LSST Applications
21.0.0-172-gfb10e10a+18fedfabac,22.0.0+297cba6710,22.0.0+80564b0ff1,22.0.0+8d77f4f51a,22.0.0+a28f4c53b1,22.0.0+dcf3732eb2,22.0.1-1-g7d6de66+2a20fdde0d,22.0.1-1-g8e32f31+297cba6710,22.0.1-1-geca5380+7fa3b7d9b6,22.0.1-12-g44dc1dc+2a20fdde0d,22.0.1-15-g6a90155+515f58c32b,22.0.1-16-g9282f48+790f5f2caa,22.0.1-2-g92698f7+dcf3732eb2,22.0.1-2-ga9b0f51+7fa3b7d9b6,22.0.1-2-gd1925c9+bf4f0e694f,22.0.1-24-g1ad7a390+a9625a72a8,22.0.1-25-g5bf6245+3ad8ecd50b,22.0.1-25-gb120d7b+8b5510f75f,22.0.1-27-g97737f7+2a20fdde0d,22.0.1-32-gf62ce7b1+aa4237961e,22.0.1-4-g0b3f228+2a20fdde0d,22.0.1-4-g243d05b+871c1b8305,22.0.1-4-g3a563be+32dcf1063f,22.0.1-4-g44f2e3d+9e4ab0f4fa,22.0.1-42-gca6935d93+ba5e5ca3eb,22.0.1-5-g15c806e+85460ae5f3,22.0.1-5-g58711c4+611d128589,22.0.1-5-g75bb458+99c117b92f,22.0.1-6-g1c63a23+7fa3b7d9b6,22.0.1-6-g50866e6+84ff5a128b,22.0.1-6-g8d3140d+720564cf76,22.0.1-6-gd805d02+cc5644f571,22.0.1-8-ge5750ce+85460ae5f3,master-g6e05de7fdc+babf819c66,master-g99da0e417a+8d77f4f51a,w.2021.48
LSST Data Management Base Package
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Public Member Functions | |
def | __init__ (self, dataIds=None, refCats=None, butler=None, **kwargs) |
def | getPixelBoxCatalog (self, bbox, wcs, filterList, epoch=None, bboxToSpherePadding=None) |
def | getSkyCircleCatalog (self, center, radius, filterList, epoch=None, catalogFormat='numpy') |
Public Attributes | |
refObjLoader | |
Static Public Attributes | |
ConfigClass = LoadReferenceCatalogConfig | |
Load multi-band reference objects from a reference catalog. Parameters ---------- dataIds : iterable of `lsst.daf.butler.dataId`, optional An iterable object of dataIds which point to reference catalogs in a Gen3 repository. Required for Gen3. refCats : iterable of `lsst.daf.butler.DeferredDatasetHandle`, optional An iterable object of dataset refs for reference catalogs in a Gen3 repository. Required for Gen3. butler : `lsst.daf.persistence.Butler`, optional A Gen2 butler. Required for Gen2.
Definition at line 77 of file loadReferenceCatalog.py.
def lsst.pipe.tasks.loadReferenceCatalog.LoadReferenceCatalogTask.__init__ | ( | self, | |
dataIds = None , |
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refCats = None , |
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butler = None , |
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** | kwargs | ||
) |
Definition at line 94 of file loadReferenceCatalog.py.
def lsst.pipe.tasks.loadReferenceCatalog.LoadReferenceCatalogTask.getPixelBoxCatalog | ( | self, | |
bbox, | |||
wcs, | |||
filterList, | |||
epoch = None , |
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bboxToSpherePadding = None |
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) |
Get a multi-band reference catalog by specifying a bounding box and WCS. The catalog will be in `numpy.ndarray`, with positions proper-motion corrected to "epoch" (if specified, and if the reference catalog has proper motions); sources cut on a reference selector (if "config.doReferenceSelection = True"); and color-terms applied (if "config.doApplyColorTerms = True"). The format of the reference catalog will be of the format: dtype = [('ra', 'np.float64'), ('dec', 'np.float64'), ('refMag', 'np.float32', (len(filterList), )), ('refMagErr', 'np.float32', (len(filterList), ))] Reference magnitudes (AB) and errors will be 99 for non-detections in a given band. Parameters ---------- bbox : `lsst.geom.Box2I` Box which bounds a region in pixel space. wcs : `lsst.afw.geom.SkyWcs` Wcs object defining the pixel to sky (and reverse) transform for the supplied bbox. filterList : `List` [ `str` ] List of camera physicalFilter names to retrieve magnitudes. epoch : `astropy.time.Time`, optional Epoch to which to correct proper motion and parallax (if available), or `None` to not apply such corrections. bboxToSpherePadding : `int`, optional Padding to account for translating a set of corners into a spherical (convex) boundary that is certain to encompass the entire area covered by the bbox. Returns ------- refCat : `numpy.ndarray` Reference catalog.
Definition at line 114 of file loadReferenceCatalog.py.
def lsst.pipe.tasks.loadReferenceCatalog.LoadReferenceCatalogTask.getSkyCircleCatalog | ( | self, | |
center, | |||
radius, | |||
filterList, | |||
epoch = None , |
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catalogFormat = 'numpy' |
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) |
Get a multi-band reference catalog by specifying a center and radius. The catalog will be in `numpy.ndarray`, with positions proper-motion corrected to "epoch" (if specified, and if the reference catalog has proper motions); sources cut on a reference selector (if "config.doReferenceSelection = True"); and color-terms applied (if "config.doApplyColorTerms = True"). The format of the reference catalog will be of the format: dtype = [('ra', 'np.float64'), ('dec', 'np.float64'), ('refMag', 'np.float32', (len(filterList), )), ('refMagErr', 'np.float32', (len(filterList), ))] Reference magnitudes (AB) and errors will be 99 for non-detections in a given band. Parameters ---------- center : `lsst.geom.SpherePoint` Point defining the center of the circular region. radius : `lsst.geom.Angle` Defines the angular radius of the circular region. filterList : `List` [ `str` ] List of camera physicalFilter names to retrieve magnitudes. epoch : `astropy.time.Time`, optional Epoch to which to correct proper motion and parallax (if available), or `None` to not apply such corrections. Parameters ---------- refCat : `numpy.ndarray` Reference catalog.
Definition at line 172 of file loadReferenceCatalog.py.
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static |
Definition at line 91 of file loadReferenceCatalog.py.
lsst.pipe.tasks.loadReferenceCatalog.LoadReferenceCatalogTask.refObjLoader |
Definition at line 98 of file loadReferenceCatalog.py.