/dports/astro/astrometry/astrometry.net-0.85/util/ |
H A D | sip.c | 109 tan_pixelxy2xyzarr(&(sip->wcstan), U, V, xyz); in sip_pixelxy2xyzarr() 112 tan_pixelxy2xyzarr(&(sip->wcstan), px, py, xyz); in sip_pixelxy2xyzarr() 118 tan_pixelxy2xyzarr(tan, px, py, xyz); in tan_pixelxy2radec() 233 void tan_pixelxy2xyzarr(const tan_t* tan, double px, double py, double *xyz) in tan_pixelxy2xyzarr() function
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H A D | tpv.c | 125 tan_pixelxy2xyzarr(&(tpv->wcstan), U, V, xyz); in tpv_pixelxy2xyzarr()
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H A D | fit-wcs.c | 736 tan_pixelxy2xyzarr(tanin, crpix[0], crpix[1], crxyz); in fit_tan_wcs_solve()
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H A D | util.i | 1691 tan_pixelxy2xyzarr($self, 0.5+$self->imagew/2.0, 0.5+$self->imageh/2.0, xyz); 1698 tan_pixelxy2xyzarr($self, x, y, xyz);
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H A D | c.py | 1588 def tan_pixelxy2xyzarr(tan, px, py, xyz): function 1589 return _util.tan_pixelxy2xyzarr(tan, px, py, xyz)
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H A D | util.py | 1588 def tan_pixelxy2xyzarr(tan, px, py, xyz): function 1589 return _util.tan_pixelxy2xyzarr(tan, px, py, xyz)
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H A D | util_wrap.c | 4197 tan_pixelxy2xyzarr(self, 0.5+self->imagew/2.0, 0.5+self->imageh/2.0, xyz); in tan_t_xyzcenter() 4204 tan_pixelxy2xyzarr(self, x, y, xyz); in tan_t_pixelxy2xyz() 26064 tan_pixelxy2xyzarr((tan_t const *)arg1,arg2,arg3,arg4); in _wrap_tan_pixelxy2xyzarr()
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/dports/astro/stellarsolver/stellarsolver-1.8/stellarsolver/astrometry/util/ |
H A D | sip.c | 108 tan_pixelxy2xyzarr(&(sip->wcstan), U, V, xyz); in sip_pixelxy2xyzarr() 111 tan_pixelxy2xyzarr(&(sip->wcstan), px, py, xyz); in sip_pixelxy2xyzarr() 117 tan_pixelxy2xyzarr(tan, px, py, xyz); in tan_pixelxy2radec() 221 void tan_pixelxy2xyzarr(const tan_t* tan, double px, double py, double *xyz) in tan_pixelxy2xyzarr() function
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H A D | fit-wcs.c | 736 tan_pixelxy2xyzarr(tanin, crpix[0], crpix[1], crxyz); in fit_tan_wcs_solve()
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/dports/astro/astrometry/astrometry.net-0.85/include/astrometry/ |
H A D | sip.h | 182 void tan_pixelxy2xyzarr(const tan_t* tan, double px, double py, double *xyz);
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/dports/astro/stellarsolver/stellarsolver-1.8/stellarsolver/astrometry/include/astrometry/ |
H A D | sip.h | 182 void tan_pixelxy2xyzarr(const tan_t* tan, double px, double py, double *xyz);
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/dports/astro/astrometry/astrometry.net-0.85/solver/ |
H A D | whynot.c | 950 tan_pixelxy2xyzarr(&wcs, W/2.0, H/2.0, mo.center); in main() 951 tan_pixelxy2xyzarr(&wcs, 0, 0, llxyz); in main()
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H A D | solver.c | 412 tan_pixelxy2xyzarr(tan, cx, cy, mo->center); in set_center_and_radius() 413 tan_pixelxy2xyzarr(tan, lx, ly, xyz); in set_center_and_radius()
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/dports/astro/stellarsolver/stellarsolver-1.8/stellarsolver/astrometry/blind/ |
H A D | solver.c | 407 tan_pixelxy2xyzarr(tan, cx, cy, mo->center); in set_center_and_radius() 408 tan_pixelxy2xyzarr(tan, lx, ly, xyz); in set_center_and_radius()
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