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def | __init__ (self, *args, **kwargs) |
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def | run (self, skyInfo, tempExpRefList, imageScalerList, weightList, *args, **kwargs) |
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def | buildDifferenceImage (self, skyInfo, tempExpRefList, imageScalerList, weightList) |
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def | detectClip (self, exp, tempExpRefList) |
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def | detectClipBig (self, clipList, clipFootprints, clipIndices, detectionFootprints, maskClipValue, maskDetValue, coaddBBox) |
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Assemble a coadded image from a set of coadded temporary exposures,
being careful to clip & flag areas with potential artifacts.
In ``AssembleCoaddTask``, we compute the coadd as an clipped mean (i.e.,
we clip outliers). The problem with doing this is that when computing the
coadd PSF at a given location, individual visit PSFs from visits with
outlier pixels contribute to the coadd PSF and cannot be treated correctly.
In this task, we correct for this behavior by creating a new
``badMaskPlane`` 'CLIPPED'. We populate this plane on the input
coaddTempExps and the final coadd where
i. difference imaging suggests that there is an outlier and
ii. this outlier appears on only one or two images.
Such regions will not contribute to the final coadd. Furthermore, any
routine to determine the coadd PSF can now be cognizant of clipped regions.
Note that the algorithm implemented by this task is preliminary and works
correctly for HSC data. Parameter modifications and or considerable
redesigning of the algorithm is likley required for other surveys.
``SafeClipAssembleCoaddTask`` uses a ``SourceDetectionTask``
"clipDetection" subtask and also sub-classes ``AssembleCoaddTask``.
You can retarget the ``SourceDetectionTask`` "clipDetection" subtask
if you wish.
Notes
-----
The `lsst.pipe.base.cmdLineTask.CmdLineTask` interface supports a
flag ``-d`` to import ``debug.py`` from your ``PYTHONPATH``;
see `baseDebug` for more about ``debug.py`` files.
`SafeClipAssembleCoaddTask` has no debug variables of its own.
The ``SourceDetectionTask`` "clipDetection" subtasks may support debug
variables. See the documetation for `SourceDetectionTask` "clipDetection"
for further information.
Examples
--------
`SafeClipAssembleCoaddTask` assembles a set of warped ``coaddTempExp``
images into a coadded image. The `SafeClipAssembleCoaddTask` is invoked by
running assembleCoadd.py *without* the flag '--legacyCoadd'.
Usage of ``assembleCoadd.py`` expects a data reference to the tract patch
and filter to be coadded (specified using
'--id = [KEY=VALUE1[^VALUE2[^VALUE3...] [KEY=VALUE1[^VALUE2[^VALUE3...] ...]]')
along with a list of coaddTempExps to attempt to coadd (specified using
'--selectId [KEY=VALUE1[^VALUE2[^VALUE3...] [KEY=VALUE1[^VALUE2[^VALUE3...] ...]]').
Only the coaddTempExps that cover the specified tract and patch will be
coadded. A list of the available optional arguments can be obtained by
calling assembleCoadd.py with the --help command line argument:
.. code-block:: none
assembleCoadd.py --help
To demonstrate usage of the `SafeClipAssembleCoaddTask` in the larger
context of multi-band processing, we will generate the HSC-I & -R band
coadds from HSC engineering test data provided in the ci_hsc package.
To begin, assuming that the lsst stack has been already set up, we must
set up the obs_subaru and ci_hsc packages. This defines the environment
variable $CI_HSC_DIR and points at the location of the package. The raw
HSC data live in the ``$CI_HSC_DIR/raw`` directory. To begin assembling
the coadds, we must first
- ``processCcd``
process the individual ccds in $CI_HSC_RAW to produce calibrated exposures
- ``makeSkyMap``
create a skymap that covers the area of the sky present in the raw exposures
- ``makeCoaddTempExp``
warp the individual calibrated exposures to the tangent plane of the coadd</DD>
We can perform all of these steps by running
.. code-block:: none
$CI_HSC_DIR scons warp-903986 warp-904014 warp-903990 warp-904010 warp-903988
This will produce warped coaddTempExps for each visit. To coadd the
warped data, we call ``assembleCoadd.py`` as follows:
.. code-block:: none
assembleCoadd.py $CI_HSC_DIR/DATA --id patch=5,4 tract=0 filter=HSC-I \
--selectId visit=903986 ccd=16 --selectId visit=903986 ccd=22 --selectId visit=903986 ccd=23 \
--selectId visit=903986 ccd=100--selectId visit=904014 ccd=1 --selectId visit=904014 ccd=6 \
--selectId visit=904014 ccd=12 --selectId visit=903990 ccd=18 --selectId visit=903990 ccd=25 \
--selectId visit=904010 ccd=4 --selectId visit=904010 ccd=10 --selectId visit=904010 ccd=100 \
--selectId visit=903988 ccd=16 --selectId visit=903988 ccd=17 --selectId visit=903988 ccd=23 \
--selectId visit=903988 ccd=24
This will process the HSC-I band data. The results are written in
``$CI_HSC_DIR/DATA/deepCoadd-results/HSC-I``.
You may also choose to run:
.. code-block:: none
scons warp-903334 warp-903336 warp-903338 warp-903342 warp-903344 warp-903346 nnn
assembleCoadd.py $CI_HSC_DIR/DATA --id patch=5,4 tract=0 filter=HSC-R --selectId visit=903334 ccd=16 \
--selectId visit=903334 ccd=22 --selectId visit=903334 ccd=23 --selectId visit=903334 ccd=100 \
--selectId visit=903336 ccd=17 --selectId visit=903336 ccd=24 --selectId visit=903338 ccd=18 \
--selectId visit=903338 ccd=25 --selectId visit=903342 ccd=4 --selectId visit=903342 ccd=10 \
--selectId visit=903342 ccd=100 --selectId visit=903344 ccd=0 --selectId visit=903344 ccd=5 \
--selectId visit=903344 ccd=11 --selectId visit=903346 ccd=1 --selectId visit=903346 ccd=6 \
--selectId visit=903346 ccd=12
to generate the coadd for the HSC-R band if you are interested in following
multiBand Coadd processing as discussed in ``pipeTasks_multiBand``.
Definition at line 1382 of file assembleCoadd.py.
def lsst.pipe.tasks.assembleCoadd.SafeClipAssembleCoaddTask.detectClip |
( |
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self, |
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exp, |
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tempExpRefList |
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) |
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Detect clipped regions on an exposure and set the mask on the
individual tempExp masks.
Detect footprints in the difference image after smoothing the
difference image with a Gaussian kernal. Identify footprints that
overlap with one or two input ``coaddTempExps`` by comparing the
computed overlap fraction to thresholds set in the config. A different
threshold is applied depending on the number of overlapping visits
(restricted to one or two). If the overlap exceeds the thresholds,
the footprint is considered "CLIPPED" and is marked as such on the
coaddTempExp. Return a struct with the clipped footprints, the indices
of the ``coaddTempExps`` that end up overlapping with the clipped
footprints, and a list of new masks for the ``coaddTempExps``.
Parameters
----------
exp : `lsst.afw.image.Exposure`
Exposure to run detection on.
tempExpRefList : `list`
List of data reference to tempExp.
Returns
-------
result : `lsst.pipe.base.Struct`
Result struct with components:
- ``clipFootprints``: list of clipped footprints.
- ``clipIndices``: indices for each ``clippedFootprint`` in
``tempExpRefList``.
- ``clipSpans``: List of dictionaries containing spanSet lists
to clip. Each element contains the new maskplane name
("CLIPPED") as the key and list of ``SpanSets`` as the value.
- ``detectionFootprints``: List of DETECTED/DETECTED_NEGATIVE plane
compressed into footprints.
Definition at line 1608 of file assembleCoadd.py.