1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182 183 184 185 186 187 188 189 190 191 192 193 194 195 196 197 198 199 200 201 202 203 204 205 206 207 208 209 210 211 212 213 214 215 216 217 218 219 220 221 222 223 224 225 226 227 228 229 230 231 232 233 234 235 236 237 238 239 240 241 242 243 244 245 246 247 248 249 250 251 252 253 254 255 256 257 258 259 260 261 262 263 264 265 266 267 268 269 270 271 272 273 274 275 276 277 278 279 280 281 282 283 284 285 286 287 288 289 290 291 292 293 294 295 296 297 298 299 300 301 302 303 304 305 306 307 308 309 310 311 312 313 314 315 316 317 318 319 320 321 322 323 324 325 326 327 328 329 330 331 332 333 334 335 336 337 338 339 340 341 342 343 344 345 346 347 348 349 350 351 352 353 354 355 356 357 358 359 360 361 362 363 364 365 366 367 368 369 370 371 372 373 374 375 376 377 378 379 380 381 382 383 384 385 386 387 388 389 390 391 392 393 394 395 396 397 398 399 400 401 402 403 404 405 406 407 408 409 410 411 412 413 414 415 416 417 418 419 420 421 422 423 424 425 426 427 428 429 430 431 432 433 434 435 436 437 438 439 440 441 442 443 444 445 446 447 448 449 450 451 452 453 454 455 456 457 458 459 460 461 462 463 464 465 466 467 468 469 470 471 472 473 474 475 476 477 478 479 480 481 482 483 484 485 486 487 488 489 490 491 492 493 494 495 496 497 498 499 500 501 502 503 504 505 506 507 508 509 510 511 512 513 514 515 516 517 518 519 520 521 522 523 524 525 526 527 528 529 530 531 532 533 534 535 536 537 538 539 540 541 542 543 544 545 546 547 548 549 550 551 552 553 554 555 556 557 558 559 560 561 562 563 564 565 566 567 568 569 570 571 572 573 574 575 576 577 578 579 580 581 582 583 584 585 586 587 588 589 590 591 592 593 594 595 596 597 598 599 600 601 602 603 604 605 606 607 608 609 610 611 612 613 614 615 616 617 618 619 620 621 622 623 624 625 626 627 628 629 630 631 632 633 634 635 636 637 638 639 640 641 642 643 644 645 646 647 648 649 650 651 652 653 654 655 656 657 658 659 660 661 662 663 664 665 666 667 668 669 670 671 672 673 674 675 676 677 678 679 680 681 682 683 684 685 686 687 688 689 690 691 692 693 694 695 696 697 698 699 700 701 702 703 704 705 706 707 708 709 710 711 712 713 714 715 716 717 718 719 720 721 722 723 724 725 726 727 728 729 730 731 732 733 734 735 736 737 738 739 740 741 742 743 744 745 746 747 748 749 750 751 752 753 754 755 756 757 758 759 760 761 762 763 764 765 766 767 768 769 770 771 772 773 774 775 776 777 778 779 780 781 782 783 784 785 786 787 788 789 790 791 792 793 794 795 796 797 798 799 800 801 802 803 804 805 806 807 808 809 810 811 812 813 814 815 816 817 818 819 820 821 822 823 824 825 826 827 828 829 830 831 832 833 834 835 836 837 838 839 840 841 842 843 844 845 846 847 848 849 850 851 852 853 854 855 856 857 858 859 860 861 862 863 864 865 866 867 868 869 870 871 872 873 874 875 876 877 878 879 880 881 882 883 884 885 886 887 888 889 890 891 892 893 894 895 896 897 898 899 900 901 902 903 904 905 906 907 908 909 910 911 912 913 914 915 916 917 918 919 920 921 922 923 924 925 926 927 928 929 930 931 932 933 934 935 936 937 938 939 940 941 942 943 944 945 946 947 948 949 950 951 952 953 954 955 956 957 958 959 960 961 962 963 964 965 966 967 968 969 970 971 972 973 974 975 976 977 978 979 980 981 982 983 984 985 986 987 988 989 990 991 992 993 994 995 996 997 998
|
/* File xy2sky.c
* July 18, 2007
* By Jessica Mink, Harvard-Smithsonian Center for Astrophysics
* Send bug reports to jmink@cfa.harvard.edu
Copyright (C) 1996-2007
Smithsonian Astrophysical Observatory, Cambridge, MA USA
This program is free software; you can redistribute it and/or
modify it under the terms of the GNU General Public License
as published by the Free Software Foundation; either version 2
of the License, or (at your option) any later version.
This program is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
GNU General Public License for more details.
You should have received a copy of the GNU General Public License
along with this program; if not, write to the Free Software Foundation,
Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA
*/
#include <stdio.h>
#include <stdlib.h>
#include <string.h>
#include <fcntl.h>
#include <errno.h>
#include <unistd.h>
#include <math.h>
#include "libwcs/wcs.h"
#include "libwcs/fitsfile.h"
#include "libwcs/wcscat.h"
static void PrintUsage();
extern struct WorldCoor *GetWCSFITS(); /* Read WCS from FITS or IRAF header */
static void PrintHead();
static int verbose = 0; /* verbose/debugging flag */
static int append = 0; /* append input line flag */
static int tabtable = 0; /* tab table output flag */
static int identifier = 0; /* 1st column=id flag */
static char coorsys[16];
static int linmode = -1;
static int face = 1;
static int ncm = 0;
static int printhead = 0;
static char printonly = 'n';
static int centerset = 0;
static int sizeset = 0;
static int scaleset = 0;
static int version = 0; /* If 1, print only program name and version */
static char *RevMsg = "XY2SKY WCSTools 3.9.7, 26 April 2022, Jessica Mink (jmink@cfa.harvard.edu)";
int
main (ac, av)
int ac;
char **av;
{
char *str, *str1;
char wcstring[64];
char lstr = 64;
int ndecset = 0;
int degout = 0;
int ndec = 3;
int nlines, iline;
int entx = 0;
int enty = 0;
int entmag = 0;
int i, ic;
double x, y, mag;
double cra, cdec, dra, ddec, secpix, drot;
double eqout = 0.0;
double eqin = 0.0;
int sysout = 0;
int wp, hp, nx, ny, lhead;
FILE *fd = NULL;
char *ln, *listcoord;
char *listname;
char **fnx, *newfn;
int *ft, *newft;
char linebuff[1024];
char *line;
char *header;
char *fn;
int bitpix = 0;
struct WorldCoor *wcs;
char xstr[32], ystr[32], mstr[32];
char rastr[32], decstr[32];
char keyword[16];
char temp[64];
int ncx = 0;
char *cofile;
char *cobuff;
char *space, *cstr, *dstr;
char *fni;
int nterms = 0;
char *ilistfile;
int modwcs = 0;
double mag0, magx;
double coeff[5];
struct Tokens tokens;
struct TabTable *tabxy;
struct WorldCoor *GetFITSWCS();
nfile = 0;
fn = (char **)calloc (maxnfile, sizeof(char *));
ft = (int *)calloc (maxnfile, sizeof(int));
listcoord = NULL;
listfile = NULL;
*coorsys = 0;
cofile = NULL;
/* Check for help or version command first */
str = *(av+1);
if (!str || !strcmp (str, "help") || !strcmp (str, "-help"))
PrintUsage (str);
if (!strcmp (str, "version") || !strcmp (str, "-version")) {
version = 1;
PrintUsage (str);
}
/* crack arguments */
for (av++; --ac > 0; av++) {
fn = *av;
if (*(str = *av)=='-') {
char c;
while ((c = *++str))
switch (c) {
case 'v': /* more verbosity */
verbose++;
break;
case 'a': /* Append input line to sky position */
append++;
break;
case 'b': /* initial coordinates on command line in B1950 */
str1 = *(av+1);
ic = (int)str1[0];
if (*(str+1) || ic < 48 || ic > 58) {
setsys(WCS_B1950);
sysout = WCS_B1950;
eqout = 1950.0;
}
else if (ac < 3)
PrintUsage (str);
else {
setsys (WCS_B1950);
sysout = WCS_B1950;
eqout = 1950.0;
strcpy (rastr, *++av);
ac--;
strcpy (decstr, *++av);
ac--;
setcenter (rastr, decstr);
modwcs = 1;
}
strcpy (coorsys,"B1950");
break;
case 'c': /* Magnitude conversion coefficients */
if (ac < 2)
PrintUsage (str);
cofile = *++av;
ac--;
break;
case 'd': /* Output degrees instead of hh:mm:ss dd:mm:ss */
degout++;
break;
case 'e': /* Output galactic coordinates */
str1 = *(av+1);
ic = (int)str1[0];
if (*(str+1) || ic < 48 || ic > 58) {
setsys (WCS_ECLIPTIC);
sysout = WCS_ECLIPTIC;
eqout = 2000.0;
}
else if (ac < 3)
PrintUsage (str);
else {
setsys (WCS_ECLIPTIC);
sysout = WCS_ECLIPTIC;
eqout = 2000.0;
strcpy (rastr, *++av);
ac--;
strcpy (decstr, *++av);
ac--;
setcenter (rastr, decstr);
modwcs = 1;
}
strcpy (coorsys,"ecliptic");
degout++;
break;
case 'f': /* Face to use for projections with 3rd dimension */
if (ac < 2)
PrintUsage (str);
face = atoi (*++av);
(void) wcszin (face);
ac--;
break;
case 'g': /* Output galactic coordinates */
str1 = *(av+1);
ic = (int)str1[0];
if (*(str+1) || ic < 48 || ic > 58) {
setsys (WCS_GALACTIC);
sysout = WCS_GALACTIC;
eqout = 2000.0;
}
else if (ac < 3)
PrintUsage (str);
else {
setsys (WCS_GALACTIC);
sysout = WCS_GALACTIC;
eqout = 2000.0;
strcpy (rastr, *++av);
ac--;
strcpy (decstr, *++av);
ac--;
setcenter (rastr, decstr);
modwcs = 1;
}
strcpy (coorsys,"galactic");
degout++;
break;
case 'h': /* Print column heading */
printhead++;
break;
case 'i': /* 1st column = star id */
identifier++;
break;
case 'j': /* center coordinates on command line in J2000 */
str1 = *(av+1);
ic = (int)str1[0];
if (*(str+1) || ic < 48 || ic > 58) {
setsys(WCS_J2000);
sysout = WCS_J2000;
eqout = 2000.0;
}
else if (ac < 3)
PrintUsage (str);
else {
setsys(WCS_J2000);
sysout = WCS_J2000;
eqout = 2000.0;
strcpy (rastr, *++av);
ac--;
strcpy (decstr, *++av);
ac--;
setcenter (rastr, decstr);
modwcs = 1;
}
strcpy (coorsys,"J2000");
break;
case 'k': /* column for X; Y is next column */
ncx = atoi (*++av);
ac--;
break;
case 'l': /* Mode for output of linear coordinates */
if (ac < 2)
PrintUsage (str);
linmode = atoi (*++av);
ac--;
break;
case 'm': /* column for magnitude */
ncm = atoi (*++av);
ac--;
break;
case 'n': /* Number of decimal places in output sec or deg */
if (ac < 2)
PrintUsage (str);
ndec = atoi (*++av);
ndecset++;
ac--;
break;
case 'o': /* Output only the following part of the coordinates */
if (ac < 2)
PrintUsage (str);
av++;
printonly = **av;
ac--;
break;
case 'p': /* Initial plate scale in arcseconds per pixel */
if (ac < 2)
PrintUsage (str);
setsecpix (atof (*++av));
ac--;
break;
case 'q': /* Equinox for output */
if (ac < 2)
PrintUsage (str);
strcpy (coorsys, *++av);
ac--;
break;
case 's': /* Size of image in X and Y pixels */
if (ac < 3)
PrintUsage(str);
nx = atoi (*++av);
ac--;
ny = atoi (*++av);
ac--;
modwcs = 1;
setnpix (nx, ny);
break;
case 't': /* Output tab table */
tabtable++;
break;
case 'x': /* X and Y coordinates of reference pixel */
if (ac < 3)
PrintUsage (str);
x = atof (*++av);
ac--;
y = atof (*++av);
ac--;
setrefpix (x, y);
modwcs = 1;
break;
case 'y': /* Epoch of image in FITS date format */
if (ac < 2)
PrintUsage (str);
setdateobs (*++av);
ac--;
modwcs = 1;
break;
case 'z': /* Use AIPS classic WCS */
setdefwcs (WCS_ALT);
break;
default:
PrintUsage (str);
break;
}
/* Read name of list file and classify it */
else if (fn[0] == '@') {
listname = *av + 1;
/* List of image files */
if (isimlist (listname)) {
listfile = listname;
nfile = getfilelines (listfile);
}
/* List of files which may be image files (checked when extracted) */
else if (isfilelist (listname, rootdir)) {
listfile = listname;
nfile = getfilelines (listfile);
}
/* List of x y coordinates */
else {
listcoord = listname;
if (strcmp (listcoord,"STDIN")==0 || strcmp (listcoord,"stdin")==0) {
fd = stdin;
nlines = 10000;
tabxy = NULL;
if (printhead || verbose || tabtable)
PrintHead (fn, wcs, NULL, listcoord);
}
else if (istab (listcoord)) {
tabxy = tabopen (listcoord, 0);
nlines = tabxy->nlines;
tabtable = 1;
wcs->tabsys = 1;
if (append) {
tabtable++;
PrintHead (fn, wcs, tabxy, listcoord);
}
else
PrintHead (fn, wcs, NULL, listcoord);
/* Find columns for X and Y */
entx = tabccol (tabxy, "x");
enty = tabccol (tabxy, "y");
/* Find column for magnitude */
if (!(entmag = tabccol (tabxy, "mag"))) {
if (!(entmag = tabccol (tabxy, "magv"))) {
if (!(entmag = tabccol (tabxy, "magj")))
entmag = tabccol (tabxy, "magr");
}
}
}
else {
if (printhead || verbose || tabtable)
PrintHead (fn, wcs, NULL, listcoord);
tabxy = NULL;
nlines = getfilelines (listcoord);
fd = fopen (listcoord, "r");
if (fd == NULL) {
fprintf (stderr, "Cannot read file %s\n", listcoord);
nlines = 0;
}
}
}
}
/* Add file name to list of possible image files */
else if (isfits(fn) || isiraf(fn) || istiff(fn) || isjpeg(fn) || isgif(fn)) {
if (nfile >= maxnfile) {
maxnfile = maxnfile * 2;
nbytes = maxnfile * sizeof (char *);
newfn = (char **) calloc (maxnfile, sizeof (char *));
for (i = 0; i < nfile; i++)
newfn[i] = fn[i];
free (fn);
fn = newfn;
newft = (int *) calloc (maxnfile*2, sizeof (int));
for (i = 0; i < nfile; i++)
newft[i] = ft[i];
free (ft);
ft = newft;
maxnfile = maxnfile * 2;
}
fnx[nfile] = *av;
if (isfits (*av))
ftx[nfile] = FILE_FITS;
else
ftx[nfile] = FILE_IRAF;
lfn = strlen (fn);
if (lfn > maxlfn)
maxlfn = lfn;
nfile++;
}
}
/* If no files and no coordinates print online help */
if (nfile == 0 && nlines == 0)
PrintUsage ();
/* If no file is given make WCS from arguments if coordinates entered */
wcs = NULL;
if (nfile == 0 && nlines > 0) {
fni = NULL;
lhead = 14400;
header = (char *) calloc (1, lhead);
strcpy (header, "END ");
for (i = 4; i < lhead; i++)
header[i] = ' ';
hlength (header, 14400);
hputl (header, "SIMPLE", 1);
hputi4 (header, "BITPIX", bitpix);
hputi4 (header, "NAXIS", 2);
hputi4 (header, "NAXIS1", 100);
hputi4 (header, "NAXIS2", 100);
wcs = GetFITSWCS (fni,header,verbose,&cra,&cdec,&dra,&ddec,&secpix,
&wp, &hp, &sysout, &eqout);
if (nowcs (wcs)) {
fprintf (stderr, "Incomplete WCS on command line\n");
wcsfree (wcs);
free (header);
exit (1);
}
else
nfile = 1;
}
/* Loop through files */
for (ifile = 0; ifile < nfiles; ifile++) {
if (!wcs || ifile > 0) {
fni = fn[i];
if (isfits(fni) || isiraf(fni) || istiff(fni) ||
isjpeg(fni) || isgif(fni)) {
wcs = GetWCSFITS (fni, verbose);
if (nowcs (wcs)) {
printf ("%s: No WCS for file, cannot compute image size\n", fni);
wcsfree (wcs);
exit(1);
}
}
}
if (linmode > -1)
setwcslin (wcs, linmode);
if (wcs->sysout == WCS_B1950)
wcsoutinit (wcs, "B1950");
if (wcs->sysout == WCS_J2000)
wcsoutinit (wcs, "J2000");
if (*coorsys)
wcsoutinit (wcs, coorsys);
/* Get magnitude conversion polynomial coefficients */
if (cofile != NULL) {
cobuff = getfilebuff (cofile);
mag0 = 0.0;
(void) agetr8 (cobuff, "mag0", &mag0);
for (i = 0; i < 5; i++) {
coeff[i] = 0.0;
sprintf (keyword, "mcoeff%d", i);
(void) agetr8 (cobuff, keyword, &coeff[i]);
if (coeff[i] != 0.0) nterms = i + 1;
}
if (ncm == 0)
ncm = 3;
}
if (degout) {
wcs->degout = degout;
if (!ndecset) {
ndec = 5;
ndecset++;
}
}
if (tabtable)
wcs->tabsys = 1;
if (ndecset)
wcs->ndec = ndec;
}
/* Loop through image coordinates */
while (ac-- > 1) {
/* Process file of image coordinates */
listcoord = *av;
if (listcoord[0] == '@') {
ln = listcoord;
while (*ln++)
*(ln-1) = *ln;
if (strcmp (listcoord,"STDIN")==0 || strcmp (listcoord,"stdin")==0) {
fd = stdin;
nlines = 10000;
tabxy = NULL;
if (printhead || verbose || tabtable)
PrintHead (fn, wcs, NULL, listcoord);
}
else if (istab (listcoord)) {
tabxy = tabopen (listcoord, 0);
nlines = tabxy->nlines;
tabtable = 1;
wcs->tabsys = 1;
if (append) {
tabtable++;
PrintHead (fn, wcs, tabxy, listcoord);
}
else
PrintHead (fn, wcs, NULL, listcoord);
/* Find columns for X and Y */
entx = tabccol (tabxy, "x");
enty = tabccol (tabxy, "y");
/* Find column for magnitude */
if (!(entmag = tabccol (tabxy, "mag"))) {
if (!(entmag = tabccol (tabxy, "magv"))) {
if (!(entmag = tabccol (tabxy, "magj")))
entmag = tabccol (tabxy, "magr");
}
}
}
else {
if (printhead || verbose || tabtable)
PrintHead (fn, wcs, NULL, listcoord);
tabxy = NULL;
nlines = getfilelines (listcoord);
fd = fopen (listcoord, "r");
if (fd == NULL) {
fprintf (stderr, "Cannot read file %s\n", listcoord);
nlines = 0;
}
}
for (iline = 0; iline < nlines; iline++) {
if (tabxy != NULL) {
/* Read line for next position */
if ((line = gettabline (tabxy, iline+1)) == NULL) {
fprintf (stderr,"Cannot read star %d\n", iline);
break;
}
/* Extract x, y, and magnitude */
(void) setoken (&tokens, line, "tab");
x = tabgetr8 (&tokens, entx);
y = tabgetr8 (&tokens, enty);
if (ncm)
mag = tabgetr8 (&tokens, entmag);
}
else {
if (!fgets (linebuff, 1023, fd))
break;
line = linebuff;
if (line[0] == '#')
continue;
if (ncm || ncx)
setoken (&tokens, line, "");
if (ncx) {
getoken (&tokens, ncx, xstr, 31);
getoken (&tokens, ncx+1, ystr, 31);
}
else if (identifier)
sscanf (line,"%s %s %s", temp, xstr, ystr);
else
sscanf (line,"%s %s", xstr, ystr);
x = atof (xstr);
y = atof (ystr);
if (ncm) {
wcs->printsys = 0;
getoken (&tokens, ncm, mstr, 31);
mag = atof (mstr);
}
}
if (pix2wcst (wcs, x, y, wcstring, lstr)) {
/* Remove coordinate system if tab table output
if (tabtable) {
ctab = strrchr (wcstring, (char) 9);
*ctab = (char) 0;
} */
if (wcs->sysout == WCS_ECLIPTIC) {
sprintf(temp,"%.5f",wcs->epoch);
strcat (wcstring, " ");
strcat (wcstring, temp);
}
if (ncm) {
magx = polcomp (mag, mag0, nterms, coeff);
if (tabtable)
sprintf(temp," %6.2f", magx);
else
sprintf(temp," %6.2f", magx);
strcat (wcstring, temp);
}
if (append) {
if (tabtable)
printf ("%s %s", wcstring, line);
else
printf ("%s %s", wcstring, line);
}
else {
if (tabtable)
printf ("%s ", wcstring);
else
printf ("%s ", wcstring);
if (verbose && !tabtable)
printf (" <- ");
if (wcs->nxpix > 9999 || wcs->nypix > 9999) {
if (tabtable)
printf ("%9.3f %9.3f ",x, y);
else
printf ("%9.3f %9.3f ",x, y);
}
else if (wcs->nxpix > 999 || wcs->nypix > 999) {
if (tabtable)
printf ("%8.3f %8.3f ",x, y);
else
printf ("%8.3f %8.3f ",x, y);
}
else {
if (tabtable)
printf ("%7.3f %7.3f ",x, y);
else
printf ("%7.3f %9.3f ",x, y);
}
if (wcs->naxis > 2) {
if (tabtable)
printf ("%2d ", face);
else
printf ("%2d ", face);
}
}
printf ("\n");
}
}
av++;
}
/* Process image coordinates from the command line */
else if (ac > 1) {
if (printhead || verbose) {
PrintHead (fn, wcs, NULL, NULL);
printhead = 0;
}
x = atof (*av);
ac--;
y = atof (*++av);
if (pix2wcst (wcs, x, y, wcstring, lstr)) {
if (wcs->sysout == WCS_ECLIPTIC) {
sprintf(temp,"%.5f",wcs->epoch);
if (tabtable)
strcat (wcstring, " ");
else
strcat (wcstring, " ");
strcat (wcstring, temp);
}
if (ncm) {
magx = polcomp (mag, mag0, nterms, coeff);
if (tabtable)
sprintf(temp," %6.2f", magx);
else
sprintf(temp," %6.2f", magx);
strcat (wcstring, temp);
}
if (printonly == 'r') {
space = strchr (wcstring, ' ');
*space = (char) 0;
printf ("%s ", wcstring);
if (tabtable)
printf ("%s ", wcstring);
else
printf ("%s ", wcstring);
}
else if (printonly == 'd') {
dstr = strchr (wcstring, ' ') + 1;
space = strchr (dstr, ' ');
*space = (char) 0;
if (tabtable)
printf ("%s ", dstr);
else
printf ("%s ", dstr);
}
else if (printonly == 's') {
dstr = strchr (wcstring, ' ') + 1;
cstr = strchr (dstr, ' ') + 1;
if (tabtable)
printf ("%s ", cstr);
else
printf ("%s ", cstr);
}
else {
if (tabtable)
printf ("%s ", wcstring);
else
printf ("%s ", wcstring);
if (verbose && !tabtable)
printf (" <- ");
if (wcs->nxpix > 9999 || wcs->nypix > 9999) {
if (tabtable)
printf ("%9.3f %9.3f ",x, y);
else
printf ("%9.3f %9.3f ",x, y);
}
else if (wcs->nxpix > 999 || wcs->nypix > 999) {
if (tabtable)
printf ("%8.3f %8.3f ",x, y);
else
printf ("%8.3f %8.3f ",x, y);
}
else {
if (tabtable)
printf ("%7.3f %7.3f ",x, y);
else
printf ("%7.3f %9.3f ",x, y);
}
if (wcs->naxis > 2) {
if (tabtable)
printf ("%2d ", face);
else
printf ("%2d ", face);
}
}
printf ("\n");
}
av++;
}
}
wcsfree (wcs);
return (0);
}
static void
PrintUsage (command)
char *command;
{
fprintf (stderr,"%s\n",RevMsg);
if (version)
exit (-1);
if (command != NULL) {
if (command[0] == '*')
fprintf (stderr, "%s\n", command);
else
fprintf (stderr, "* Missing argument for command: %c\n", command[0]);
exit (1);
}
fprintf (stderr,"Compute RA Dec from X Y using WCS in FITS and IRAF image files\n");
fprintf (stderr,"Usage: [-abdjgv] [-n ndec] file.fits x1 y1 ... xn yn\n");
fprintf (stderr," or : [-abdjgv] [-n ndec] file.fits @listname\n");
fprintf (stderr," -a: append input line after output position\n");
fprintf (stderr," -b [RA Dec]: Output (center) B1950 (FK4)\n");
fprintf (stderr," -c: file with coefficients for magnitude conversion\n");
fprintf (stderr," -d: RA and Dec output in degrees\n");
fprintf (stderr," -e [long lat]: Output (center) in ecliptic coordinates\n");
fprintf (stderr," -f: Number of face to use for 3-d projection\n");
fprintf (stderr," -g [long lat]: Output (center) in galactic coordinates\n");
fprintf (stderr," -i: first column is star id; 2nd, 3rd are x,y position\n");
fprintf (stderr," -j [RA Dec]: Output (center) J2000 (FK5)\n");
fprintf (stderr," -k num: Column for image X coordinate; Y follows\n");
fprintf (stderr," -l: mode for output of LINEAR WCS coordinates\n");
fprintf (stderr," -m col: column for magnitude (defaults to 3 if -c used)\n");
fprintf (stderr," -n num: number of decimal places in output RA seconds\n");
fprintf (stderr," -o r|d|s: print only ra, dec, or coordinate system\n");
fprintf (stderr," -p num: Initial plate scale in arcsec per pixel\n");
fprintf (stderr," -q: output equinox if not 2000 or 1950\n");
fprintf (stderr," -s x y: horizontal and vertical dimensions of image \n");
fprintf (stderr," -t: tab table output\n");
fprintf (stderr," -v: verbose\n");
fprintf (stderr," -x x y: X and Y coordinates of reference pixel (default is center)\n");
fprintf (stderr," -y date: Epoch of image in FITS date format or year\n");
fprintf (stderr," -y date: Epoch of image in FITS date format or year\n");
fprintf (stderr," -z: use AIPS classic projections instead of WCSLIB\n");
exit (1);
}
static void
PrintHead (fn, wcs, tabxy, listfile)
char *fn; /* Name of file containing list of x,y coordinates */
struct WorldCoor *wcs; /* World coordinate system structure */
struct TabTable *tabxy; /* tab table structure */
char *listfile; /* Name of file with list of input coordinates */
{
char newline = (char) 10;
char *eol;
char *ctab, *tabhead;
int lhead, i;
if (tabtable) {
printf ("image %s\n", fn);
if (listfile != NULL)
printf ("listfile %s\n", listfile);
printf ("radecsys %s\n",wcs->radecout);
printf ("epoch %.4f\n",wcs->epoch);
printf ("program %s\n",RevMsg);
if (wcs->sysout == WCS_B1950 || wcs->sysout == WCS_J2000)
printf ("ra dec ");
else if (wcs->sysout == WCS_GALACTIC)
printf ("glon glat ");
else if (wcs->sysout == WCS_ECLIPTIC)
printf ("elon elat ");
if (wcs->sysout == WCS_ECLIPTIC || wcs->sysout == WCS_GALACTIC)
printf ("sys ");
else
printf ("sys ");
if (wcs->sysout == WCS_ECLIPTIC)
printf ("epoch ");
if (ncm)
printf ("mag ");
if (tabxy != NULL) {
eol = strchr (tabxy->tabhead, newline);
*eol = (char) 0;
if (wcs->sysout == WCS_B1950 || wcs->sysout == WCS_J2000) {
lhead = strlen (tabxy->tabhead);
tabhead = (char *) calloc (lhead+4, sizeof (char));
ctab = tabhead;
for (i = 0; i < lhead; i++) {
*ctab++ = tabxy->tabhead[i];
if (*(ctab-2) == 'r' && *(ctab-1) == 'a')
*ctab++ = '0';
if (*(ctab-3) == 'd' && *(ctab-2) == 'e' && *(ctab-1) == 'c')
*ctab++ = '0';
}
printf ("%s", tabhead);
}
else
printf ("%s", tabxy->tabhead);
*eol = newline;
}
else {
printf ("x y ");
if (wcs->naxis > 2)
printf ("z ");
}
printf ("\n");
if (wcs->degout)
printf ("--------- --------- ");
else
printf ("------------ ------------ ");
if (wcs->sysout == WCS_ECLIPTIC || wcs->sysout == WCS_GALACTIC)
printf ("-------- ");
else
printf ("----- ");
if (wcs->sysout == WCS_ECLIPTIC)
printf ("---------- ");
if (ncm)
printf ("------ ");
if (tabxy != NULL) {
eol = strchr (tabxy->tabdash, newline);
*eol = (char) 0;
printf ("%s", tabxy->tabdash);
*eol = newline;
}
else {
printf ("-------- --------");
if (wcs->naxis > 2)
printf (" -----");
}
printf ("\n");
}
else {
fprintf (stderr,"%s\n",RevMsg);
if (listfile == NULL)
fprintf (stderr,
"Print sky coordinates from %s image coordinates\n", fn);
else
fprintf (stderr,
"Print sky coordinates from %s image coordinates in %s\n",
fn, listfile);
if (wcs->sysout == WCS_ECLIPTIC || wcs->sysout == WCS_GALACTIC)
printf ("Longitude Latitude Sys ");
else
printf (" RA Dec Sys ");
if (wcs->sysout == WCS_ECLIPTIC)
printf(" Epoch ");
if (verbose) printf (" ");
printf (" X Y\n");
}
return;
}
/*
* Feb 23 1996 New program
* Apr 24 1996 Version 1.1: Add B1950, J2000, or galactic coordinate output options
* Jun 10 1996 Change name of subroutine which reads WCS
* Aug 28 1996 Remove unused variables after lint
* Nov 1 1996 Add options to set number of decimal places and output degrees
*
* Dec 15 1997 Print message if no WCS; read IRAF 2.11 header format
* Dec 15 1997 Drop -> if output sky coordinates are in degrees
* Dec 31 1997 Allow entire input line to be appended to sky position
*
* Jan 7 1998 Apply WFPC and WFPC2 pixel corrections if requested
* Jan 7 1998 Add tab table output using -t
* Jan 26 1998 Implement Mark Calabretta's WCSLIB
* Jan 29 1998 Add -z for AIPS classic WCS projections
* Feb 18 1998 Version 2.0: Full Calabretta implementation
* Mar 12 1998 Version 2.1: IRAF TNX projection added
* Mar 27 1998 Version 2.2: Polynomial plate fit added
* Apr 24 1998 Increase size of WCS string from 40 to 64
* Apr 28 1998 Change coordinate system flag to WCS_*
* Apr 28 1998 Add output mode for linear coordinates
* Apr 28 1998 Add ecliptic coordinate system output
* May 13 1998 Allow arbitrary equinox for output coordinates
* Jun 25 1998 Set WCS subroutine choice with SETDEFWCS()
* Jul 7 1998 Change setlinmode() to setwcslin()
* Jul 7 1998 Add -f for face to use in 3-d projection
* Jul 7 1998 Add 3rd dimension in output
* Nov 30 1998 Add version and help commands for consistency
*
* Mar 29 1999 Add -i option for X,Y after ID in input file (J.-B. Marquette)
* Apr 29 1999 Drop pix2wcst declaration; it is in wcs.h
* Jun 2 1999 Make tab output completely-defined catalog
* Oct 15 1999 Free wcs using wcsfree()
* Oct 22 1999 Link includes to libwcs
*
* Jan 28 2000 Call setdefwcs() with WCS_ALT instead of 1
*
* Jul 19 2001 Add -x to specify column for X coordinate; Y follows immediately
* Jul 19 2001 Add -m to specify column for magnitude
* Jul 19 2001 Add -c to specify column for magnitude coefficients
* Jul 23 2001 Add code to calibrate magnitudes using polynomial from immatch
* Jul 25 2001 Ignore lines with # in first column
* Sep 12 2001 Fix output to match column headings
* Oct 16 2001 Increase maximum input line length from 200 to 1024
* Oct 16 2001 Add option to prepend coordinates to tab-separated table
* Oct 19 2001 Change names of old ra and dec columns if prepending ra and dec
* Dec 13 2001 Add -h for headings and add to verbose output
*
* Apr 8 2002 Free wcs structure if no WCS is found in file header
*
* Jun 19 2002 Add verbose argument to GetWCSFITS()
*
* Jan 7 2003 Fix bug which dropped declination for tab output from file
* Jan 7 2003 Fix bug which failed to ignore #-commented-out input file lines
* Apr 7 2003 Add -o to output only RA, Dec, or system
* Oct 14 2003 Change naxes to naxes in wcs structure
*
* Feb 23 2006 Allow appended headers in TIFF, JPEG, and GIF files
* Jun 21 2006 Initialize uninitialized variables
*
* Jan 10 2007 Declare RevMsg static, not const
* Jan 10 2007 Add buffer size=0 to tabopen() call
* May 2 2007 Add heading for radecsys column in tab table output
* Jul 5 2007 Parse command line arguments to initialize a WCS without a file
* Jul 18 2007 Call tabccol() instead of tabcol()
*/
|