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In the next major release of the LSST stack, the system for measuring the properties of sources will be replaced by a new one, housed mostly in the new
meas_base package. In addition to providing new
Task classes and a new plugin interface for measurement algorithms, this overhaul also includes changes to the schemas of the catalogs produced by the measurement framework. The new framework will not be entirely complete as of the next release, but it will have sufficient functionality to replace the old framework as the default. The old system will remain available via config on the S14 final release, but will be removed entirely before the W15 release.
The main entry point for the new measurement framework is the new
SingleFrameMeasurementTask class (in meas_base), which is intended as an almost drop-in replacement for the current
SourceMeasurementTask (in meas_algorithms). It's not drop-in replacement, because it has different plugins, a slightly different slot system, and an entirely different output schema - so we will use it everywhere SourceMeasurementTask was used before, but many other additional configuration settings need to be modified when retargeting the measurement task to keep it all working. We've provided configuration files to make that easy, as described in the next section.
SingleFrameMeasurementTask combines the work previously done by two classes, the old
SourceMeasurementTask and the C++
MeasureSources class. It initializes the plugins (which determines the schema) in its constructor, then invokes the plugins on each source in the image, replacing neighbors with noise as it does so (this is delegated to the
NoiseReplacer class, which replaces the
ReplaceWithNoiseTask subtask). Unlike
SingleFrameMeasurementTask does not do forced photometry (see below). Sources are also processed in a slightly different order (see Simultaneous Multi-Object Measurement).
For the present, you will continue to support the measurement.py task in meas_algorithms. The measurement task used by processCcd and processCoadd is controlled by configurations items in CalibrateConfig and ProcessImageConfig, and can be retargeted back to the original meas_algorithms framework using the following python code:
from lsst.meas.algorithms.measurement import SourceMeasurementTask
Please note that the original framework writes tables with version=0 schemata, and expects the plugins and fieldnames to use the old naming conventions. For example, you must refer to the SdssCentroid plugin as 'centroid.sdss' and the value it stores in the output table will be afw.geom.PointD type with the name 'centroid.sdss'.
Some care has been taken to make all of the tasks called by processImage sensitive to which measurement framework and schema version are in use, so that the pipeline will work with either measurement task. However, the developer should be careful when accessing or adding fields to the schemas to know which measurement task and which naming conventions are in effect. For new code, we encourage the use of the meas_base measurement framework and schema version=1 tables.
NOTE: If you are reading this document prior to the changeover to the end of Summer 14, just the opposite instructions will hold for using the New Framework. That is, you must retargetted the above 3 tasks using the SingleFrameMeasurementTask which resides in lsst.meas.base.sfm.
The changes to
Schema objects to support the new measurement framework are handled by a new versioning mechanism, which allows the old behavior (necessary for the old framework) to coexist with the new behavior in the stack. A
Schema with version=0 corresponds to one appropriate for use with the old
SourceMeasurementTask, while version>0 corresponds to
SingleFrameMeasurementTask and the new forced photometry tasks. Here are the differences between versions:
Schema::operatoroperator when joining pieces of field names.
In version>0, we have stronger naming convention for fields generating by plugin algorithms, which tie the plugin name and location to its outputs. These conventions are used by the
meas_baseuse "base" as their prefix, while those in
ip_diffimwould use simply "diffim". The "class" part of the name is simply the name of the class that defines the algorithm, minus any explict "Plugin" or "Algorithm" suffix. For instance, the field name prefix used by
SdssShapeAlgorithmclass would be "base_SdssShape".
We have added an alias feature to the
Schema class, via an
AliasMap object it holds. Aliases are handled simply as an extra stage in
Key lookup - when a
Key is requested via a string, its beginning is compared against all aliases to see if it should be replaced. Partial replacements are allowed, but only at the beginning, and multiple replacements are not. For example, if the
AliasMap includes the mapping "slot_PsfFlux"->"base_PsfFlux", then a Key lookup on "slot_PsfFlux_flux" will resolve to "base_PsfFlux_flux", but a lookup on "r_slot_PsfFlux_flux" will not be affected. Because
Key lookup happens implicitly when getting a value from a record via string, this makes it even more important to do
Key lookup once in advance rather than use a string to access the same value repeatedly.
The alias system is available for both version 0 and version > 0 tables, and is now used to define the slot mechanism in SourceTable/SourceRecord/SourceCatalog in both cases; each slot corresponds to a predefined field name prefix that is mapped to an actual measurement via an alias. These predefined names are the name of the slot, starting with a capital letter (e.g. "PsfFlux", "Centroid"), prefixed with "slot_" (or "slot." for version 0). For instance, a typical AliasMap containing slot definitions would have the following mappings for version 1:
Slot definitions are now persisted simply as aliases, with slots saved via older versions of the stack translated into aliases when read from disk. Changing one of these aliases in an
AliasMap attached to a
SourceTable will notify the table that slots have changed and the cached Keys that correspond to them must be updated (in fact, the old slot definers, such as
SourceTable::definePsfFlux() are now implemented by simply changing the alias and letting the notification callback do its work).
Note that this means that slot values can now be accessed via string, just like any normal measurement.
While the old SourceMeasurementTask processed sources in the order set by the catalog it was given, SingleFrameMeasurementTask and ForcedMeasurementTask instead iterate over deblend families; within each family, the children are processed individually first, followed by the parent. After the individual source measurements, plugins are then given an opportunity to measure all the children at once at once, using an interface that was not present in the old framework, using the same pixel values used in the parent measurement but writing outputs to per-child records. This allows us to support plugins that fit multiple objects simultaneously (possibly using the earlier non-simultaneous measurements as input).
This will likely provide the easiest route to properly-deblended forced photometry; rather than attempt to transform deblender outputs from frame to frame, or rely on a full, multi-epoch deblender, we can simply fit families simultaneously in forced mode. This does not, of course, address the problem of consistent multi-band detection or deblending.
Currently we have no plugins that use this API. Of our current algorihtms, only the PSF flux and the galaxy model flux are likely to ever be usable in this mode.
For issues that we expect to complete before the S14 release, please see the epics below. These include improvements to error-handling, miscellaneous code cleanups, FunctorKeys for array fields, and a multiple-aperture photometry plugin.
For issues that we expect to complete in W15, please these epics for a complete list. These include reimplementing aperture corrections, reimplemented database ingest, converting extension algorithms to the new plugin system, and removing the old measurement framework and all remaining code that depends on it.