <cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
1076 \begin_inset Text
1077
1078 \layout Standard
1079
1080
1081 \begin_inset Formula \( PR_{maj} \)
1082 \end_inset
1083
1084
1085 \end_inset
1086 </cell>
1087 <cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
1088 \begin_inset Text
1089
1090 \layout Standard
1091
1092
1093 \begin_inset Formula \( PR_{min} \)
1094 \end_inset
1095
1096
1097 \end_inset
1098 </cell>
1099 <cell multicolumn="1" alignment="center" valignment="top" usebox="none">
1100 \begin_inset Text
1101
1102 \layout Standard
1103
1104
1105 \begin_inset Formula \( \Theta  \)
1106 \end_inset
1107
1108
1109 \begin_inset ERT
1110 status Collapsed
1111
1112 \layout Standard
1113
1114 \backslash
1115 tablenotemark{b}
1116 \end_inset
1117
1118
1119 \end_inset
1120 </cell>
1121 <cell alignment="center" valignment="top" usebox="none">
1122 \begin_inset Text
1123
1124 \layout Standard
1125
1126 Ref.
1127 \end_inset
1128 </cell>
1129 </row>
1130 <row>
1131 <cell alignment="center" valignment="top" usebox="none">
1132 \begin_inset Text
1133
1134 \layout Standard
1135
1136
1137 \begin_inset ERT
1138 status Collapsed
1139
1140 \layout Standard
1141
1142 \backslash
1143 tableline
1144 \backslash
1145 tableline
1146 \end_inset
1147
1148 1
1149 \end_inset
1150 </cell>
1151 <cell alignment="right" valignment="top" usebox="none">
1152 \begin_inset Text
1153
1154 \layout Standard
1155
1156 33472.5
1157 \end_inset
1158 </cell>
1159 <cell alignment="right" valignment="top" usebox="none">
1160 \begin_inset Text
1161
1162 \layout Standard
1163
1164 -0.1
1165 \end_inset
1166 </cell>
1167 <cell alignment="right" valignment="top" usebox="none">
1168 \begin_inset Text
1169
1170 \layout Standard
1171
1172 0.4
1173 \end_inset
1174 </cell>
1175 <cell alignment="right" valignment="top" usebox="none">
1176 \begin_inset Text
1177
1178 \layout Standard
1179
1180 53
1181 \end_inset
1182 </cell>
1183 <cell alignment="right" valignment="top" usebox="none">
1184 \begin_inset Text
1185
1186 \layout Standard
1187
1188 27.4
1189 \end_inset
1190 </cell>
1191 <cell alignment="right" valignment="top" usebox="none">
1192 \begin_inset Text
1193
1194 \layout Standard
1195
1196 2.065
1197 \end_inset
1198 </cell>
1199 <cell alignment="right" valignment="top" usebox="none">
1200 \begin_inset Text
1201
1202 \layout Standard
1203
1204 1.940
1205 \end_inset
1206 </cell>
1207 <cell alignment="right" valignment="top" usebox="none">
1208 \begin_inset Text
1209
1210 \layout Standard
1211
1212 3.900
1213 \end_inset
1214 </cell>
1215 <cell alignment="right" valignment="top" usebox="none">
1216 \begin_inset Text
1217
1218 \layout Standard
1219
1220 68.3
1221 \end_inset
1222 </cell>
1223 <cell alignment="right" valignment="top" usebox="none">
1224 \begin_inset Text
1225
1226 \layout Standard
1227
1228 116.2
1229 \end_inset
1230 </cell>
1231 <cell alignment="right" valignment="top" usebox="none">
1232 \begin_inset Text
1233
1234 \layout Standard
1235
1236 -27.639
1237 \end_inset
1238 </cell>
1239 <cell alignment="right" valignment="top" usebox="none">
1240 \begin_inset Text
1241
1242 \layout Standard
1243
1244 1,2
1245 \end_inset
1246 </cell>
1247 </row>
1248 <row>
1249 <cell alignment="center" valignment="top" usebox="none">
1250 \begin_inset Text
1251
1252 \layout Standard
1253
1254  2
1255 \end_inset
1256 </cell>
1257 <cell alignment="right" valignment="top" usebox="none">
1258 \begin_inset Text
1259
1260 \layout Standard
1261
1262 27802.4
1263 \end_inset
1264 </cell>
1265 <cell alignment="right" valignment="top" usebox="none">
1266 \begin_inset Text
1267
1268 \layout Standard
1269
1270 -0.3
1271 \end_inset
1272 </cell>
1273 <cell alignment="right" valignment="top" usebox="none">
1274 \begin_inset Text
1275
1276 \layout Standard
1277
1278 -0.2
1279 \end_inset
1280 </cell>
1281 <cell alignment="right" valignment="top" usebox="none">
1282 \begin_inset Text
1283
1284 \layout Standard
1285
1286 60
1287 \end_inset
1288 </cell>
1289 <cell alignment="right" valignment="top" usebox="none">
1290 \begin_inset Text
1291
1292 \layout Standard
1293
1294 3.7
1295 \end_inset
1296 </cell>
1297 <cell alignment="right" valignment="top" usebox="none">
1298 \begin_inset Text
1299
1300 \layout Standard
1301
1302 1.628
1303 \end_inset
1304 </cell>
1305 <cell alignment="right" valignment="top" usebox="none">
1306 \begin_inset Text
1307
1308 \layout Standard
1309
1310 1.510
1311 \end_inset
1312 </cell>
1313 <cell alignment="right" valignment="top" usebox="none">
1314 \begin_inset Text
1315
1316 \layout Standard
1317
1318 2.156
1319 \end_inset
1320 </cell>
1321 <cell alignment="right" valignment="top" usebox="none">
1322 \begin_inset Text
1323
1324 \layout Standard
1325
1326 6.8
1327 \end_inset
1328 </cell>
1329 <cell alignment="right" valignment="top" usebox="none">
1330 \begin_inset Text
1331
1332 \layout Standard
1333
1334 7.5
1335 \end_inset
1336 </cell>
1337 <cell alignment="right" valignment="top" usebox="none">
1338 \begin_inset Text
1339
1340 \layout Standard
1341
1342 -26.764
1343 \end_inset
1344 </cell>
1345 <cell alignment="right" valignment="top" usebox="none">
1346 \begin_inset Text
1347
1348 \layout Standard
1349
1350 3
1351 \end_inset
1352 </cell>
1353 </row>
1354 <row>
1355 <cell alignment="center" valignment="top" usebox="none">
1356 \begin_inset Text
1357
1358 \layout Standard
1359
1360  3
1361 \end_inset
1362 </cell>
1363 <cell alignment="right" valignment="top" usebox="none">
1364 \begin_inset Text
1365
1366 \layout Standard
1367
1368 29210.6
1369 \end_inset
1370 </cell>
1371 <cell alignment="right" valignment="top" usebox="none">
1372 \begin_inset Text
1373
1374 \layout Standard
1375
1376 0.9
1377 \end_inset
1378 </cell>
1379 <cell alignment="right" valignment="top" usebox="none">
1380 \begin_inset Text
1381
1382 \layout Standard
1383
1384 0.3
1385 \end_inset
1386 </cell>
1387 <cell alignment="right" valignment="top" usebox="none">
1388 \begin_inset Text
1389
1390 \layout Standard
1391
1392 60
1393 \end_inset
1394 </cell>
1395 <cell alignment="right" valignment="top" usebox="none">
1396 \begin_inset Text
1397
1398 \layout Standard
1399
1400 3.4
1401 \end_inset
1402 </cell>
1403 <cell alignment="right" valignment="top" usebox="none">
1404 \begin_inset Text
1405
1406 \layout Standard
1407
1408 1.622
1409 \end_inset
1410 </cell>
1411 <cell alignment="right" valignment="top" usebox="none">
1412 \begin_inset Text
1413
1414 \layout Standard
1415
1416 1.551
1417 \end_inset
1418 </cell>
1419 <cell alignment="right" valignment="top" usebox="none">
1420 \begin_inset Text
1421
1422 \layout Standard
1423
1424 2.159
1425 \end_inset
1426 </cell>
1427 <cell alignment="right" valignment="top" usebox="none">
1428 \begin_inset Text
1429
1430 \layout Standard
1431
1432 6.7
1433 \end_inset
1434 </cell>
1435 <cell alignment="right" valignment="top" usebox="none">
1436 \begin_inset Text
1437
1438 \layout Standard
1439
1440 7.3
1441 \end_inset
1442 </cell>
1443 <cell alignment="right" valignment="top" usebox="none">
1444 \begin_inset Text
1445
1446 \layout Standard
1447
1448 -40.272
1449 \end_inset
1450 </cell>
1451 <cell alignment="right" valignment="top" usebox="none">
1452 \begin_inset Text
1453
1454 \layout Standard
1455
1456 4
1457 \end_inset
1458 </cell>
1459 </row>
1460 <row>
1461 <cell alignment="center" valignment="top" usebox="none">
1462 \begin_inset Text
1463
1464 \layout Standard
1465
1466  4
1467 \end_inset
1468 </cell>
1469 <cell alignment="right" valignment="top" usebox="none">
1470 \begin_inset Text
1471
1472 \layout Standard
1473
1474 32733.8
1475 \end_inset
1476 </cell>
1477 <cell alignment="right" valignment="top" usebox="none">
1478 \begin_inset Text
1479
1480 \layout Standard
1481
1482 -1.2
1483 \begin_inset ERT
1484 status Collapsed
1485
1486 \layout Standard
1487
1488 \backslash
1489 tablenotemark{c}
1490 \end_inset
1491
1492
1493 \end_inset
1494 </cell>
1495 <cell alignment="right" valignment="top" usebox="none">
1496 \begin_inset Text
1497
1498 \layout Standard
1499
1500 -0.5
1501 \end_inset
1502 </cell>
1503 <cell alignment="right" valignment="top" usebox="none">
1504 \begin_inset Text
1505
1506 \layout Standard
1507
1508 41
1509 \end_inset
1510 </cell>
1511 <cell alignment="right" valignment="top" usebox="none">
1512 \begin_inset Text
1513
1514 \layout Standard
1515
1516 54.8
1517 \end_inset
1518 </cell>
1519 <cell alignment="right" valignment="top" usebox="none">
1520 \begin_inset Text
1521
1522 \layout Standard
1523
1524 2.282
1525 \end_inset
1526 </cell>
1527 <cell alignment="right" valignment="top" usebox="none">
1528 \begin_inset Text
1529
1530 \layout Standard
1531
1532 2.156
1533 \end_inset
1534 </cell>
1535 <cell alignment="right" valignment="top" usebox="none">
1536 \begin_inset Text
1537
1538 \layout Standard
1539
1540 4.313
1541 \end_inset
1542 </cell>
1543 <cell alignment="right" valignment="top" usebox="none">
1544 \begin_inset Text
1545
1546 \layout Standard
1547
1548 117.4
1549 \end_inset
1550 </cell>
1551 <cell alignment="right" valignment="top" usebox="none">
1552 \begin_inset Text
1553
1554 \layout Standard
1555
1556 78.2
1557 \end_inset
1558 </cell>
1559 <cell alignment="right" valignment="top" usebox="none">
1560 \begin_inset Text
1561
1562 \layout Standard
1563
1564 -35.847
1565 \end_inset
1566 </cell>
1567 <cell alignment="right" valignment="top" usebox="none">
1568 \begin_inset Text
1569
1570 \layout Standard
1571
1572 5,6
1573 \end_inset
1574 </cell>
1575 </row>
1576 <row>
1577 <cell alignment="center" valignment="top" usebox="none">
1578 \begin_inset Text
1579
1580 \layout Standard
1581
1582  5
1583 \end_inset
1584 </cell>
1585 <cell alignment="right" valignment="top" usebox="none">
1586 \begin_inset Text
1587
1588 \layout Standard
1589
1590  9607.4
1591 \end_inset
1592 </cell>
1593 <cell alignment="right" valignment="top" usebox="none">
1594 \begin_inset Text
1595
1596 \layout Standard
1597
1598 -0.4
1599 \end_inset
1600 </cell>
1601 <cell alignment="right" valignment="top" usebox="none">
1602 \begin_inset Text
1603
1604 \layout Standard
1605
1606 -0.4
1607 \end_inset
1608 </cell>
1609 <cell alignment="right" valignment="top" usebox="none">
1610 \begin_inset Text
1611
1612 \layout Standard
1613
1614 60
1615 \end_inset
1616 </cell>
1617 <cell alignment="right" valignment="top" usebox="none">
1618 \begin_inset Text
1619
1620 \layout Standard
1621
1622 1.4
1623 \end_inset
1624 </cell>
1625 <cell alignment="right" valignment="top" usebox="none">
1626 \begin_inset Text
1627
1628 \layout Standard
1629
1630 1.669
1631 \begin_inset ERT
1632 status Collapsed
1633
1634 \layout Standard
1635
1636 \backslash
1637 tablenotemark{c}
1638 \end_inset
1639
1640
1641 \end_inset
1642 </cell>
1643 <cell alignment="right" valignment="top" usebox="none">
1644 \begin_inset Text
1645
1646 \layout Standard
1647
1648 1.574
1649 \end_inset
1650 </cell>
1651 <cell alignment="right" valignment="top" usebox="none">
1652 \begin_inset Text
1653
1654 \layout Standard
1655
1656 2.343
1657 \end_inset
1658 </cell>
1659 <cell alignment="right" valignment="top" usebox="none">
1660 \begin_inset Text
1661
1662 \layout Standard
1663
1664 8.0
1665 \end_inset
1666 </cell>
1667 <cell alignment="right" valignment="top" usebox="none">
1668 \begin_inset Text
1669
1670 \layout Standard
1671
1672 8.9
1673 \end_inset
1674 </cell>
1675 <cell alignment="right" valignment="top" usebox="none">
1676 \begin_inset Text
1677
1678 \layout Standard
1679
1680 -33.417
1681 \end_inset
1682 </cell>
1683 <cell alignment="right" valignment="top" usebox="none">
1684 \begin_inset Text
1685
1686 \layout Standard
1687
1688 7
1689 \end_inset
1690 </cell>
1691 </row>
1692 <row>
1693 <cell alignment="center" valignment="top" bottomline="true" usebox="none">
1694 \begin_inset Text
1695
1696 \layout Standard
1697
1698  6
1699 \end_inset
1700 </cell>
1701 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1702 \begin_inset Text
1703
1704 \layout Standard
1705
1706 31638.6
1707 \end_inset
1708 </cell>
1709 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1710 \begin_inset Text
1711
1712 \layout Standard
1713
1714 1.6
1715 \end_inset
1716 </cell>
1717 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1718 \begin_inset Text
1719
1720 \layout Standard
1721
1722 0.1
1723 \end_inset
1724 </cell>
1725 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1726 \begin_inset Text
1727
1728 \layout Standard
1729
1730 39
1731 \end_inset
1732 </cell>
1733 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1734 \begin_inset Text
1735
1736 \layout Standard
1737
1738 315.2
1739 \end_inset
1740 </cell>
1741 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1742 \begin_inset Text
1743
1744 \layout Standard
1745
1746  3.433
1747 \end_inset
1748 </cell>
1749 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1750 \begin_inset Text
1751
1752 \layout Standard
1753
1754 3.075
1755 \end_inset
1756 </cell>
1757 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1758 \begin_inset Text
1759
1760 \layout Standard
1761
1762 7.488
1763 \end_inset
1764 </cell>
1765 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1766 \begin_inset Text
1767
1768 \layout Standard
1769
1770 92.1
1771 \end_inset
1772 </cell>
1773 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1774 \begin_inset Text
1775
1776 \layout Standard
1777
1778 25.3
1779 \end_inset
1780 </cell>
1781 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1782 \begin_inset Text
1783
1784 \layout Standard
1785
1786 -12.052
1787 \end_inset
1788 </cell>
1789 <cell alignment="right" valignment="top" bottomline="true" usebox="none">
1790 \begin_inset Text
1791
1792 \layout Standard
1793
1794 8
1795 \end_inset
1796 </cell>
1797 </row>
1798 </lyxtabular>
1799
1800 \end_inset
1801
1802
1803 \layout Standard
1804
1805
1806 \begin_inset ERT
1807 status Collapsed
1808
1809 \layout Standard
1810
1811 \backslash
1812 tablenotetext{a}{Sample footnote for table~
1813 \backslash
1814 ref{tbl-2} that was generated with the
1815 \backslash
1816 LaTeX
1817 \backslash
1818  table environment}
1819 \layout Standard
1820
1821 \backslash
1822 tablenotetext{b}{Yet another sample footnote for table~
1823 \backslash
1824 ref{tbl-2}}
1825 \layout Standard
1826
1827 \backslash
1828 tablenotetext{c}{Another sample footnote for table~
1829 \backslash
1830 ref{tbl-2}}
1831 \end_inset
1832
1833
1834 \layout TableComments
1835
1836 We can also attach a long-ish paragraph of explanatory material to a table.
1837  Use
1838 \backslash
1839 tablerefs to append a list of references.
1840  The following references were from a different table: I've patched them
1841  in here to show how they look, but don't take them too seriously---I certainly
1842  have not.
1843 \layout TableRefs
1844
1845 (1) Barbuy, Spite, & Spite 1985; (2) Bond 1980; (3) Carbon et al.
1846  1987; (4) Hobbs & Duncan 1987; (5) Gilroy et al.
1847  1988: (6) Gratton & Ortolani 1986; (7) Gratton & Sneden 1987; (8) Gratton
1848  & Sneden (1988); (9) Gratton & Sneden 1991; (10) Kraft et al.
1849  1982; (11) LCL, or Laird, 1990; (12) Leep & Wallerstein 1981; (13) Luck
1850  & Bond 1981; (14) Luck & Bond 1985; (15) Magain 1987; (16) Magain 1989;
1851  (17) Peterson 1981; (18) Peterson, Kurucz, & Carney 1990; (19) RMB; (20)
1852  Schuster & Nissen 1988; (21) Schuster & Nissen 1989b; (22) Spite et al.
1853  1984; (23) Spite & Spite 1986; (24) Hobbs & Thorburn 1991; (25) Hobbs et
1854  al.
1855  1991; (26) Olsen 1983.
1856 \end_inset
1857
1858 \layout Standard
1859
1860
1861 \begin_inset ERT
1862 status Collapsed
1863
1864 \layout Standard
1865 % LyX can load deluxetable files verbatim.
1866  To see this in action, uncomment the following
1867 \end_inset
1868
1869
1870 \layout Standard
1871
1872
1873 \begin_inset ERT
1874 status Collapsed
1875
1876 \layout Standard
1877 % line (delete the
1878 \end_inset
1879
1880
1881 \begin_inset Quotes eld
1882 \end_inset
1883
1884
1885 \begin_inset ERT
1886 status Collapsed
1887
1888 \layout Standard
1889 %
1890 \end_inset
1891
1892
1893 \begin_inset Quotes erd
1894 \end_inset
1895
1896
1897 \begin_inset ERT
1898 status Collapsed
1899
1900 \layout Standard
1901 ) and copy the file table.tex from the AASTeX 5.0 distribution into
1902 \end_inset
1903
1904
1905 \layout Standard
1906
1907
1908 \begin_inset ERT
1909 status Collapsed
1910
1911 \layout Standard
1912 % the same directory as this file.
1913 \end_inset
1914
1915
1916 \layout Standard
1917
1918
1919 \begin_inset ERT
1920 status Collapsed
1921
1922 \layout Standard
1923 %
1924 \end_inset
1925
1926
1927 \begin_inset Include \input{table}
1928
1929 \end_inset
1930
1931
1932
1933 \the_end