price@price-laptop:~/LSST/obs/subaru (tickets/DM-7889=) $ git sub
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commit 0e9fb31f1d7ae0a4ab85401a6c9c979b3364cbcc
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Author: Paul Price <price@astro.princeton.edu>
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Date: Fri Nov 4 14:17:45 2016 -0400
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activate measurements used in s16a production afterburner
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The HSC s16a production's afterburner included two measurements features
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which have been ported to LSST: measurement on the undeblended image (to
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allow potentially useful measurements where the deblender fails, and to
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compare with software that doesn't use a deblender), and measurement of
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convolved fluxes (to provide fluxes in multiple bands with a common
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seeing, e.g., for photometric redshifts). This patch activates these
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features for HSC and Suprime-Cam.
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config/convolvedFluxes.py | 9 +++++++++
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config/forcedPhotCoadd.py | 27 +++++++++++++++++++++++++++
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config/measureCoaddSources.py | 1 +
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config/processCcd.py | 6 ++++++
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4 files changed, 43 insertions(+)
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price@price-laptop:~/LSST/meas/extensions/convolved (tickets/DM-7889=) $ git subcommit 5c904dca6e5f32c4c3a3f1b31e4e5afa44a42a43
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Author: Paul Price <price@astro.princeton.edu>
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Date: Mon Nov 7 20:49:48 2016 -0600
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wrap ConvolvedFluxPlugin to allow use in forced measurement
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Change the ConvolvedFluxPlugin class into a base class that we then
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wrap with the appropriate plugin base class. There's also a little
|
bit of fiddling required to give the forced measurement a slightly
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different signature.
|
|
In order to do the forced measurement, we need to add transformation
|
from the reference frame to the measurement frame. Since we're
|
already doing forced measurement (center is provided, aperture shape
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and radius are provided), moved the calculation into a 'measureForced'
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method, and have 'measure' call that with a null transformation.
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Modified the test to check that forced measurement also works.
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python/lsst/meas/extensions/convolved/convolved.py | 203 ++++++++++++++-------
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tests/test_convolved.py | 76 ++++++--
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2 files changed, 201 insertions(+), 78 deletions(-)
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price@price-laptop:~/LSST/meas/base (tickets/DM-7889=) $ git sub
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commit 7d67323726849bf986d3c0a7261dbdd8e32e2c94
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Author: Paul Price <price@astro.princeton.edu>
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Date: Mon Nov 7 20:47:05 2016 -0600
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refactor undeblended measurement into BaseMeasurementTask
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This makes it available in the ForcedMeasurementTask as well as
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SingleFrameMeasurementTask. Unfortunately, the actual measurement
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iteration cannot live in BaseMeasurementTask because the forced
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measurement requires iterating through two catalogs in sync, while
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the single frame measurement only has one.
|
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python/lsst/meas/base/baseMeasurement.py | 24 ++++++++++++++++++++++++
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python/lsst/meas/base/forcedMeasurement.py | 13 +++++++++++++
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python/lsst/meas/base/sfm.py | 30 +++++++-----------------------
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3 files changed, 44 insertions(+), 23 deletions(-)
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price@price-laptop:~/LSST/meas/extensions/photometryKron (tickets/DM-7889=) $ git sub
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commit dab9e3e939b0b34bcadced5fd5a9faa493ca8eda
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Author: Paul Price <price@astro.princeton.edu>
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Date: Tue Nov 15 21:25:37 2016 -0500
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make source of Kron radius configurable for forced mode
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The source of the Kron radius was hard-wired to _name+"_radius",
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but this doesn't work for the undeblended version (which has a
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different name that doesn't exist in the reference catalog).
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Making the source configurable solves this problem.
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include/lsst/meas/extensions/photometryKron.h | 5 ++++-
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src/KronPhotometry.cc | 2 +-
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2 files changed, 5 insertions(+), 2 deletions(-)
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This was a LOT more work than I was expecting because, in addition to adding a configuration file, it also required:
Lauren MacArthur, would you mind having a look at these, please? If you feel it's a bit much, we can split it up.
price@price-laptop:~/LSST/obs/subaru (tickets/DM-7889=) $ git sub
commit 0e9fb31f1d7ae0a4ab85401a6c9c979b3364cbcc
Author: Paul Price <price@astro.princeton.edu>
Date: Fri Nov 4 14:17:45 2016 -0400
activate measurements used in s16a production afterburner
The HSC s16a production's afterburner included two measurements features
which have been ported to LSST: measurement on the undeblended image (to
allow potentially useful measurements where the deblender fails, and to
compare with software that doesn't use a deblender), and measurement of
convolved fluxes (to provide fluxes in multiple bands with a common
seeing, e.g., for photometric redshifts). This patch activates these
features for HSC and Suprime-Cam.
config/convolvedFluxes.py | 9 +++++++++
config/forcedPhotCoadd.py | 27 +++++++++++++++++++++++++++
config/measureCoaddSources.py | 1 +
config/processCcd.py | 6 ++++++
4 files changed, 43 insertions(+)
price@price-laptop:~/LSST/meas/extensions/convolved (tickets/DM-7889=) $ git subcommit 5c904dca6e5f32c4c3a3f1b31e4e5afa44a42a43
Author: Paul Price <price@astro.princeton.edu>
Date: Mon Nov 7 20:49:48 2016 -0600
wrap ConvolvedFluxPlugin to allow use in forced measurement
Change the ConvolvedFluxPlugin class into a base class that we then
wrap with the appropriate plugin base class. There's also a little
bit of fiddling required to give the forced measurement a slightly
different signature.
In order to do the forced measurement, we need to add transformation
from the reference frame to the measurement frame. Since we're
already doing forced measurement (center is provided, aperture shape
and radius are provided), moved the calculation into a 'measureForced'
method, and have 'measure' call that with a null transformation.
Modified the test to check that forced measurement also works.
python/lsst/meas/extensions/convolved/convolved.py | 203 ++++++++++++++-------
tests/test_convolved.py | 76 ++++++--
2 files changed, 201 insertions(+), 78 deletions(-)
price@price-laptop:~/LSST/meas/base (tickets/DM-7889=) $ git sub
commit 7d67323726849bf986d3c0a7261dbdd8e32e2c94
Author: Paul Price <price@astro.princeton.edu>
Date: Mon Nov 7 20:47:05 2016 -0600
refactor undeblended measurement into BaseMeasurementTask
This makes it available in the ForcedMeasurementTask as well as
SingleFrameMeasurementTask. Unfortunately, the actual measurement
iteration cannot live in BaseMeasurementTask because the forced
measurement requires iterating through two catalogs in sync, while
the single frame measurement only has one.
python/lsst/meas/base/baseMeasurement.py | 24 ++++++++++++++++++++++++
python/lsst/meas/base/forcedMeasurement.py | 13 +++++++++++++
python/lsst/meas/base/sfm.py | 30 +++++++-----------------------
3 files changed, 44 insertions(+), 23 deletions(-)
price@price-laptop:~/LSST/meas/extensions/photometryKron (tickets/DM-7889=) $ git sub
commit dab9e3e939b0b34bcadced5fd5a9faa493ca8eda
Author: Paul Price <price@astro.princeton.edu>
Date: Tue Nov 15 21:25:37 2016 -0500
make source of Kron radius configurable for forced mode
The source of the Kron radius was hard-wired to _name+"_radius",
but this doesn't work for the undeblended version (which has a
different name that doesn't exist in the reference catalog).
Making the source configurable solves this problem.
include/lsst/meas/extensions/photometryKron.h | 5 ++++-
src/KronPhotometry.cc | 2 +-
2 files changed, 5 insertions(+), 2 deletions(-)