Loading [MathJax]/extensions/tex2jax.js
LSST Applications g0000d66e7c+ce78115f25,g0485b4d2cb+c8d56b10d4,g0fba68d861+fcbc158cd0,g1ec0fe41b4+3e153770da,g1fd858c14a+57ee4e1624,g2440f9efcc+8c5ae1fdc5,g35bb328faa+8c5ae1fdc5,g4d2262a081+1e04cc5a47,g53246c7159+8c5ae1fdc5,g55585698de+7a33f081c8,g56a49b3a55+b9d5cac73f,g60b5630c4e+7a33f081c8,g67b6fd64d1+035c836e50,g78460c75b0+7e33a9eb6d,g786e29fd12+668abc6043,g7ac00fbb6c+b938379438,g8352419a5c+8c5ae1fdc5,g8852436030+5ba78a36c9,g89139ef638+035c836e50,g94187f82dc+7a33f081c8,g989de1cb63+035c836e50,g9d31334357+7a33f081c8,g9f33ca652e+e34120223a,ga815be3f0b+911242149a,gabe3b4be73+8856018cbb,gabf8522325+21619da9f3,gb1101e3267+0b44b44611,gb89ab40317+035c836e50,gc91f06edcd+e59fb3c9bc,gcf25f946ba+5ba78a36c9,gd6cbbdb0b4+958adf5c1f,gde0f65d7ad+6c98dcc924,ge278dab8ac+83c63f4893,ge410e46f29+035c836e50,gf35d7ec915+97dd712d81,gf5e32f922b+8c5ae1fdc5,gf67bdafdda+035c836e50,gf6800124b1+1714c04baa,w.2025.19
LSST Data Management Base Package
All Classes Namespaces Files Functions Variables Typedefs Enumerations Enumerator Properties Friends Macros Modules Pages
lsst.meas.astrom.approximateWcs Namespace Reference

Classes

class  _MockTestCase
 

Functions

 approximateWcs (wcs, bbox, order=3, nx=20, ny=20, iterations=3, skyTolerance=0.001 *lsst.geom.arcseconds, pixelTolerance=0.02, useTanWcs=False)
 

Function Documentation

◆ approximateWcs()

lsst.meas.astrom.approximateWcs.approximateWcs ( wcs,
bbox,
order = 3,
nx = 20,
ny = 20,
iterations = 3,
skyTolerance = 0.001*lsst.geom.arcseconds,
pixelTolerance = 0.02,
useTanWcs = False )
Approximate an existing WCS as a TAN-SIP WCS

The fit is performed by evaluating the WCS at a uniform grid of points
within a bounding box.

Parameters
----------
wcs : `lsst.afw.geom.SkyWcs`
    wcs to approximate
bbox : `lsst.geom.Box2I`
    the region over which the WCS will be fit
order : `int`
    order of SIP fit
nx : `int`
    number of grid points along x
ny : `int`
    number of grid points along y
iterations : `int`
    number of times to iterate over fitting
skyTolerance : `lsst.geom.Angle`
    maximum allowed difference in world coordinates between
    input wcs and approximate wcs (default is 0.001 arcsec)
pixelTolerance : `float`
    maximum allowed difference in pixel coordinates between
    input wcs and approximate wcs (default is 0.02 pixels)
useTanWcs : `bool`
    send a TAN version of wcs to the fitter? It is documented to require that,
    but I don't think the fitter actually cares

Returns
-------
fitWcs : `lsst.afw.geom.SkyWcs`
    the fit TAN-SIP WCS

Definition at line 43 of file approximateWcs.py.

44 skyTolerance=0.001*lsst.geom.arcseconds, pixelTolerance=0.02, useTanWcs=False):
45 """Approximate an existing WCS as a TAN-SIP WCS
46
47 The fit is performed by evaluating the WCS at a uniform grid of points
48 within a bounding box.
49
50 Parameters
51 ----------
52 wcs : `lsst.afw.geom.SkyWcs`
53 wcs to approximate
54 bbox : `lsst.geom.Box2I`
55 the region over which the WCS will be fit
56 order : `int`
57 order of SIP fit
58 nx : `int`
59 number of grid points along x
60 ny : `int`
61 number of grid points along y
62 iterations : `int`
63 number of times to iterate over fitting
64 skyTolerance : `lsst.geom.Angle`
65 maximum allowed difference in world coordinates between
66 input wcs and approximate wcs (default is 0.001 arcsec)
67 pixelTolerance : `float`
68 maximum allowed difference in pixel coordinates between
69 input wcs and approximate wcs (default is 0.02 pixels)
70 useTanWcs : `bool`
71 send a TAN version of wcs to the fitter? It is documented to require that,
72 but I don't think the fitter actually cares
73
74 Returns
75 -------
76 fitWcs : `lsst.afw.geom.SkyWcs`
77 the fit TAN-SIP WCS
78 """
79 if useTanWcs:
80 crpix = wcs.getPixelOrigin()
81 crval = wcs.getSkyOrigin()
82 cdMatrix = wcs.getCdMatrix(crpix)
83 tanWcs = afwGeom.makeSkyWcs(crpix=crpix, crval=crval, cdMatrix=cdMatrix)
84 else:
85 tanWcs = wcs
86
87 # create a matchList consisting of a grid of points covering the bbox
88 refSchema = afwTable.SimpleTable.makeMinimalSchema()
89 refCoordKey = afwTable.CoordKey(refSchema["coord"])
90 refCat = afwTable.SimpleCatalog(refSchema)
91
92 sourceSchema = afwTable.SourceTable.makeMinimalSchema()
93 SingleFrameMeasurementTask(schema=sourceSchema) # expand the schema
94 sourceCentroidKey = afwTable.Point2DKey(sourceSchema["slot_Centroid"])
95
96 sourceCat = afwTable.SourceCatalog(sourceSchema)
97
98 matchList = []
99
100 bboxd = lsst.geom.Box2D(bbox)
101 for x in np.linspace(bboxd.getMinX(), bboxd.getMaxX(), nx):
102 for y in np.linspace(bboxd.getMinY(), bboxd.getMaxY(), ny):
103 pixelPos = lsst.geom.Point2D(x, y)
104 skyCoord = wcs.pixelToSky(pixelPos)
105
106 refObj = refCat.addNew()
107 refObj.set(refCoordKey, skyCoord)
108
109 source = sourceCat.addNew()
110 source.set(sourceCentroidKey, pixelPos)
111
112 matchList.append(afwTable.ReferenceMatch(refObj, source, 0.0))
113
114 # The TAN-SIP fitter is fitting x and y separately, so we have to iterate to make it converge
115 for indx in range(iterations):
116 sipObject = makeCreateWcsWithSip(matchList, tanWcs, order, bbox)
117 tanWcs = sipObject.getNewWcs()
118 fitWcs = sipObject.getNewWcs()
119
120 mockTest = _MockTestCase()
121 assertWcsAlmostEqualOverBBox(mockTest, wcs, fitWcs, bbox, maxDiffSky=skyTolerance,
122 maxDiffPix=pixelTolerance)
123
124 return fitWcs
A FunctorKey used to get or set celestial coordinates from a pair of lsst::geom::Angle keys.
Definition aggregates.h:292
A floating-point coordinate rectangle geometry.
Definition Box.h:413
std::shared_ptr< SkyWcs > makeSkyWcs(daf::base::PropertySet &metadata, bool strip=false)
Construct a SkyWcs from FITS keywords.
Definition SkyWcs.cc:521