| /dports/astro/py-astlib/astLib-0.11.7/PyWCSTools/wcssubs-3.9.5/ |
| H A D | wcs.i | 23 …ble cra, double cdec, double secpix, int xrpix, int yrpix, int nxpix, int nypix, double rotate, in…
24 struct WorldCoor *wcskinit(int nxpix, int nypix, char *ctype1, char *ctype2, double crpix1, double …
60 double nypix; /* Number of pixels in Y-dimension of image */ member
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| H A D | wcsinit.c | 313 wcs->nypix = 0;
314 hgetr8 (hstring, "NAXIS2", &wcs->nypix);
315 if (wcs->nypix < 1)
316 hgetr8 (hstring, "IMAGEH", &wcs->nypix);
317 if (naxes > 1 && wcs->nypix < 1) {
337 else if (i == 1 && wcs->nypix > 1) {
340 j = wcs->nypix;
692 if (cdelt2 == 0.0 && wcs->nypix > 1)
907 wcs->crpix[1] = 0.5 * wcs->nypix;
987 wcs->crpix[1] = 0.5 + (wcs->nypix * 0.5);
[all …]
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| H A D | wcs.c | 143 int nypix; /* Number of pixels along y-axis */
166 wcs->nypix = nypix;
268 wcs->nypix = naxis2;
1061 if (wcs->nxpix < 1.5 || wcs->nypix < 1.5) {
1219 ypix = 0.5 * wcs->nypix;
1247 (void) pix2wcs (wcs,xpix,wcs->nypix,&xpos2,&ypos2);
1264 secpixh = height / (wcs->nypix - 1.0);
1340 ycpix = (0.5 * wcs->nypix) + 0.5;
1361 ypix = wcs->nypix + 0.5;
1400 (void) pix2wcs (wcs,1.0,wcs->nypix,&xpos2,&ypos2);
[all …]
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| H A D | wcs.h | 64 double nypix; /* Number of pixels in Y-dimension of image */ member
373 int nypix, /* Number of pixels along y-axis */
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| H A D | dsspos.c | 299 if (*ypix < 0.5 || *ypix > wcs->nypix+0.5)
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| H A D | platepos.c | 287 if (*ypix < 0.5 || *ypix > wcs->nypix+0.5)
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| H A D | wcs_wrap.c | 4678 if (arg1) (arg1)->nypix = arg2; in _wrap_WorldCoor_nypix_set()
4701 result = (double) ((arg1)->nypix); in _wrap_WorldCoor_nypix_get()
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| /dports/astro/stellarium/stellarium-0.21.3/util/ |
| H A D | genSkyTiles.py | 131 nypix=int(xmp.get_array_item(ns, 'Spatial.ReferenceDimension', 2).keys()[0])
155 header.update('NAXIS2', nypix)
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| /dports/astro/p5-Starlink-AST/Starlink-AST-1.05/ast/ |
| H A D | dssmap.h | 172 double nypix; /* Number of pixels in Y-dimension of image */ member
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| /dports/astro/oskar/OSKAR-2.8.0/extern/cfitsio/ |
| H A D | quantize.c | 84 int fits_quantize_float (long row, float fdata[], long nxpix, long nypix, int nullcheck, in fits_quantize_float() argument
121 nx = nxpix * nypix; in fits_quantize_float()
131 FnNoise5_float(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_float()
160 FnNoise3_float(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_float()
273 int fits_quantize_double (long row, double fdata[], long nxpix, long nypix, int nullcheck, in fits_quantize_double() argument
310 nx = nxpix * nypix; in fits_quantize_double()
320 FnNoise5_double(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_double()
349 FnNoise3_double(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_double()
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| /dports/astro/cfitsio/cfitsio-3.49/ |
| H A D | quantize.c | 84 int fits_quantize_float (long row, float fdata[], long nxpix, long nypix, int nullcheck, in fits_quantize_float() argument
121 nx = nxpix * nypix; in fits_quantize_float()
131 FnNoise5_float(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_float()
160 FnNoise3_float(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_float()
273 int fits_quantize_double (long row, double fdata[], long nxpix, long nypix, int nullcheck, in fits_quantize_double() argument
310 nx = nxpix * nypix; in fits_quantize_double()
320 FnNoise5_double(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_double()
349 FnNoise3_double(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_double()
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| /dports/science/healpix/Healpix_3.50/src/healpy/cfitsio/ |
| H A D | quantize.c | 84 int fits_quantize_float (long row, float fdata[], long nxpix, long nypix, int nullcheck, in fits_quantize_float() argument
121 nx = nxpix * nypix; in fits_quantize_float()
131 FnNoise5_float(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_float()
160 FnNoise3_float(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_float()
273 int fits_quantize_double (long row, double fdata[], long nxpix, long nypix, int nullcheck, in fits_quantize_double() argument
309 nx = nxpix * nypix; in fits_quantize_double()
319 FnNoise5_double(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_double()
348 FnNoise3_double(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_double()
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| /dports/astro/py-astropy/astropy-5.0/cextern/cfitsio/lib/ |
| H A D | quantize.c | 84 int fits_quantize_float (long row, float fdata[], long nxpix, long nypix, int nullcheck, in fits_quantize_float() argument
121 nx = nxpix * nypix; in fits_quantize_float()
131 FnNoise5_float(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_float()
160 FnNoise3_float(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_float()
273 int fits_quantize_double (long row, double fdata[], long nxpix, long nypix, int nullcheck, in fits_quantize_double() argument
310 nx = nxpix * nypix; in fits_quantize_double()
320 FnNoise5_double(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_double()
349 FnNoise3_double(fdata, nxpix, nypix, nullcheck, in_null_value, &ngood, in fits_quantize_double()
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| /dports/astro/py-astlib/astLib-0.11.7/PyWCSTools/ |
| H A D | wcs.py | 194 if _newclass:nypix = _swig_property(_wcs.WorldCoor_nypix_get, _wcs.WorldCoor_nypix_set)
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| /dports/astro/astrometry/astrometry.net-0.85/util/ |
| H A D | anwcs.c | 161 return wcs->nypix; in wcstools_imageh()
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| /dports/astro/stellarsolver/stellarsolver-1.8/stellarsolver/astrometry/util/ |
| H A D | anwcs.c | 161 return wcs->nypix; in wcstools_imageh()
|