ColorColorFitPlot

class lsst.analysis.tools.actions.plot.ColorColorFitPlot(*args, **kw)

Bases: PlotAction

Make a color-color plot and overplot a prefited line to the fit region.

This is mostly used for the stellar locus plots and also includes panels that illustrate the goodness of the given fit.

Attributes Summary

applyContext

Apply a Context to an AnalysisAction recursively.

doPlotDistVsColor

Plot distance from fit as a function of color in lower right panel? (bool, default True)

doPlotRedBlueHists

Plot distance from fit histograms separated into blue and red star subsamples? (bool, default False)

history

identity

If a configurable action is assigned to a ConfigurableActionField, or a ConfigurableActionStructField the name of the field will be bound to this variable when it is retrieved.

magLabel

Label to use for the magnitudes used to color code by (str)

minPointsForFit

Minimum number of valid objects to bother attempting a fit.

plotName

The name for the plot.

plotTypes

Selection of types of objects to plot.

xAxisLabel

Label to use for the x axis (str)

xLims

Minimum and maximum x-axis limit to force (provided as a list of [xMin, xMax]).

yAxisLabel

Label to use for the y axis (str)

yLims

Minimum and maximum y-axis limit to force (provided as a list of [yMin, yMax]).

Methods Summary

__call__(data, **kwargs)

Call self as a function.

addInputSchema(inputSchema)

Add the supplied inputSchema argument to the class such that it will be returned along side any other arguments in a call to getInputSchema.

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.

getFormattedInputSchema(**kwargs)

Return input schema, with keys formatted with any arguments supplied by kwargs passed to this method.

getInputSchema(**kwargs)

Return the schema an AnalysisAction expects to be present in the arguments supplied to the __call__ method.

getOutputNames([config])

Returns a list of names that will be used as keys if this action's call method returns a mapping.

getOutputSchema()

Return the schema an AnalysisAction will produce, if the __call__ method returns KeyedData, otherwise this may return None.

getPlotType()

items()

Get configurations as (field name, field value) pairs.

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.

loadFromString(code[, root, filename, ...])

Modify this Config in place by executing the Python code in the provided string.

makePlot(data, plotInfo, **kwargs)

Make stellar locus plots using pre fitted values.

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, skipImports])

Save a configuration file to a stream, which, when loaded, reproduces this config.

saveToString([skipImports])

Return the Python script form of this configuration as an executable string.

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

applyContext

Apply a Context to an AnalysisAction recursively.

Generally this method is called from within an AnalysisTool to configure all AnalysisActions at one time to make sure that they all are consistently configured. However, it is permitted to call this method if you are aware of the effects, or from within a specific execution environment like a python shell or notebook.

Parameters:
contextContext

The specific execution context, this may be a single context or a joint context, see Context for more info.

doPlotDistVsColor

Plot distance from fit as a function of color in lower right panel? (bool, default True)

doPlotRedBlueHists

Plot distance from fit histograms separated into blue and red star subsamples? (bool, default False)

history

Read-only history.

identity: str | None = None

If a configurable action is assigned to a ConfigurableActionField, or a ConfigurableActionStructField the name of the field will be bound to this variable when it is retrieved.

magLabel

Label to use for the magnitudes used to color code by (str)

minPointsForFit

Minimum number of valid objects to bother attempting a fit. Deprecated: This field is no longer used. The value should go as an entry to the paramsDict keyed as minObjectForFit. Will be removed after v27. (int, default 5)

Valid Range = [1,inf)

plotName

The name for the plot. (str)

plotTypes

Selection of types of objects to plot. Can take any combination of stars, galaxies, unknown, mag, any. (List, default ['stars'])

xAxisLabel

Label to use for the x axis (str)

xLims

Minimum and maximum x-axis limit to force (provided as a list of [xMin, xMax]). If None, limits will be computed and set based on the data. (List, default None)

yAxisLabel

Label to use for the y axis (str)

yLims

Minimum and maximum y-axis limit to force (provided as a list of [yMin, yMax]). If None, limits will be computed and set based on the data. (List, default None)

Methods Documentation

__call__(data: MutableMapping[str, ndarray[Any, dtype[ScalarType]] | Scalar | HealSparseMap | Tensor], **kwargs) Mapping[str, Figure] | Figure

Call self as a function.

addInputSchema(inputSchema: Tensor]]]) None

Add the supplied inputSchema argument to the class such that it will be returned along side any other arguments in a call to getInputSchema.

Parameters:
inputSchemaKeyedDataSchema

A schema that is to be merged in with any existing schema when a call to getInputSchema is made.

compare(other, shortcut=True, rtol=1e-08, atol=1e-08, output=None)

Compare this configuration to another Config for equality.

Parameters:
otherlsst.pex.config.Config

Other Config object to compare against this config.

shortcutbool, optional

If True, return as soon as an inequality is found. Default is True.

rtolfloat, optional

Relative tolerance for floating point comparisons.

atolfloat, optional

Absolute tolerance for floating point comparisons.

outputcallable, optional

A callable that takes a string, used (possibly repeatedly) to report inequalities.

Returns:
isEqualbool

True when the two lsst.pex.config.Config instances are equal. False if there is an inequality.

Notes

Unselected targets of RegistryField fields and unselected choices of ConfigChoiceField fields are not considered by this method.

Floating point comparisons are performed by numpy.allclose.

formatHistory(name, **kwargs)

Format a configuration field’s history to a human-readable format.

Parameters:
namestr

Name of a Field in this config.

**kwargs

Keyword arguments passed to lsst.pex.config.history.format.

Returns:
historystr

A string containing the formatted history.

freeze()

Make this config, and all subconfigs, read-only.

getFormattedInputSchema(**kwargs) Tensor]]]

Return input schema, with keys formatted with any arguments supplied by kwargs passed to this method.

Returns:
resultKeyedDataSchema

The schema this action requires to be present when calling this action, formatted with any input arguments (e.g. band=’i’)

getInputSchema(**kwargs) Tensor]]]

Return the schema an AnalysisAction expects to be present in the arguments supplied to the __call__ method.

Returns:
resultKeyedDataSchema

The schema this action requires to be present when calling this action, keys are unformatted.

getOutputNames(config: Config | None = None) Iterable[str]

Returns a list of names that will be used as keys if this action’s call method returns a mapping. Otherwise return an empty Iterable.

Parameters:
configlsst.pex.config.Config, optional

Configuration of the task. This is only used if the output naming needs to be config-aware.

Returns:
resultIterable of str

If a PlotAction produces more than one plot, this should be the keys the action will use in the returned Mapping.

getOutputSchema() Tensor]]] | None

Return the schema an AnalysisAction will produce, if the __call__ method returns KeyedData, otherwise this may return None.

Returns:
resultKeyedDataSchema or None

The schema this action will produce when returning from call. This will be unformatted if any templates are present. Should return None if action does not return KeyedData.

getPlotType() str
items()

Get configurations as (field name, field value) pairs.

Returns:
itemsItemsView

Iterator of tuples for each configuration. Tuple items are:

  1. Field name.

  2. Field value.

keys()

Get field names.

Returns:
namesKeysView

List of lsst.pex.config.Field names.

load(filename, root='config')

Modify this config in place by executing the Python code in a configuration file.

Parameters:
filenamestr

Name of the configuration file. A configuration file is Python module.

rootstr, 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 to 5.

loadFromStream(stream, root='config', filename=None, extraLocals=None)

Modify this Config in place by executing the Python code in the provided stream.

Parameters:
streamfile-like object, str, bytes, or CodeType

Stream containing configuration override code. If this is a code object, it should be compiled with mode="exec".

rootstr, 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 to 5.

filenamestr, optional

Name of the configuration file, or None if unknown or contained in the stream. Used for error reporting.

extraLocalsdict of str to object, optional

Any extra variables to include in local scope when loading.

Notes

For backwards compatibility reasons, this method accepts strings, bytes and code objects as well as file-like objects. New code should use loadFromString instead for most of these types.

loadFromString(code, root='config', filename=None, extraLocals=None)

Modify this Config in place by executing the Python code in the provided string.

Parameters:
codestr, bytes, or CodeType

Stream containing configuration override code.

rootstr, 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 to 5.

filenamestr, optional

Name of the configuration file, or None if unknown or contained in the stream. Used for error reporting.

extraLocalsdict of str to object, optional

Any extra variables to include in local scope when loading.

Raises:
ValueError

Raised if a key in extraLocals is the same value as the value of the root argument.

makePlot(data: MutableMapping[str, ndarray[Any, dtype[ScalarType]] | Scalar | HealSparseMap | Tensor], plotInfo: Mapping[str, str], **kwargs) Figure

Make stellar locus plots using pre fitted values.

Parameters:
dataKeyedData

The data to plot the points from, for more information please see the notes section.

plotInfodict

A dictionary of information about the data being plotted with keys:

  • "run"

    The output run for the plots (str).

  • "skymap"

    The type of skymap used for the data (str).

  • "filter"

    The filter used for this data (str).

  • "tract"

    The tract that the data comes from (str).

Returns:
figmatplotlib.figure.Figure

The resulting figure.

Notes

The axis labels are given by self.xAxisLabel and self.yAxisLabel. The perpendicular distance of the points to the fit line is given in a histogram in the second panel.

For the code to work it expects various quantities to be present in the data that it is given.

The quantities that are expected to be present are:

  • Statistics that are shown on the plot or used by the plotting code:
    • approxMagDepth

      The approximate magnitude corresponding to the SN cut used.

    • f"{self.plotName}_sigmaMAD"

      The sigma mad of the distances to the line fit.

    • f"{self.plotName or ''}_median"

      The median of the distances to the line fit.

  • Parameters from the fitting code that are illustrated on the plot:
    • "bFixed"

      The fixed intercept to fall back on.

    • "mFixed"

      The fixed gradient to fall back on.

    • "bODR"

      The intercept calculated by the final orthogonal distance regression fitting.

    • "mODR"

      The gradient calculated by the final orthogonal distance regression fitting.

    • "xMin`"

      The x minimum of the box used in the fit.

    • "xMax"

      The x maximum of the box used in the fit.

    • "yMin"

      The y minimum of the box used in the fit.

    • "yMax"

      The y maximum of the box used in the fit.

    • "mPerp"

      The gradient of the line perpendicular to the line from the second ODR fit.

    • "bPerpMin"

      The intercept of the perpendicular line that goes through xMin.

    • "bPerpMax"

      The intercept of the perpendicular line that goes through xMax.

    • "goodPoints"

      The points that passed the initial set of cuts (typically in fluxType S/N, extendedness, magnitude, and isfinite).

    • "fitPoints"

      The points use in the final fit.

  • The main inputs to plot:

    x, y, mag

Examples

An example of the plot produced from this code is here:

../_images/stellarLocusExample.png

For a detailed example of how to make a plot from the command line please see the getting started guide.

names()

Get all the field names in the config, recursively.

Returns:
nameslist of str

Field names.

save(filename, root='config')

Save a Python script to the named file, which, when loaded, reproduces this config.

Parameters:
filenamestr

Desination filename of this configuration.

rootstr, optional

Name to use for the root config variable. The same value must be used when loading (see lsst.pex.config.Config.load).

saveToStream(outfile, root='config', skipImports=False)

Save a configuration file to a stream, which, when loaded, reproduces this config.

Parameters:
outfilefile-like object

Destination file object write the config into. Accepts strings not bytes.

rootstr, optional

Name to use for the root config variable. The same value must be used when loading (see lsst.pex.config.Config.load).

skipImportsbool, optional

If True then do not include import statements in output, this is to support human-oriented output from pipetask where additional clutter is not useful.

saveToString(skipImports=False)

Return the Python script form of this configuration as an executable string.

Parameters:
skipImportsbool, optional

If True then do not include import statements in output, this is to support human-oriented output from pipetask where additional clutter is not useful.

Returns:
codestr

A code string readable by loadFromString.

setDefaults()

Subclass hook for computing defaults.

Notes

Derived Config classes that must compute defaults rather than using the Field instances’s defaults should do so here. To correctly use inherited defaults, implementations of setDefaults must call their base class’s setDefaults.

toDict()

Make a dictionary of field names and their values.

Returns:
dict_dict

Dictionary with keys that are Field names. Values are Field values.

Notes

This method uses the toDict method of individual fields. Subclasses of Field may need to implement a toDict 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 a Config 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 and fieldC:

>>> 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 and ConfigChoiceField) are defined in lsst.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.

values()

Get field values.

Returns:
valuesValuesView

Iterator of field values.