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/*** File libwcs/imsetwcs.c
*** March 1, 2001
*** By Doug Mink, dmink@cfa.harvard.edu
*** Harvard-Smithsonian Center for Astrophysics
*** (based on UIowa code)
*/
#include <stdio.h>
#include <stdlib.h>
#include <math.h>
#include <string.h>
#include "fitshead.h"
#include "vimoswcs.h"
#include "lvimoswcs.h"
#include "vimoswcscat.h"
extern int FindStars();
extern int TriMatch();
extern int FocasMatch();
extern int StarMatch();
extern int ReadMatch();
extern int FitMatch();
extern int FitPlate();
extern int FluxSortStars(double *sx, double *sy, double *sb, int *sc, int ns);
extern struct WorldCoor *GetFITSVIMOSWCS ();
extern char *getimcat();
extern void SetFITSVIMOSWCS();
extern void fk524e();
extern int iscdfit();
void setsecpix2 (double secpix);
void setsecpix (double secpix);
void setrefpix (double x, double y);
void setdcenter(double ra, double dec);
void setcd(double * cd);
void setsys(int comsys0);
void setrot(int rot);
void fk425e(double *ra, double *dec, double epoch);
/* Set the C* WCS fields in a FITS header based on a reference catalog
* by finding stars in the image and in the reference catalog and
* fitting the scaling, rotation, and offsets.
* verbose generates extra info on stderr.
* Try using deeper reference star catalog searches if there is trouble.
* Return 1 if all ok, else 0
*/
/* These parameters can be set on the command line */
static double tolerance = PIXDIFF; /* +/- this many pixels is a hit */
static double refmag1 = MAGLIM1; /* reference catalog magnitude limit */
static double refmag2 = MAGLIM2; /* reference catalog magnitude limit */
static char defcatname[8]; /* default catalog name */
static double frac = 1.0; /* Additional catalog/image stars */
static int nofit = 0; /* if =1, do not fit WCS */
static int maxcat = MAXSTARS; /* Maximum number of catalog stars to use */
static int fitvimoswcs = 1; /* If 1, fit WCS, else use current WCS */
static int fitplate = 0; /* If 1, fit polynomial, else do not */
static double imfrac0 = 0.0; /* If > 0.0, multiply image dimensions
by this for search */
static int classd = -1; /* Guide Star Catalog object classes */
static int uplate = 0; /* UJ Catalog plate number to use */
static int iterate0 = 0; /* If 1, search field again */
static int toliterate0 = 0; /* if 1, halve tolerances when iter */
static int recenter0 = 0; /* If 1, search again with new center*/
static char matchcat[32]=""; /* Match catalog name */
static int irafout = 0; /* if 1, write X Y RA Dec out */
static void PrintRes();
extern void SetFITSPlate();
/* Set the C* WCS fields in the input image header based on the given limiting
* reference mag.
* Finding stars in the input image and in the reference catalog between
* refmag1 and refmag2 and compute the angle and offsets which result in the best fit.
* verbose generates extra info on stdout.
* return 0 if all ok, else -1
*/
int
SetVIMOSWCSFITS (filename, header, image, refcatname, verbose)
char *filename; /* image file name */
char *header; /* FITS header */
char *image; /* Image pixels */
char *refcatname; /* Name of reference catalog */
int verbose;
{
double *gnum; /* Reference star numbers */
double *gra; /* Reference star right ascensions in degrees */
double *gdec; /* Reference star declinations in degrees */
double *gpra; /* Reference star right ascension proper motions (deg)*/
double *gpdec; /* Reference star declination proper motions (deg) */
double *gm; /* Reference star magnitudes */
double *gmb; /* Reference star blue magnitudes */
double *gx; /* Reference star image X-coordinates in pixels */
double *gy; /* Reference star image Y-coordinates in pixels */
int *gc; /* Reference object types */
int *goff; /* Reference star offscale flags */
int ng; /* Number of reference stars in image */
int nbg; /* Number of brightest reference stars from search */
int nrg; /* Number of brightest reference stars actually used */
double *sx; /* Image star image X-coordinates in pixels */
double *sy; /* Image star image X-coordinates in pixels */
double *sb; /* Image star image flux in counts */
int *sp; /* Image star peak fluxes in counts */
int ns; /* Number of image stars */
int nbs; /* Number of brightest image stars actually used */
double cra, cdec; /* Nominal center in degrees from RA/DEC FITS fields */
double dra, ddec; /* Image half-widths in degrees */
double secpix; /* Pixel size in arcseconds */
int imw, imh; /* Image size, pixels */
int imsearch = 1; /* Flag set if image should be searched for sources */
int nmax; /* Maximum number of matches possible (nrg or nbs) */
double mag1,mag2;
int refcat; /* reference catalog switch */
double dxys;
char numstr[32];
int minstars;
int ngmax;
int nbin, nbytes;
int iterate, toliterate;
int niter = 0;
int recenter = recenter0;
int ret = 0;
int is, ig, igs;
char rstr[32], dstr[32];
double refeq, refep;
double maxnum;
int nnfld;
int refsys;
char refcoor[8];
char title[80];
char *imcatname; /* file name for image star catalog, if used */
struct WorldCoor *vimoswcs=0; /* WCS structure */
double *sx1, *sy1, *gra1, *gdec1, *gnum1, *gm1;
double imfrac = imfrac0;
int nmatch;
double ra,dec;
double dx, dy, dx2, dy2, dxy, tol2;
struct StarCat *starcat;
iterate = iterate0;
toliterate = toliterate0;
gnum = NULL;
gra = NULL;
gdec = NULL;
gpra = NULL;
gpdec = NULL;
gm = NULL;
gmb = NULL;
gx = NULL;
gy = NULL;
gc = NULL;
goff = NULL;
sb = NULL;
sx = NULL;
sy = NULL;
sp = NULL;
starcat = NULL;
/* Use already-matched stars first, if they are present */
if (strlen (matchcat) > 0) {
refsys = VIMOSWCS_J2000;
refeq = 2000.0;
if ((nbin = ReadMatch (matchcat, &sx, &sy, &gra, &gdec, verbose)) < 1) {
ret = 0;
goto out;
}
/* Set WCS from image header and command line */
vimoswcs = GetFITSVIMOSWCS (filename,header,verbose,&cra,&cdec,&dra,&ddec,
&secpix, &imw,&imh,&refsys, &refeq);
if (novimoswcs (vimoswcs)) {
ret = 0;
goto out;
}
nbin = FitMatch (nbin, sx, sy, gra, gdec, vimoswcs, verbose);
hputs (header, "WCSRFCAT", matchcat);
hputs (header, "WCSIMCAT", matchcat);
hputi4 (header, "WCSMATCH", nbin);
hputi4 (header, "WCSNREF", nbin);
if (!(gnum = (double *) calloc (nbin, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gnum\n",
nbin*sizeof(double));
for (is = 0; is < nbin; is++)
gnum[is] = (double)(is + 1);
if (!(gx = (double *) calloc (nbin, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gx\n",
nbin*sizeof(double));
if (!(gy = (double *) calloc (nbin, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gy\n",
nbin*sizeof(double));
if (!(goff = (int *) calloc (nbin, sizeof(int))))
fprintf (stderr, "Could not calloc %d bytes for gy\n",
nbin*sizeof(double));
SetFITSVIMOSWCS (header, vimoswcs);
nrg = nbin;
ns = nbin;
if (refcatname == NULL)
goto match;
}
/* Set reference catalog coordinate system and epoch */
if (nofit) {
refsys = 0;
refeq = 0.0;
}
else {
refcat = RefCat (refcatname, title, &refsys, &refeq, &refep);
vimoswcscstr (refcoor, refsys, refeq, refep);
}
/* get nominal position and scale */
getfield:
vimoswcs = GetFITSVIMOSWCS (filename,header,verbose,&cra,&cdec,&dra,&ddec,&secpix,
&imw,&imh,&refsys, &refeq);
if (novimoswcs (vimoswcs)) {
ret = 0;
goto out;
}
if (nofit) {
SetFITSVIMOSWCS (header, vimoswcs);
ret = 1;
goto out;
}
if (fitvimoswcs) {
vimoswcs->prjcode = VIMOSWCS_TAN;
vimoswcseqset (vimoswcs, refeq);
}
if (refcatname == NULL) {
refcatname = CatName (refcat);
if (refcatname == NULL) {
ret = 0;
goto out;
}
}
if (imfrac > 0.0) {
dra = dra * imfrac;
ddec = ddec * imfrac;
}
if (refmag1 == refmag2) {
mag1 = 0.0;
mag2 = 0.0;
}
else {
mag1 = refmag1;
mag2 = refmag2;
}
/* Allocate arrays for results of reference star search */
ngmax = maxcat;
if (imfrac > 1.0)
ngmax = (int) ((double) ngmax * imfrac * imfrac);
nbytes = ngmax * sizeof (double);
if (!(gnum = (double *) calloc (ngmax, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gnum\n",
ngmax*sizeof(double));
if (!(gra = (double *) calloc (ngmax, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gra\n",
ngmax*sizeof(double));
if (!(gdec = (double *) calloc (ngmax, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gdec\n",
ngmax*sizeof(double));
if (!(gpra = (double *) calloc (ngmax, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gpra\n",
ngmax*sizeof(double));
if (!(gpdec = (double *) calloc (ngmax, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gpdec\n",
ngmax*sizeof(double));
if (!(gm = (double *) calloc (ngmax, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gm\n",
ngmax*sizeof(double));
if (!(gmb = (double *) calloc (ngmax, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gmb\n",
ngmax*sizeof(double));
if (!(gc = (int *) calloc (ngmax, sizeof(int))))
fprintf (stderr, "Could not calloc %d bytes for gc\n",
ngmax*sizeof(int));
/* Find the nearby reference stars, in ra/dec */
ng = ctgread (refcatname,refcat,0,cra,cdec,dra,ddec,0.0,refsys,refeq,
vimoswcs->epoch,mag1,mag2,ngmax,&starcat,
gnum,gra,gdec,gpra,gpdec,gm,gmb,gc,NULL,verbose*100);
if (ng > ngmax)
nrg = ngmax;
else
nrg = ng;
minstars = MINSTARS;
/* Project the reference stars into pixels on a plane at ra0/dec0 */
if (!(gx = (double *) calloc (ngmax, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gx\n",
ngmax*sizeof(double));
if (!(gy = (double *) calloc (ngmax, sizeof(double))))
fprintf (stderr, "Could not calloc %d bytes for gy\n",
ngmax*sizeof(double));
if (!(goff = (int *) calloc (ngmax, sizeof(int))))
fprintf (stderr, "Could not calloc %d bytes for gy\n",
ngmax*sizeof(double));
if (!gx || !gy || !goff) {
ret = 0;
goto out;
}
/* use the nominal WCS info to find x/y on image */
for (ig = 0; ig < nrg; ig++) {
gx[ig] = 0.0;
gy[ig] = 0.0;
vimoswcs2pix (vimoswcs, gra[ig], gdec[ig], &gx[ig], &gy[ig], &goff[ig]);
}
/* Sort reference stars by brightness (magnitude) */
MagSortStars (gnum, gra, gdec, gpra, gpdec, gx, gy, gm, gmb, gc, NULL, nrg);
/* Note how reference stars were selected */
if (ng > ngmax) {
if (verbose)
fprintf (stderr,"Using %d / %d reference stars brighter than %.1f\n",
nrg, ng, gm[nrg-1]);
}
else {
if (verbose) {
if (refmag1 > 0.0 && refmag2 > 0.0)
fprintf (stderr,"Using all %d reference stars from %.1f to %.1f mag.\n",
ng, refmag1, refmag2);
else if (refmag2 > 0.0)
fprintf (stderr,"Using all %d reference stars brighter than %.1f\n",
ng,refmag2);
else
fprintf (stderr,"using all %d reference stars\n", ng);
}
}
if (verbose) {
fprintf (stderr,"%s:\n",refcatname);
for (ig = 0; ig < nrg; ig++) {
if (ig == 0)
maxnum = gnum[ig];
else if (gnum[ig] > maxnum)
maxnum = gnum[ig];
}
nnfld = CatNumLen (refcat, maxnum, 0);
for (ig = 0; ig < nrg; ig++) {
ra2str (rstr, 32, gra[ig], 3);
dec2str (dstr, 32, gdec[ig], 2);
CatNum (refcat, nnfld, 0, gnum[ig], numstr);
fprintf (stderr,"%s %s %s %5.2f %6.1f %6.1f\r",
numstr,rstr,dstr,gm[ig],gx[ig],gy[ig]);
}
fprintf (stderr,"\n");
}
if (nrg < minstars) {
if (ng < 0)
fprintf (stderr, "Error getting reference stars: %d\n", ng);
else if (ng == 0)
fprintf (stderr,"No reference stars found in image area\n");
else if (fitvimoswcs)
fprintf (stderr, "Found only %d out of %d reference stars needed\n",
nrg, minstars);
if (ng <= 0 || fitvimoswcs) {
ret = 0;
goto out;
}
}
/* Discover star-like things in the image, in pixels */
if (imsearch) {
ns = FindStars (header, image, &sx, &sy, &sb, &sp, verbose);
if (ns < minstars) {
if (ns < 0)
fprintf (stderr, "Error getting image stars: %d\n", ns);
else if (ns == 0)
fprintf (stderr,"No stars found in image\n");
else if (fitvimoswcs)
fprintf (stderr, "Need at least %d image stars but only found %d\n",
minstars, ns);
if (ns <= 0 || fitvimoswcs) {
ret = 0;
iterate = 0;
recenter = 0;
goto out;
}
}
imsearch = 0;
}
/* Fit a world coordinate system if requested */
if (fitvimoswcs) {
niter++;
/* Sort star-like objects in image by brightness */
FluxSortStars (sx, sy, sb, sp, ns);
/* If matching a catalog field the same size as the image field,
use only as many star-like objects as reference stars. If using
a larger catalog field (imfrac > 0), increase the number of stars
proportionately (imfrac^2 * the number of image stars). To adjust
for different bandpasses between the image and the reference catalog
use frac * the number of reference stars if more than image stars
or frac * the number of image stars if more than reference stars.
*/
if (imfrac > 0.0) {
double imfrac2 = imfrac * imfrac;
if (ns > (nrg / imfrac2)) {
nbs = nrg * frac / imfrac2;
if (nbs > ns)
nbs = ns;
nbg = nrg;
}
else {
nbs = ns;
nbg = (int) ((double) nbs * imfrac2);
if (nbg > nrg)
nbg = nrg;
}
}
else {
if (ns > nrg) {
nbs = nrg * frac;
if (nbs > ns)
nbs = ns;
nbg = nrg;
}
else {
nbs = ns;
nbg = nbs * frac;
if (nbg > nrg)
nbg = nrg;
}
}
if (verbose) {
if (nbg == ng)
fprintf (stderr,"Using all %d reference stars\n", ng);
else
fprintf (stderr,"Using brightest %d / %d reference stars\n", nbg, ng);
if (nbs == ns)
fprintf (stderr,"Using all %d image stars\n", ns);
else
fprintf (stderr,"Using brightest %d / %d image stars\n", nbs,ns);
}
if (verbose) {
char rastr[32], decstr[32];
double xmag, mdiff, ra, dec;
for (is = 0; is < nbs; is++) {
pix2vimoswcs (vimoswcs, sx[is], sy[is], &ra, &dec);
ra2str (rastr, 32, ra, 3);
dec2str (decstr, 32, dec, 2);
xmag = -2.5 * log10 (sb[is]);
if (!is) mdiff = gm[0] - xmag;
xmag = xmag + mdiff;
fprintf (stderr,"%4d %s %s %6.2f %6.1f %6.1f %d\r",
is+1, rastr, decstr, xmag, sx[is], sy[is], sp[is]);
}
fprintf (stderr,"\n");
}
/* Match offsets between all pairs of image stars and reference stars
and fit WCS to matches */
nbin = StarMatch (nbs,sx,sy,nbg,gra,gdec,gx,gy,tolerance,vimoswcs,verbose);
if (nbin < 0) {
fprintf (stderr, "Star registration failed.\n");
ret = 0;
goto out;
}
else if (verbose)
fprintf (stderr,"%d / %d bin hits\n", nbin, nbg);
hputs (header, "WCSRFCAT", refcatname);
imcatname = getimcat ();
if (strlen (imcatname) == 0)
hputs (header, "WCSIMCAT", filename);
else
hputs (header, "WCSIMCAT", imcatname);
hputi4 (header, "WCSMATCH", nbin);
if (ns < nbg)
hputi4 (header, "WCSNREF", ns);
else
hputi4 (header, "WCSNREF", nbg);
hputnr8 (header, "WCSTOL", 4, tolerance);
SetFITSVIMOSWCS (header, vimoswcs);
}
/* Match reference and image stars */
match:
nmatch=0;
if (verbose || !fitvimoswcs) {
imcatname = getimcat ();
if (vimoswcs->ncoeff1 > 0)
printf ("# %d-term x, %d-term y polynomial fit\n",
vimoswcs->ncoeff1, vimoswcs->ncoeff2);
else
printf ("# Arcsec/Pixel= %.6f %.6f Rotation= %.6f degrees\n",
3600.0*vimoswcs->xinc, 3600.0*vimoswcs->yinc, vimoswcs->rot);
ra2str (rstr, 32, vimoswcs->xref, 3);
dec2str (dstr, 32, vimoswcs->yref, 2);
printf ("# Optical axis= %s %s %s x= %.2f y= %.2f\n",
rstr,dstr, refcoor, vimoswcs->xrefpix, vimoswcs->yrefpix);
ra = vimoswcs->xref;
dec = vimoswcs->yref;
if (refsys == VIMOSWCS_J2000) {
(void)fk524e (&ra, &dec, vimoswcs->epoch);
ra2str (rstr, 32, ra, 3);
dec2str (dstr, 32, dec, 2);
printf ("# Optical axis= %s %s B1950 x= %.2f y= %.2f\n",
rstr,dstr, vimoswcs->xrefpix, vimoswcs->yrefpix);
}
else {
fk425e (&ra, &dec, vimoswcs->epoch);
ra2str (rstr, 32, ra, 3);
dec2str (dstr, 32, dec, 2);
printf ("# Optical axis= %s %s J2000 x= %.2f y= %.2f\n",
rstr,dstr, vimoswcs->xrefpix, vimoswcs->yrefpix);
}
}
/* Find star matches for this offset and print them */
tol2 = tolerance * tolerance;
/* Use the fit WCS info to find catalog star x/y on image */
for (ig = 0; ig < nrg; ig++) {
gx[ig] = 0.0;
gy[ig] = 0.0;
vimoswcs2pix (vimoswcs, gra[ig], gdec[ig], &gx[ig], &gy[ig], &goff[ig]);
}
/* Set maximum number of matches which are possible */
if (nrg < ns)
nmax = nrg;
else
nmax = ns;
/* Find best catalog matches to stars in image */
nmatch = 0;
nbytes = ns * sizeof (double);
gra1 = (double *) malloc (nbytes);
gdec1 = (double *) malloc (nbytes);
gm1 = (double *) malloc (nbytes);
gnum1 = (double *) malloc (nbytes);
sx1 = (double *) malloc (nbytes);
sy1 = (double *) malloc (nbytes);
for (is = 0; is < ns; is++) {
dxys = -1.0;
igs = -1;
for (ig = 0; ig < nrg; ig++) {
if (!goff[ig]) {
dx = gx[ig] - sx[is];
dy = gy[ig] - sy[is];
dx2 = dx * dx;
dy2 = dy * dy;
dxy = dx2 + dy2;
if (dxy < tol2) {
if (dxys < 0.0) {
dxys = dxy;
igs = ig;
}
else if (dxy < dxys) {
dxys = dxy;
igs = ig;
}
}
}
}
if (igs > -1) {
gnum1[nmatch] = gnum[igs];
if (gm != NULL)
gm1[nmatch] = gm[igs];
else
gm1[nmatch] = 0.0;
gra1[nmatch] = gra[igs];
gdec1[nmatch] = gdec[igs];
sx1[nmatch] = sx[is];
sy1[nmatch] = sy[is];
nmatch++;
}
}
/* If there were any matches found, print them */
if (nmatch > 0) {
int rprint = verbose || !fitvimoswcs;
hputi4 (header, "WCSMATCH", nmatch);
hputi4 (header, "WCSNREF", nmax);
hputnr8 (header, "WCSTOL", 4, tolerance);
if (rprint)
if (refcatname == NULL)
printf ("# nmatch= %d nstars= %d in and %s niter= %d\n",
nmatch, nmax, matchcat, niter);
else if (strlen (imcatname) == 0)
printf ("# nmatch= %d nstars= %d between %s and %s niter= %d\n",
nmatch, nmax, refcatname, filename, niter);
else
printf ("# nmatch= %d nstars= %d between %s and %s niter= %d\n",
nmatch, nmax, refcatname, imcatname, niter);
PrintRes (header,vimoswcs,nmatch,sx1,sy1,gra1,gdec1,gm1,gnum1,refcat,rprint);
/* Fit the matched catalog and image stars with a polynomial */
if (!iterate && !recenter && fitplate) {
if (verbose)
fprintf (stderr,"Fitting matched stars with a polynomial\n");
/* Fit residuals */
if (FitPlate (vimoswcs, sx1, sy1, gra1, gdec1, nmatch, fitplate,
verbose))
fprintf (stderr,"FitPlate cannot fit matches\n");
/* Print the new residuals */
else {
if (refcatname == NULL)
printf ("# nmatch= %d nstars= %d in %s niter= %d\n",
nmatch, nmax, matchcat, niter);
else if (strlen (imcatname) == 0)
printf ("# nmatch= %d nstars= %d between %s and %s niter= %d\n",
nmatch, nmax, refcatname, filename, niter);
else
printf ("# nmatch= %d nstars= %d between %s and %s niter= %d\n",
nmatch, nmax, refcatname, imcatname, niter);
PrintRes (header,vimoswcs,nmatch,sx1,sy1,gra1,gdec1,gm1,gnum1,refcat,verbose);
SetFITSPlate (header, vimoswcs);
}
}
}
else {
if (refcatname == NULL)
fprintf (stderr, "SetVIMOSWCSFITS: No matches in %s:\n",
matchcat);
else if (strlen (imcatname) == 0)
fprintf (stderr, "SetVIMOSWCSFITS: No matches between %s and %s:\n",
refcatname, filename);
else
fprintf (stderr, "SetVIMOSWCSFITS: No matches between %s and %s:\n",
refcatname, imcatname);
hputi4 (header, "WCSMATCH", 0);
}
if (gra1) free ((char *)gra1);
if (gdec1) free ((char *)gdec1);
if (gm1) free ((char *)gm1);
if (gnum1) free ((char *)gnum1);
ret = 1;
out:
/* Free catalog source arrays */
if (gra) free ((char *)gra);
if (gdec) free ((char *)gdec);
if (gpra) free ((char *)gpra);
if (gpdec) free ((char *)gpdec);
if (gm) free ((char *)gm);
if (gmb) free ((char *)gmb);
if (gnum) free ((char *)gnum);
if (gx) free ((char *)gx);
if (gy) free ((char *)gy);
if (gc) free ((char *)gc);
if (iterate) {
setdcenter (vimoswcs->xref, vimoswcs->yref);
setsys (vimoswcs->sysvimoswcs);
setrefpix (vimoswcs->xrefpix, vimoswcs->yrefpix);
if (iscdfit())
setcd (vimoswcs->cd);
else {
setsecpix (-3600.0 * vimoswcs->xinc);
setsecpix2 (3600.0 * vimoswcs->yinc);
setrot (vimoswcs->rot);
}
iterate--;
imfrac = 0.0;
free (vimoswcs);
goto getfield;
}
if (toliterate) {
setdcenter (vimoswcs->xref, vimoswcs->yref);
setsys (vimoswcs->sysvimoswcs);
setrefpix (vimoswcs->xrefpix, vimoswcs->yrefpix);
if (iscdfit())
setcd (vimoswcs->cd);
else {
setsecpix (-3600.0 * vimoswcs->xinc);
setsecpix2 (3600.0 * vimoswcs->yinc);
setrot (vimoswcs->rot);
}
tolerance = tolerance * 0.5;
toliterate--;
imfrac = 0.0;
free (vimoswcs);
goto getfield;
}
if (recenter) {
double ra, dec, x, y;
x = 0.5*vimoswcs->nxpix;
y = 0.5*vimoswcs->nypix;
pix2vimoswcs (vimoswcs, x, y, &ra, &dec);
setdcenter (ra, dec);
setsys (vimoswcs->sysvimoswcs);
setrefpix (x, y);
setsecpix (-3600.0 * vimoswcs->xinc);
setsecpix2 (3600.0 * vimoswcs->yinc);
setrot (vimoswcs->rot);
recenter = 0;
imfrac = 0.0;
free (vimoswcs);
goto getfield;
}
if (vimoswcs) free (vimoswcs);
/* Free image source arrays */
if (sx) free ((char *)sx);
if (sy) free ((char *)sy);
if (sb) free ((char *)sb);
if (sp) free ((char *)sp);
return (ret);
}
static void
PrintRes (header, vimoswcs, nmatch, sx1, sy1, gra1, gdec1, gm1, gnum1, refcat, verbose)
char *header; /* Image FITS header */
struct WorldCoor *vimoswcs; /* Image World Coordinate System */
int nmatch; /* Number of image/catalog matches */
double *sx1, *sy1; /* Image star pixel coordinates */
double *gra1, *gdec1; /* Reference catalog sky coordinates */
double *gm1; /* Reference catalog magnitudes */
double *gnum1; /* Reference catalog numbers */
int refcat; /* Reference catalog code */
int verbose; /* True for more information */
{
int i, goff;
double gx, gy, dx, dy, dx2, dy2, dxy;
double sep, sep2, rsep, rsep2, dsep, dsep2;
double dmatch, dmatch1, sra, sdec;
double sepsum = 0.0;
double rsepsum = 0.0;
double rsep2sum = 0.0;
double dsepsum = 0.0;
double dsep2sum = 0.0;
double sep2sum = 0.0;
double dxsum = 0.0;
double dysum = 0.0;
double dx2sum = 0.0;
double dy2sum = 0.0;
double dxysum = 0.0;
double maxnum;
int nnfld;
char rstr[32], dstr[32], numstr[32];
for (i = 0; i < nmatch; i++) {
if (i == 0)
maxnum = gnum1[i];
else if (gnum1[i] > maxnum)
maxnum = gnum1[i];
}
nnfld = CatNumLen (refcat, maxnum, 0);
for (i = 0; i < nmatch; i++) {
vimoswcs2pix (vimoswcs, gra1[i], gdec1[i], &gx, &gy, &goff);
dx = gx - sx1[i];
dy = gy - sy1[i];
dx2 = dx * dx;
dy2 = dy * dy;
dxy = dx2 + dy2;
dxsum = dxsum + dx;
dysum = dysum + dy;
dx2sum = dx2sum + dx2;
dy2sum = dy2sum + dy2;
dxysum = dxysum + sqrt (dxy);
pix2vimoswcs (vimoswcs, sx1[i], sy1[i], &sra, &sdec);
sep = 3600.0 * vimoswcsdist(gra1[i],gdec1[i],sra,sdec);
rsep = 3600.0 * ((gra1[i]-sra) * cos(degrad(sdec)));
rsep2 = rsep * rsep;
dsep = 3600.0 * (gdec1[i] - sdec);
dsep2 = dsep * dsep;
sepsum = sepsum + sep;
rsepsum = rsepsum + rsep;
dsepsum = dsepsum + dsep;
rsep2sum = rsep2sum + rsep2;
dsep2sum = dsep2sum + dsep2;
sep2sum = sep2sum + (sep*sep);
ra2str (rstr, 32, gra1[i], 3);
dec2str (dstr, 32, gdec1[i], 2);
if (irafout)
printf (" %6.1f %6.1f %s %s %5.2f ",sx1[i],sy1[i],rstr,dstr,gm1[i]);
CatNum (refcat, nnfld, 0, gnum1[i], numstr);
printf (" %s",numstr);
if (!irafout)
printf (" %s %s %5.2f %6.1f %6.1f ",rstr,dstr,gm1[i],sx1[i],sy1[i]);
printf ("%6.2f %6.2f %6.2f\n", rsep, dsep, sep);
}
dmatch = (double) nmatch;
dmatch1 = (double) (nmatch - 1);
dx = dxsum / dmatch;
dy = dysum / dmatch;
dx2 = sqrt (dx2sum / dmatch1);
dy2 = sqrt (dy2sum / dmatch1);
dxy = dxysum / dmatch;
rsep = rsepsum / dmatch;
dsep = dsepsum / dmatch;
rsep2 = sqrt (rsep2sum / dmatch1);
dsep2 = sqrt (dsep2sum / dmatch1);
sep = sepsum / dmatch;
sep2 = sqrt (sep2sum / dmatch1);
printf ("# Mean dx= %.4f/%.4f dy= %.4f/%.4f dxy= %.4f\n",
dx, dx2, dy, dy2, dxy);
printf ("# Mean dra= %.4f/%.4f ddec= %.4f/%.4f sep= %.4f/%.4f\n",
rsep, rsep2, dsep, dsep2, sep, sep2);
hputi4 (header, "WCSMATCH", nmatch);
hputnr8 (header, "WCSSEP", 3, sep);
return;
}
/* Subroutines to initialize various parameters */
void
settolerance (tol)
double tol;
{ tolerance = tol; return; }
void
setirafout ()
{ irafout = 1; return; }
void
setmatch (cat)
char *cat;
{
strcpy (matchcat, cat);
return;
}
void
setreflim (lim1, lim2)
double lim1, lim2;
{ refmag2 = lim2;
if (lim1 > -2.0) refmag1 = lim1;
return; }
void
setclass (class)
int class;
{ classd = class;
return; }
void
setfitvimoswcs (wfit)
int wfit;
{ fitvimoswcs = wfit;
return; }
void
setfitplate (nc)
int nc;
{ fitplate = nc;
return; }
void
setplate (plate)
int plate;
{ uplate = plate;
return; }
void
setnofit ()
{ nofit = 1;
return; }
void
setfrac (frac0)
double frac0;
{ if (frac0 < 1.0) frac = 1.0 + frac0;
else frac = frac0;
return; }
/* Fraction by which to increase dimensions of area to be searched */
void
setimfrac (frac0)
double frac0;
{ if (frac0 > 0.0) imfrac0 = frac0;
else imfrac0 = 1.0;
return; }
void
setmaxcat (ncat)
int ncat;
{ if (ncat < 1) maxcat = 25;
else maxcat = ncat;
return; }
void
setiterate (iter)
int iter;
{ iterate0 = iterate0 + iter;
return; }
void
setiteratet (iter)
int iter;
{ toliterate0 = toliterate0 + iter;
return; }
void
setrecenter (recenter)
int recenter;
{ recenter0 = recenter;
return; }
/* Feb 29 1996 New program
* Apr 30 1996 Add FOCAS-style catalog matching
* May 1 1996 Add initial image center from command line
* May 2 1996 Set up four star matching modes
* May 15 1996 Pass verbose flag; allow other reference catalogs
* May 16 1996 Remove sorting to separate file sortstar.c
* May 17 1996 Add class and verbose arguments
* May 22 1996 Allow for named reference catalog
* May 23 1996 Use pre-existing WCS for center, if it is present
* May 29 1996 Simplify program by always using WCS structure
* May 30 1996 Make reference/image pair matching the default method
* Jun 11 1996 Number and zero positions of image stars
* Jun 12 1996 Be more careful with nominal WCS setting
* Jun 14 1996 Add residual table
* Jun 28 1996 Set FITS header from WCS
* Jul 3 1996 Set epoch from old equinox if not already set
* Jul 19 1996 Declare tabread
* Jul 19 1996 Set image center in WCS if DSS WCS
* Jul 22 1996 Debug tab table reading
* Aug 5 1996 Add option to change WCS projection
* Aug 5 1996 Check for SECPIX1 as well as SECPIX
* Aug 5 1996 Set number of parameters to fit here
* Aug 7 1996 Save specified number of decimal places in header parameters
* Aug 7 1996 Rename old center parameters
* Aug 26 1996 Decrease default pixel tolerance from 20 to 10
* Aug 26 1996 Drop unused variable EQ in setfitswcs
* Aug 28 1996 Improve output format for matched stars
* Sep 1 1996 Set some defaults in lwcs.h
* Sep 3 1996 Fix bug to set plate scale from command line
* Sep 4 1996 Print reference catalog name on separate line from entries
* Sep 17 1996 Clean up code
* Oct 15 1996 Break off getfitswcs into separate file
* Nov 18 1996 Add USNO A catalog searching
* Nov 18 1996 Write same number into CROAT2 as CROTA1
* Nov 19 1996 If EPOCH was equinox in original image or not set, set it
* Dec 10 1996 Make equinox double in getfitswcs call
*
* Mar 17 1997 Print found reference stars even when there are not enough
* Jul 14 1997 If nfit is negative return with header set for nominal WCS
* Aug 4 1997 Reset nfit limit to 7 for reference pixel fit and fix nfit0 bug
* Aug 20 1997 Make maximum number of reference stars settable on the command line
* Aug 28 1997 Print star ID numbers in appropriate format for each catalog
* Aug 28 1997 Add option to match image to reference stars without fitting WCS
* Sep 3 1997 Add option to change image dimensions by a fraction
* Sep 9 1997 Return with default WCS in header only if nfit < -7
* Sep 9 1997 Print separate right ascension and declination residuals
* Sep 11 1997 Print average magnitude as well as value of residuals
* Oct 16 1997 Print same information for image stars as for reference stars
* Oct 22 1997 Print result of chip rotation as well as optical axis rotation
* Nov 6 1997 Move nfit entirely to matchstar
* Nov 6 1997 Rearrange output for IMMATCH use, adding filename argument
* Nov 14 1997 Increase, not multiply, dimensions by IMFRAC
* Nov 17 1997 Initialize both magnitude limits
* Dec 1 1997 Fix bug computing RA separation
* Dec 16 1997 Fix bug printing no match error message
*
* Jan 26 1998 Remove chip rotation code
* Jan 27 1998 Add switch to use either Calabretta or classic AIPS WCS
* Jan 29 1998 Fix summary to keep only one reference star per image star
* Feb 3 1998 Add option to improve WCS by fitting residuals
* Feb 12 1998 Add USNO SA catalog to reference catalog options
* Feb 12 1998 Match stars even if less than the minimum if no WCS fit
* Feb 19 1998 Increase number of reference stars if IMFRAC > 1
* Feb 22 1998 Fix residual fitting
* Mar 3 1998 Repeat field search and match after first try
* Mar 4 1998 Use imfrac on first pass, but not second
* Mar 5 1998 Correct number of stars used if IMFRAC > 1
* Mar 6 1998 Add option to use image center for second pass
* Mar 25 1998 Change residual polynomial fit to full plate-style polynomial
* Mar 25 1998 Move residual printing to a subroutine
* Mar 26 1998 Do not fit polynomial until both recenter and iterate done
* Mar 27 1998 Save plate fit coefficients to FITS header
* Apr 8 1998 Reset equinox to that of reference catalog
* Apr 30 1998 Handle prematched star/pixel file
* Jun 24 1998 Add string lengths to ra2str() and dec2str() calls
* Sep 17 1998 Allow use of catalogs with other than J2000 coordinates
* Sep 17 1998 Add coordinate system argument to GetFITSWCS()
* Sep 28 1998 Add SAO binary format catalogs (SAO, PPM, IRAS, Tycho)
* Sep 28 1998 Pass system, equinox, and epoch to all catalog search programs
* Oct 2 1998 Fix arguments in call to GetFITSWCS
* Oct 7 1998 Set projection to TAN before fitting
* Oct 16 1998 Add option to read from TDC ASCII format catalog
* Oct 26 1998 Use passed refcatname and new RefCat subroutine and wcscat.h
* Oct 26 1998 Add TDC binary catalog option
* Oct 28 1998 Only search for sources in image once
* Nov 19 1998 Add catalog name to uacread() call
* Dec 1 1998 Add version 2.0 of USNO A and SA catalogs
* Dec 8 1998 Add support for ACT and Hipparcos catalogs
* Jan 9 1999 Fix bug so that no fit option works
* Jan 26 1999 Add option to output matched image/catalog stars
* Feb 10 1999 Finish support for ACT reference catalog
* Apr 7 1999 Add file name to GetFITSWCS call
* Apr 21 1999 Fix RA residual bug: *cos(dec), not /cos(dec)
* Jul 7 1999 Fix bug setting secpix when iterating
* Jul 7 1999 List catalog and image stars without linefeeds
* Jul 9 1999 Log tabread() every 100 if verbose
* Jul 23 1999 Add BSC for very wide fields
* Jul 26 1999 Add WCSIMCAT, WCSFRCAT, WCSMATCH, and WCSSEP to header
* Jul 26 1999 Always compute residuals so WCSMATCH and WCSSEP match WCS
* Jul 27 1999 Add WCSNREF, maximum possible matches
* Aug 26 1999 Handle true number return from search subroutines
* Aug 31 1999 Set image catalog name when only matching stars
* Sep 13 1999 Do all catalog searches through catread()
* Sep 15 1999 Fix improper uses of ng instead of nrg
* Sep 16 1999 Add zero distsort argument to catread() call
* Sep 29 1999 Add option to start with pre-matched stars
* Oct 22 1999 Change catread() to ctgread() to avoid system conflict
* Nov 23 1999 Free wcs only after it is used to set up iterate or recenter
*
* Feb 8 2000 If iterating, halve pixel tolerance on second pass
* Feb 11 2000 Print maximum number of matches with number matched
* Feb 15 2000 Drop maximum number of image stars
* Feb 15 2000 When iterating, reinitialize CD matrix if it's being fit
* Mar 1 2000 Modify residual output so = used instead of :
* Mar 1 2000 Add seperate option to tighten tolerances when iterating
* Mar 10 2000 Add proper motion arguments to ctgread()
* Mar 10 2000 Do not change WCS unless fitting
* Mar 13 2000 Use PropCat() to dind out whether catalog has proper motion
* Mar 15 2000 Add proper motion arguments to RASortStars() and ctgread()
* Mar 28 2000 Separate tolerance reducing iterations and other iterations
* May 26 2000 Set catalog number field size using CatNumLen()
* Jun 22 2000 Fix bug created in last update (found by J.-B. Marquette)
* Jul 12 2000 Add catalog data structre to ctgread() call
* Jul 25 2000 Pass address of star catalog data structure address
* Dec 6 2000 If no reference catalog is set, skip catalog fit
* Dec 6 2000 Drop static refcatname and setrefcat()
* Dec 18 2000 Always allocate proper motion arrays; clean up code after lint
* Dec 18 2000 Call ReadMatch() to read file of X/Y/RA/Dec matches
*
* Jan 8 2001 Add verbose flag to ReadMatch() call
* Jan 9 2001 Fix bug in FitMatch() call
* Jan 11 2001 All output except residuals to stderr
* Mar 1 2001 Fill in catalog name using CatName() if not set
*/
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