File CircularApertureFlux.h¶
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namespace
lsst
Class for a simple mapping implementing a generic AstrometryTransform.
Remove all non-astronomical counts from the Chunk Exposure’s pixels.
Forward declarations for lsst::utils::Cache
For details on the Cache class, see the Cache.h file.
It uses a template rather than a pointer so that the derived classes can use the specifics of the transform. The class simplePolyMapping overloads a few routines.
A base class for image defects
Numeric constants used by the Integrate.h integrator routines.
Compute Image Statistics
- Note
Gauss-Kronrod-Patterson quadrature coefficients for use in quadpack routine qng. These coefficients were calculated with 101 decimal digit arithmetic by L. W. Fullerton, Bell Labs, Nov 1981.
- Note
The Statistics class itself can only handle lsst::afw::image::MaskedImage() types. The philosophy has been to handle other types by making them look like lsst::afw::image::MaskedImage() and reusing that code. Users should have no need to instantiate a Statistics object directly, but should use the overloaded makeStatistics() factory functions.
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namespace
meas
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namespace
base
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class
CircularApertureFluxAlgorithm
: public lsst::meas::base::ApertureFluxAlgorithm Public Functions
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CircularApertureFluxAlgorithm
(Control const &ctrl, std::string const &name, afw::table::Schema &schema, daf::base::PropertySet &metadata)
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virtual void
measure
(afw::table::SourceRecord &record, afw::image::Exposure<float> const &exposure) const Measure the configured apertures on the given image.
Python plugins will delegate to this method.
- Parameters
[inout] record
: Record used to save outputs and retrieve positions.[in] exposure
: Image to be measured.
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class
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namespace