JointcalConfig¶
-
class
lsst.jointcal.
JointcalConfig
¶ Bases:
lsst.pex.config.Config
Config for JointcalTask
Attributes Summary
allowLineSearch
Allow a line search during minimization, if it is reasonable for the model (models with a significant non-linear component, e.g. applyColorTerms
Apply photometric color terms to reference stars?Requires that colorterms be set to a ColortermLibrary ( bool
, defaultFalse
)astrometryChipOrder
Order of the per-chip transform for the constrained astrometry model. astrometryDoRankUpdate
Do the rank update step during minimization (should not change the astrometry fit). astrometryModel
Type of model to fit to astrometry ( str
, default'constrained'
)astrometryRefObjLoader
Reference object loader for astrometric fit ( ConfigurableInstance
, default<class 'lsst.meas.algorithms.loadIndexedReferenceObjects.LoadIndexedReferenceObjectsConfig'>
)astrometryReferenceSelector
How to down-select the loaded astrometry reference catalog. astrometrySimpleOrder
Polynomial order for fitting the simple astrometry model. astrometryVisitOrder
Order of the per-visit transform for the constrained astrometry model. coaddName
Type of coadd, typically deep or goodSeeing ( str
, default'deep'
)colorterms
Library of photometric reference catalog name to color term dict. doAstrometry
Fit astrometry and write the fitted result. doPhotometry
Fit photometry and write the fitted result. history
matchCut
Matching radius between fitted and reference stars (arcseconds) ( float
, default3.0
)maxAstrometrySteps
Maximum number of minimize iterations to take when fitting photometry. maxPhotometrySteps
Maximum number of minimize iterations to take when fitting photometry. minMeasuredStarsPerCcd
Minimum number of measuredStars per ccdImage before printing warnings ( int
, default100
)minMeasurements
Minimum number of associated measured stars for a fitted star to be included in the fit ( int
, default2
)minRefStarsPerCcd
Minimum number of measuredStars per ccdImage before printing warnings ( int
, default30
)outlierRejectSigma
How many sigma to reject outliers at during minimization. photometryDoRankUpdate
Do the rank update step during minimization. photometryErrorPedestal
Systematic term to apply to the measured error on flux or magnitude as a fraction of source flux or magnitude delta (e.g. photometryModel
Type of model to fit to photometry ( str
, default'constrainedMagnitude'
)photometryRefObjLoader
Reference object loader for photometric fit ( ConfigurableInstance
, default<class 'lsst.meas.algorithms.loadIndexedReferenceObjects.LoadIndexedReferenceObjectsConfig'>
)photometryReferenceSelector
How to down-select the loaded photometry reference catalog. photometryVisitOrder
Order of the per-visit polynomial transform for the constrained photometry model. positionErrorPedestal
Systematic term to apply to the measured position error (pixels) ( float
, default0.02
)sourceFluxType
Source flux field to use in source selection and to get fluxes from the catalog. sourceSelector
How to select sources for cross-matching ( RegistryInstanceDict
, default'astrometry'
)useInputWcs
Use the input calexp WCSs to initialize a SimpleAstrometryModel. writeChi2ContributionFiles
Write initial/final fit files containing the contributions to chi2. writeInitMatrix
Write the pre/post-initialization Hessian and gradient to text files, for debugging.The output files will be of the form ‘astrometry_preinit-mat.txt’, in the current directory.Note that these files are the dense versions of the matrix, and so may be very large. Methods Summary
compare
(other[, shortcut, rtol, atol, output])Compare this configuration to another Config
for equality.formatHistory
(name, **kwargs)Format a configuration field’s history to a human-readable format. freeze
()Make this config, and all subconfigs, read-only. items
()Get configurations as (field name, field value)
pairs.iteritems
()Iterate over (field name, field value) pairs. iterkeys
()Iterate over field names itervalues
()Iterate over field values. keys
()Get field names. load
(filename[, root])Modify this config in place by executing the Python code in a configuration file. loadFromStream
(stream[, root, filename])Modify this Config in place by executing the Python code in the provided stream. names
()Get all the field names in the config, recursively. save
(filename[, root])Save a Python script to the named file, which, when loaded, reproduces this config. saveToStream
(outfile[, root])Save a configuration file to a stream, which, when loaded, reproduces this config. setDefaults
()Subclass hook for computing defaults. toDict
()Make a dictionary of field names and their values. update
(**kw)Update values of fields specified by the keyword arguments. validate
()Validate the Config, raising an exception if invalid. values
()Get field values. Attributes Documentation
-
allowLineSearch
¶ Allow a line search during minimization, if it is reasonable for the model (models with a significant non-linear component, e.g. constrainedPhotometry). (
bool
, defaultFalse
)
-
applyColorTerms
¶ Apply photometric color terms to reference stars?Requires that colorterms be set to a ColortermLibrary (
bool
, defaultFalse
)
-
astrometryChipOrder
¶ Order of the per-chip transform for the constrained astrometry model. (
int
, default1
)
-
astrometryDoRankUpdate
¶ Do the rank update step during minimization (should not change the astrometry fit). Skipping this can help deal with models that are too non-linear. (
bool
, defaultTrue
)
-
astrometryModel
¶ Type of model to fit to astrometry (
str
, default'constrained'
)Allowed values:
'simple'
- One polynomial per ccd
'constrained'
- One polynomial per ccd, and one polynomial per visit
'None'
- Field is optional
-
astrometryRefObjLoader
¶ Reference object loader for astrometric fit (
ConfigurableInstance
, default<class 'lsst.meas.algorithms.loadIndexedReferenceObjects.LoadIndexedReferenceObjectsConfig'>
)
-
astrometryReferenceSelector
¶ How to down-select the loaded astrometry reference catalog. (
ConfigurableInstance
, default<class 'lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig'>
)
-
astrometryVisitOrder
¶ Order of the per-visit transform for the constrained astrometry model. (
int
, default5
)
-
colorterms
¶ Library of photometric reference catalog name to color term dict. (
ColortermLibrary
, default<class 'lsst.pipe.tasks.colorterms.ColortermLibrary'>
)
-
history
¶
-
maxAstrometrySteps
¶ Maximum number of minimize iterations to take when fitting photometry. (
int
, default20
)
-
maxPhotometrySteps
¶ Maximum number of minimize iterations to take when fitting photometry. (
int
, default20
)
-
minMeasuredStarsPerCcd
¶ Minimum number of measuredStars per ccdImage before printing warnings (
int
, default100
)
-
minMeasurements
¶ Minimum number of associated measured stars for a fitted star to be included in the fit (
int
, default2
)
-
minRefStarsPerCcd
¶ Minimum number of measuredStars per ccdImage before printing warnings (
int
, default30
)
-
photometryDoRankUpdate
¶ Do the rank update step during minimization. Skipping this can help deal with models that are too non-linear. (
bool
, defaultTrue
)
-
photometryErrorPedestal
¶ Systematic term to apply to the measured error on flux or magnitude as a fraction of source flux or magnitude delta (e.g. 0.05 is 5% of flux or +50 millimag). (
float
, default0.0
)
-
photometryModel
¶ Type of model to fit to photometry (
str
, default'constrainedMagnitude'
)Allowed values:
'simpleFlux'
- One constant zeropoint per ccd and visit, fitting in flux space.
'constrainedFlux'
- Constrained zeropoint per ccd, and one polynomial per visit, fitting in flux space.
'simpleMagnitude'
- One constant zeropoint per ccd and visit, fitting in magnitude space.
'constrainedMagnitude'
- Constrained zeropoint per ccd, and one polynomial per visit, fitting in magnitude space.
'None'
- Field is optional
-
photometryRefObjLoader
¶ Reference object loader for photometric fit (
ConfigurableInstance
, default<class 'lsst.meas.algorithms.loadIndexedReferenceObjects.LoadIndexedReferenceObjectsConfig'>
)
-
photometryReferenceSelector
¶ How to down-select the loaded photometry reference catalog. (
ConfigurableInstance
, default<class 'lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig'>
)
-
photometryVisitOrder
¶ Order of the per-visit polynomial transform for the constrained photometry model. (
int
, default7
)
-
positionErrorPedestal
¶ Systematic term to apply to the measured position error (pixels) (
float
, default0.02
)
-
sourceFluxType
¶ Source flux field to use in source selection and to get fluxes from the catalog. (
str
, default'Calib'
)
-
sourceSelector
¶ How to select sources for cross-matching (
RegistryInstanceDict
, default'astrometry'
)
-
writeChi2ContributionFiles
¶ Write initial/final fit files containing the contributions to chi2. (
bool
, defaultFalse
)
-
writeInitMatrix
¶ Write the pre/post-initialization Hessian and gradient to text files, for debugging.The output files will be of the form ‘astrometry_preinit-mat.txt’, in the current directory.Note that these files are the dense versions of the matrix, and so may be very large. (
bool
, defaultFalse
)
Methods Documentation
-
compare
(other, shortcut=True, rtol=1e-08, atol=1e-08, output=None)¶ Compare this configuration to another
Config
for equality.Parameters: - other :
lsst.pex.config.Config
Other
Config
object to compare against this config.- shortcut :
bool
, optional If
True
, return as soon as an inequality is found. Default isTrue
.- rtol :
float
, optional Relative tolerance for floating point comparisons.
- atol :
float
, optional Absolute tolerance for floating point comparisons.
- output : callable, optional
A callable that takes a string, used (possibly repeatedly) to report inequalities.
Returns: - isEqual :
bool
True
when the twolsst.pex.config.Config
instances are equal.False
if there is an inequality.
See also
Notes
Unselected targets of
RegistryField
fields and unselected choices ofConfigChoiceField
fields are not considered by this method.Floating point comparisons are performed by
numpy.allclose
.- other :
-
formatHistory
(name, **kwargs)¶ Format a configuration field’s history to a human-readable format.
Parameters: - name :
str
Name of a
Field
in this config.- kwargs
Keyword arguments passed to
lsst.pex.config.history.format
.
Returns: - history :
str
A string containing the formatted history.
See also
- name :
-
freeze
()¶ Make this config, and all subconfigs, read-only.
-
items
()¶ Get configurations as
(field name, field value)
pairs.Returns: - items :
list
List of tuples for each configuration. Tuple items are:
- Field name.
- Field value.
See also
- items :
-
iteritems
()¶ Iterate over (field name, field value) pairs.
Yields: - item :
tuple
Tuple items are:
- Field name.
- Field value.
See also
- item :
-
itervalues
()¶ Iterate over field values.
Yields: - value : obj
A field value.
See also
-
keys
()¶ Get field names.
Returns: - names :
list
List of
lsst.pex.config.Field
names.
See also
- names :
-
load
(filename, root='config')¶ Modify this config in place by executing the Python code in a configuration file.
Parameters: - filename :
str
Name of the configuration file. A configuration file is Python module.
- root :
str
, optional Name of the variable in file that refers to the config being overridden.
For example, the value of root is
"config"
and the file contains:config.myField = 5
Then this config’s field
myField
is set to5
.Deprecated: For backwards compatibility, older config files that use
root="root"
instead ofroot="config"
will be loaded with a warning printed tosys.stderr
. This feature will be removed at some point.
See also
lsst.pex.config.Config.loadFromStream
,lsst.pex.config.Config.save
,lsst.pex.config.Config.saveFromStream
- filename :
-
loadFromStream
(stream, root='config', filename=None)¶ Modify this Config in place by executing the Python code in the provided stream.
Parameters: - stream : file-like object,
str
, or compiled string Stream containing configuration override code.
- root :
str
, optional Name of the variable in file that refers to the config being overridden.
For example, the value of root is
"config"
and the file contains:config.myField = 5
Then this config’s field
myField
is set to5
.Deprecated: For backwards compatibility, older config files that use
root="root"
instead ofroot="config"
will be loaded with a warning printed tosys.stderr
. This feature will be removed at some point.- filename :
str
, optional Name of the configuration file, or
None
if unknown or contained in the stream. Used for error reporting.
See also
lsst.pex.config.Config.load
,lsst.pex.config.Config.save
,lsst.pex.config.Config.saveFromStream
- stream : file-like object,
-
names
()¶ Get all the field names in the config, recursively.
Returns:
-
save
(filename, root='config')¶ Save a Python script to the named file, which, when loaded, reproduces this config.
Parameters: - filename :
str
Desination filename of this configuration.
- root :
str
, optional Name to use for the root config variable. The same value must be used when loading (see
lsst.pex.config.Config.load
).
- filename :
-
saveToStream
(outfile, root='config')¶ Save a configuration file to a stream, which, when loaded, reproduces this config.
Parameters: - outfile : file-like object
Destination file object write the config into. Accepts strings not bytes.
- root
Name to use for the root config variable. The same value must be used when loading (see
lsst.pex.config.Config.load
).
-
setDefaults
()¶ Subclass hook for computing defaults.
Notes
Derived
Config
classes that must compute defaults rather than using theField
instances’s defaults should do so here. To correctly use inherited defaults, implementations ofsetDefaults
must call their base class’ssetDefaults
.
-
toDict
()¶ Make a dictionary of field names and their values.
Returns: See also
Notes
This method uses the
toDict
method of individual fields. Subclasses ofField
may need to implement atoDict
method for this method to work.
-
update
(**kw)¶ Update values of fields specified by the keyword arguments.
Parameters: - kw
Keywords are configuration field names. Values are configuration field values.
Notes
The
__at
and__label
keyword arguments are special internal keywords. They are used to strip out any internal steps from the history tracebacks of the config. Do not modify these keywords to subvert aConfig
instance’s history.Examples
This is a config with three fields:
>>> from lsst.pex.config import Config, Field >>> class DemoConfig(Config): ... fieldA = Field(doc='Field A', dtype=int, default=42) ... fieldB = Field(doc='Field B', dtype=bool, default=True) ... fieldC = Field(doc='Field C', dtype=str, default='Hello world') ... >>> config = DemoConfig()
These are the default values of each field:
>>> for name, value in config.iteritems(): ... print(f"{name}: {value}") ... fieldA: 42 fieldB: True fieldC: 'Hello world'
Using this method to update
fieldA
andfieldC
:>>> config.update(fieldA=13, fieldC='Updated!')
Now the values of each field are:
>>> for name, value in config.iteritems(): ... print(f"{name}: {value}") ... fieldA: 13 fieldB: True fieldC: 'Updated!'
-
validate
()¶ Validate the Config, raising an exception if invalid.
Raises: - lsst.pex.config.FieldValidationError
Raised if verification fails.
Notes
The base class implementation performs type checks on all fields by calling their
validate
methods.Complex single-field validation can be defined by deriving new Field types. For convenience, some derived
lsst.pex.config.Field
-types (ConfigField
andConfigChoiceField
) are defined inlsst.pex.config
that handle recursing into subconfigs.Inter-field relationships should only be checked in derived
Config
classes after calling this method, and base validation is complete.
-