lsst.pipe.tasks ge54c72f270+6dd0a2cf65
Public Member Functions | Public Attributes | Static Public Attributes | List of all members
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsTask Class Reference
Inheritance diagram for lsst.pipe.tasks.processBrightStars.ProcessBrightStarsTask:

Public Member Functions

def __init__ (self, butler=None, initInputs=None, *args, **kwargs)
 
def applySkyCorr (self, calexp, skyCorr)
 
def extractStamps (self, inputExposure, refObjLoader=None)
 
def warpStamps (self, stamps, pixCenters)
 
def run (self, inputExposure, refObjLoader=None, dataId=None, skyCorr=None)
 
def runQuantum (self, butlerQC, inputRefs, outputRefs)
 

Public Attributes

 modelStampSize
 
 modelCenter
 

Static Public Attributes

 ConfigClass = ProcessBrightStarsConfig
 

Detailed Description

The description of the parameters for this Task are detailed in
:lsst-task:`~lsst.pipe.base.PipelineTask`.

Parameters
----------
initInputs : `Unknown`
*args
    Additional positional arguments.
**kwargs
    Additional keyword arguments.

Notes
-----
`ProcessBrightStarsTask` is used to extract, process, and store small
image cut-outs (or "postage stamps") around bright stars. It relies on
three methods, called in succession:

`extractStamps`
    Find bright stars within the exposure using a reference catalog and
    extract a stamp centered on each.
`warpStamps`
    Shift and warp each stamp to remove optical distortions and sample all
    stars on the same pixel grid.
`measureAndNormalize`
    Compute the flux of an object in an annulus and normalize it. This is
    required to normalize each bright star stamp as their central pixels
    are likely saturated and/or contain ghosts, and cannot be used.

Definition at line 179 of file processBrightStars.py.

Constructor & Destructor Documentation

◆ __init__()

def lsst.pipe.tasks.processBrightStars.ProcessBrightStarsTask.__init__ (   self,
  butler = None,
  initInputs = None,
args,
**  kwargs 
)

Definition at line 211 of file processBrightStars.py.

Member Function Documentation

◆ applySkyCorr()

def lsst.pipe.tasks.processBrightStars.ProcessBrightStarsTask.applySkyCorr (   self,
  calexp,
  skyCorr 
)
Apply correction to the sky background level.

Sky corrections can be generated with the 'skyCorrection.py'
executable in pipe_drivers. Because the sky model used by that
code extends over the entire focal plane, this can produce
better sky subtraction.
The calexp is updated in-place.

Parameters
----------
calexp : `lsst.afw.image.Exposure` or `lsst.afw.image.MaskedImage`
    Calibrated exposure.
skyCorr : `lsst.afw.math.backgroundList.BackgroundList` or `None`,
          optional
    Full focal plane sky correction, obtained by running
    `lsst.pipe.drivers.skyCorrection.SkyCorrectionTask`.

Definition at line 227 of file processBrightStars.py.

◆ extractStamps()

def lsst.pipe.tasks.processBrightStars.ProcessBrightStarsTask.extractStamps (   self,
  inputExposure,
  refObjLoader = None 
)
 Read position of bright stars within `inputExposure` from refCat
and extract them.

Parameters
----------
inputExposure : `afwImage.exposure.exposure.ExposureF`
    The image from which bright star stamps should be extracted.
refObjLoader : `lsst.meas.algorithms.ReferenceObjectLoader`, optional
    Loader to find objects within a reference catalog.

Returns
-------
result : `lsst.pipe.base.Struct`
    Results as a struct with attributes:

    ``starIms``
        List of stamps (`list`).
    ``pixCenters``
        List of corresponding coordinates to each star's center, in pixels (`list`).
    ``GMags``
        List of corresponding (Gaia) G magnitudes (`list`).
    ``gaiaIds``
        Array of corresponding unique Gaia identifiers (`np.ndarray`).

Definition at line 249 of file processBrightStars.py.

◆ run()

def lsst.pipe.tasks.processBrightStars.ProcessBrightStarsTask.run (   self,
  inputExposure,
  refObjLoader = None,
  dataId = None,
  skyCorr = None 
)
Identify bright stars within an exposure using a reference catalog,
extract stamps around each, then preprocess them. The preprocessing
steps are: shifting, warping and potentially rotating them to the same
pixel grid; computing their annular flux and normalizing them.

Parameters
----------
inputExposure : `afwImage.exposure.exposure.ExposureF`
    The image from which bright star stamps should be extracted.
refObjLoader : `lsst.meas.algorithms.ReferenceObjectLoader`, optional
    Loader to find objects within a reference catalog.
dataId : `dict` or `lsst.daf.butler.DataCoordinate`
    The dataId of the exposure (and detector) bright stars should be
    extracted from.
skyCorr : `lsst.afw.math.backgroundList.BackgroundList` or `None`,
          optional
    Full focal plane sky correction, obtained by running
    `lsst.pipe.drivers.skyCorrection.SkyCorrectionTask`.

Returns
-------
result :  `lsst.pipe.base.Struct`
    Results as a struct with attributes:

    ``brightStarStamps``
        (`bSS.BrightStarStamps`)

Definition at line 442 of file processBrightStars.py.

◆ runQuantum()

def lsst.pipe.tasks.processBrightStars.ProcessBrightStarsTask.runQuantum (   self,
  butlerQC,
  inputRefs,
  outputRefs 
)

Definition at line 515 of file processBrightStars.py.

◆ warpStamps()

def lsst.pipe.tasks.processBrightStars.ProcessBrightStarsTask.warpStamps (   self,
  stamps,
  pixCenters 
)
Warps and shifts all given stamps so they are sampled on the same
pixel grid and centered on the central pixel. This includes rotating
the stamp depending on detector orientation.

Parameters
----------
stamps : `collections.abc.Sequence`
             [`afwImage.exposure.exposure.ExposureF`]
    Image cutouts centered on a single object.
pixCenters : `collections.abc.Sequence` [`geom.Point2D`]
    Positions of each object's center (as obtained from the refCat),
    in pixels.

Returns
-------
result : `lsst.pipe.base.Struct`
    Results as a struct with attributes:

    ``warpedStars``
        List of stamps of warped stars (`list` of `afwImage.maskedImage.maskedImage.MaskedImage`).
    ``warpTransforms``
        List of the corresponding Transform from the initial star stamp
        to the common model grid (`list` of `afwGeom.TransformPoint2ToPoint2`).
    ``xy0s``
        List of coordinates of the bottom-left
        pixels of each stamp, before rotation (`list` of `geom.Point2I`).
    ``nb90Rots``
        The number of 90 degrees rotations required
        to compensate for detector orientation (`int`).

Definition at line 349 of file processBrightStars.py.

Member Data Documentation

◆ ConfigClass

lsst.pipe.tasks.processBrightStars.ProcessBrightStarsTask.ConfigClass = ProcessBrightStarsConfig
static

Definition at line 208 of file processBrightStars.py.

◆ modelCenter

lsst.pipe.tasks.processBrightStars.ProcessBrightStarsTask.modelCenter

Definition at line 222 of file processBrightStars.py.

◆ modelStampSize

lsst.pipe.tasks.processBrightStars.ProcessBrightStarsTask.modelStampSize

Definition at line 214 of file processBrightStars.py.


The documentation for this class was generated from the following file: