LSST Applications g0d33ba9806+b932483eba,g0fba68d861+d53f2a615d,g1e78f5e6d3+1e869f36eb,g1ec0fe41b4+f536777771,g1fd858c14a+d5f4961c99,g35bb328faa+fcb1d3bbc8,g4af146b050+2e821d8f6b,g4d2262a081+b02c98aa00,g53246c7159+fcb1d3bbc8,g5a012ec0e7+b20b785ecb,g60b5630c4e+b932483eba,g67b6fd64d1+4086c0989b,g78460c75b0+2f9a1b4bcd,g786e29fd12+cf7ec2a62a,g7b71ed6315+fcb1d3bbc8,g87b7deb4dc+7d8c31d03d,g8852436030+a639f189fc,g89139ef638+4086c0989b,g9125e01d80+fcb1d3bbc8,g94187f82dc+b932483eba,g989de1cb63+4086c0989b,g9f33ca652e+898eabdf38,g9f7030ddb1+b068313d7a,ga2b97cdc51+b932483eba,ga44b1db4f6+2bd830756e,gabe3b4be73+1e0a283bba,gabf8522325+fa80ff7197,gb1101e3267+f4f1608365,gb58c049af0+f03b321e39,gb89ab40317+4086c0989b,gcf25f946ba+a639f189fc,gd6cbbdb0b4+af3c3595f5,gd9a9a58781+fcb1d3bbc8,gde0f65d7ad+4078fef7e5,ge278dab8ac+d65b3c2b70,ge410e46f29+4086c0989b,gf67bdafdda+4086c0989b,gfe06eef73a+6e83fc67a4,v29.0.0.rc5
LSST Data Management Base Package
|
Classes | |
class | Index2D |
Functions | |
coordFromVec (vec, defRA=None) | |
makeSkyPolygonFromBBox (bbox, wcs) | |
Variables | |
_TinyFloat = numpy.finfo(float).tiny | |
lsst.skymap.detail.utils.coordFromVec | ( | vec, | |
defRA = None ) |
Convert an ICRS cartesian vector to an ICRS `lsst.geom.SpherePoint`. Parameters ---------- vec : `list` of `float` An ICRS catesian vector. defRA : `lsst.geom.Angle` or None The RA to use if the vector is too near a pole; ignored if not near a pole. Raises ------ RuntimeError Raised if vec too near a pole and defRA is None.
Definition at line 34 of file utils.py.
lsst.skymap.detail.utils.makeSkyPolygonFromBBox | ( | bbox, | |
wcs ) |
Make an on-sky polygon from a bbox and a SkyWcs. Parameters ---------- bbox : `lsst.geom.Box2I` or `lsst.geom.Box2D` Bounding box of region, in pixel coordinates. wcs : `lsst.afw.geom.SkyWcs` Celestial WCS. Returns ------- polygon : `lsst.sphgeom.ConvexPolygon` On-sky region
Definition at line 61 of file utils.py.