FringeTask¶
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class lsst.ip.isr.FringeTask(config: Optional[Config] = None, name: Optional[str] = None, parentTask: Optional[Task] = None, log: Optional[Union[logging.Logger, lsst.utils.logging.LsstLogAdapter]] = None)¶
- Bases: - lsst.pipe.base.Task- Task to remove fringes from a science exposure - We measure fringe amplitudes at random positions on the science exposure and at the same positions on the (potentially multiple) fringe frames and solve for the scales simultaneously. - Methods Summary - checkFilter(exposure)- Check whether we should fringe-subtract the science exposure. - emptyMetadata()- Empty (clear) the metadata for this Task and all sub-Tasks. - generatePositions(exposure, rng)- Generate a random distribution of positions for measuring fringe amplitudes. - getFullMetadata()- Get metadata for all tasks. - getFullName()- Get the task name as a hierarchical name including parent task names. - getName()- Get the name of the task. - getTaskDict()- Get a dictionary of all tasks as a shallow copy. - loadFringes(fringeExp[, expId, assembler])- Pack the fringe data into a Struct. - makeField(doc)- Make a - lsst.pex.config.ConfigurableFieldfor this task.- makeSubtask(name, **keyArgs)- Create a subtask as a new instance as the - nameattribute of this task.- measureExposure(exposure, positions[, title])- Measure fringe amplitudes for an exposure - removePedestal(fringe)- Remove pedestal from fringe exposure. - run(exposure, fringes[, seed])- Remove fringes from the provided science exposure. - solve(science, fringes)- Solve for the scale factors with iterative clipping. - subtract(science, fringes, solution)- Subtract the fringes. - timer(name, logLevel)- Context manager to log performance data for an arbitrary block of code. - Methods Documentation - 
checkFilter(exposure)¶
- Check whether we should fringe-subtract the science exposure. - Parameters: - exposure : lsst.afw.image.Exposure
- Exposure to check the filter of. 
 - Returns: - needsFringe : bool
- If True, then the exposure has a filter listed in the configuration, and should have the fringe applied. 
 
- exposure : 
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emptyMetadata() → None¶
- Empty (clear) the metadata for this Task and all sub-Tasks. 
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generatePositions(exposure, rng)¶
- Generate a random distribution of positions for measuring fringe amplitudes. - Parameters: - exposure : lsst.afw.image.Exposure
- Exposure to measure the positions on. 
- rng : numpy.random.RandomState
- Random number generator to use. 
 - Returns: - positions : numpy.array
- Two-dimensional array containing the positions to sample for fringe amplitudes. 
 
- exposure : 
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getFullMetadata() → lsst.pipe.base._task_metadata.TaskMetadata¶
- Get metadata for all tasks. - Returns: - metadata : TaskMetadata
- The keys are the full task name. Values are metadata for the top-level task and all subtasks, sub-subtasks, etc. 
 - Notes - The returned metadata includes timing information (if - @timer.timeMethodis used) and any metadata set by the task. The name of each item consists of the full task name with- .replaced by- :, followed by- .and the name of the item, e.g.:- topLevelTaskName:subtaskName:subsubtaskName.itemName - using - :in the full task name disambiguates the rare situation that a task has a subtask and a metadata item with the same name.
- metadata : 
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getFullName() → str¶
- Get the task name as a hierarchical name including parent task names. - Returns: - fullName : str
- The full name consists of the name of the parent task and each subtask separated by periods. For example: - The full name of top-level task “top” is simply “top”.
- The full name of subtask “sub” of top-level task “top” is “top.sub”.
- The full name of subtask “sub2” of subtask “sub” of top-level task “top” is “top.sub.sub2”.
 
 
- fullName : 
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getTaskDict() → Dict[str, weakref.ReferenceType[lsst.pipe.base.task.Task]]¶
- Get a dictionary of all tasks as a shallow copy. - Returns: - taskDict : dict
- Dictionary containing full task name: task object for the top-level task and all subtasks, sub-subtasks, etc. 
 
- taskDict : 
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loadFringes(fringeExp, expId=None, assembler=None)¶
- Pack the fringe data into a Struct. - This method moves the struct parsing code into a butler generation agnostic handler. - Parameters: - fringeExp : lsst.afw.exposure.Exposure
- The exposure containing the fringe data. 
- expId : int, optional
- Exposure id to be fringe corrected, used to set RNG seed. 
- assembler : lsst.ip.isr.AssembleCcdTask, optional
- An instance of AssembleCcdTask (for assembling fringe frames). 
 - Returns: 
- fringeExp : 
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classmethod makeField(doc: str) → lsst.pex.config.configurableField.ConfigurableField¶
- Make a - lsst.pex.config.ConfigurableFieldfor this task.- Parameters: - doc : str
- Help text for the field. 
 - Returns: - configurableField : lsst.pex.config.ConfigurableField
- A - ConfigurableFieldfor this task.
 - Examples - Provides a convenient way to specify this task is a subtask of another task. - Here is an example of use: - class OtherTaskConfig(lsst.pex.config.Config): aSubtask = ATaskClass.makeField("brief description of task") 
- doc : 
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makeSubtask(name: str, **keyArgs) → None¶
- Create a subtask as a new instance as the - nameattribute of this task.- Parameters: - name : str
- Brief name of the subtask. 
- keyArgs
- Extra keyword arguments used to construct the task. The following arguments are automatically provided and cannot be overridden: - “config”.
- “parentTask”.
 
 - Notes - The subtask must be defined by - Task.config.name, an instance of- ConfigurableFieldor- RegistryField.
- name : 
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measureExposure(exposure, positions, title='Fringe')¶
- Measure fringe amplitudes for an exposure - The fringe amplitudes are measured as the statistic within a square aperture. The statistic within a larger aperture are subtracted so as to remove the background. - Parameters: - exposure : lsst.afw.image.Exposure
- Exposure to measure the positions on. 
- positions : numpy.array
- Two-dimensional array containing the positions to sample for fringe amplitudes. 
- title : str, optional
- Title used for debug out plots. 
 - Returns: - fringes : numpy.array
- Array of measured exposure values at each of the positions supplied. 
 
- exposure : 
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removePedestal(fringe)¶
- Remove pedestal from fringe exposure. - Parameters: - fringe : lsst.afw.image.Exposure
- Fringe data to subtract the pedestal value from. 
 
- fringe : 
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run(exposure, fringes, seed=None)¶
- Remove fringes from the provided science exposure. - Primary method of FringeTask. Fringes are only subtracted if the science exposure has a filter listed in the configuration. - Parameters: - Returns: - solution : np.array
- Fringe solution amplitudes for each input fringe frame. 
- rms : float
- RMS error for the fit solution for this exposure. 
 
- solution : 
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solve(science, fringes)¶
- Solve for the scale factors with iterative clipping. - Parameters: - science : numpy.array
- Array of measured science image values at each of the positions supplied. 
- fringes : numpy.array
- Array of measured fringe values at each of the positions supplied. 
 - Returns: - solution : np.array
- Fringe solution amplitudes for each input fringe frame. 
- rms : float
- RMS error for the fit solution for this exposure. 
 
- science : 
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subtract(science, fringes, solution)¶
- Subtract the fringes. - Parameters: - science : lsst.afw.image.Exposure
- Science exposure from which to remove fringes. 
- fringes : lsst.afw.image.Exposureorlistthereof
- Calibration fringe files containing master fringe frames. 
- solution : np.array
- Fringe solution amplitudes for each input fringe frame. 
 - Raises: - RuntimeError
- Raised if the number of fringe frames does not match the number of measured amplitudes. 
 
- science : 
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timer(name: str, logLevel: int = 10) → Iterator[None]¶
- Context manager to log performance data for an arbitrary block of code. - Parameters: - See also - timer.logInfo
 - Examples - Creating a timer context: - with self.timer("someCodeToTime"): pass # code to time 
 
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