Analysis Tools
Utilities
toast.ops.Delete
Bases: Operator
Class to purge data from observations.
This operator takes lists of shared, detdata, intervals and meta keys to delete from observations.
Source code in toast/ops/delete.py
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toast.ops.Reset
Bases: Operator
Class to reset data from observations.
This operator takes lists of shared, detdata, intervals, and meta keys to reset.
Numerical data objects and arrays are set to zero. String objects are set to an
empty string. Any object that defines a clear() method will have that called.
Any object not matching those criteria will be set to None. Since an IntervalList
is not mutable, any specified intervals will simply be deleted.
Source code in toast/ops/reset.py
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toast.ops.Copy
Bases: Operator
Class to copy data.
This operator takes lists of shared, detdata, and meta keys to copy to a new location in each observation.
Each list contains tuples specifying the input and output key names.
Source code in toast/ops/copy.py
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toast.ops.Combine
Bases: Operator
Arithmetic with detector data.
Two detdata objects are combined element-wise using addition, subtraction, multiplication, or division. The desired operation is specified by the "op" trait as a string. The result is stored in the specified detdata object:
result = first (op) second
If the result name is the same as the first or second input, then this input will be overwritten.
Source code in toast/ops/arithmetic.py
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toast.ops.CalibrateDetectors
Bases: Operator
Multiply detector data by calibration factors.
The calibration factor can be specified as a fixed value for all detectors (for example when converting from raw ADC values) or per-detector values can be supplied as a dictionary within the observation metadata or a column of the focalplane data table. Detectors which are missing in the calibration dictionary are flagged.
This operator is frequently the first one applied to "raw" data loaded from disk. If the dtype of the input DetectorData is an integer type, it will be promoted to float64 before applying the calibration.
The units of the DetectorData can be updated with the cal_units trait.
Source code in toast/ops/calibrate.py
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toast.ops.MemoryCounter
Bases: Operator
Compute total memory used by Observations in a Data object.
Every process group iterates over their observations and sums the total memory used by detector and shared data. Metadata and interval lists are assumed to be negligible and are not counted.
Source code in toast/ops/memory_counter.py
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toast.ops.Statistics
Bases: Operator
Operator to measure and write out data statistics
Source code in toast/ops/statistics.py
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toast.ops.Pipeline
Bases: Operator
Class representing a sequence of Operators.
This runs a list of other operators over sets of detectors (default is all
detectors in one shot). By default all observations are passed to each operator,
but the observation_key and observation_value traits can be used to run the
operators on only observations which have a matching key / value pair.
Source code in toast/ops/pipeline.py
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__str__()
Converts the pipeline into a human-readable string.
Source code in toast/ops/pipeline.py
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toast.ops.RunSpt3g
Bases: Operator
Operator which runs a G3Pipeline.
This operator converts each observation to a stream of frames on each process
and then runs the specified G3 pipeline on the local frames. If the obs_import
trait is specified, the resulting frames are re-imported to a toast observation
at the end.
Source code in toast/ops/run_spt3g.py
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Flagging
toast.ops.AzimuthIntervals
Bases: Operator
Build intervals that describe the scanning motion in azimuth.
This operator passes through the azimuth angle and builds the list of intervals for standard types of scanning / turnaround motion. Note that it only makes sense to use this operator for ground-based telescopes that primarily scan in azimuth rather than more complicated (e.g. lissajous) patterns.
Source code in toast/ops/azimuth_intervals.py
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toast.ops.FlagIntervals
Bases: Operator
Operator which updates shared flags from interval lists.
This operator can be used in cases where interval information needs to be combined with shared flags. The view_mask trait is a list of tuples. Each tuple contains the name of the view (i.e. interval) to apply and the bitmask to use for that view. For each interval view, flag values in the shared_flags object are bitwise- OR'd with the specified mask for samples in the view. If the name of the view is prefixed with '~' the bitmask is applied to all samples outside the view.
Source code in toast/ops/flag_intervals.py
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toast.ops.FlagSSO
Bases: Operator
Operator which flags detector data in the vicinity of solar system objects
Source code in toast/ops/flag_sso.py
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toast.ops.SimpleDeglitch
Bases: Operator
An operator that flags extreme detector samples.
Source code in toast/ops/simple_deglitch.py
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toast.ops.SimpleJumpCorrect
Bases: Operator
An operator that identifies and corrects jumps in the data
Source code in toast/ops/simple_jumpcorrect.py
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toast.ops.FillGaps
Bases: Operator
Operator that fills flagged samples with noise.
Currently this operator just fills flagged samples with a simple polynomial plus white noise. It is mostly used for visualization. No attempt is made yet to fill the gaps with a constrained noise realization.
Source code in toast/ops/fill_gaps.py
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Filtering
Polynomial Filters
toast.ops.CommonModeFilter
Bases: Operator
Operator to regress out common mode at each time stamp.
Source code in toast/ops/polyfilter/polyfilter.py
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toast.ops.PolyFilter
Bases: Operator
Operator which applies polynomial filtering to the TOD.
Source code in toast/ops/polyfilter/polyfilter.py
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toast.ops.PolyFilter2D
Bases: Operator
Operator to regress out 2D polynomials across the focal plane.
Source code in toast/ops/polyfilter/polyfilter.py
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Specialized Filters
toast.ops.GroundFilter
Bases: Operator
Operator that applies ground template filtering to azimuthal scans.
Source code in toast/ops/groundfilter.py
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build_templates(obs)
Construct the local ground template hierarchy
Source code in toast/ops/groundfilter.py
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toast.ops.MitigateCrossTalk
Bases: Operator
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The cross talk matrix can just be a dictionary of dictionaries of values (i.e. a sparse matrix) on every process. It does not need to be a dense matrix loaded from an HDF5 file. The calling code can create this however it likes.
-
Each process has a DetectorData object representing the local data for some detectors and some timespan (e.g. obs.detdata["signal"]). It can make a copy of this and pass it to the next rank in the grid column. Each process receives a copy from the previous process in the column, accumulates to its local detectors, and passes it along. This continues until every process has accumulated the data from the other processes in the column.
Source code in toast/ops/sim_crosstalk.py
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Half Wave Plate Tools
toast.ops.HWPSynchronousModel
Bases: Operator
Operator that models and removes HWP synchronous signal.
This fits and optionally subtracts a Maxipol / EBEX style model for the HWPSS.
The time dependent drift term is optional. See the details in
toast.hwp_utils.hwpss_compute_coeff_covariance().
The 2f component of the model is optionally used to build a relative calibration between detectors, either as a fixed table per observation or as continuously varying factors.
The HWPSS model can be constructed either with one set of template coefficients for the entire observation, or one set per time interval smoothly interpolated across the observation.
Source code in toast/ops/hwpss_model.py
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toast.ops.HWPFilter
Bases: Operator
Operator that applies HWP-synchronous signal filtering.
Source code in toast/ops/hwpfilter.py
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build_templates(obs)
Construct the local HWPSS template hierarchy
Source code in toast/ops/hwpfilter.py
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toast.ops.Demodulate
Bases: Operator
Demodulate and downsample HWP-modulated data
Source code in toast/ops/demodulation.py
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toast.ops.StokesWeightsDemod
Bases: Operator
Compute the Stokes pointing weights for demodulated data
Source code in toast/ops/demodulation.py
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Pointing Matrix
toast.ops.PointingDetectorSimple
Bases: Operator
Operator which translates boresight pointing into detector frame
Source code in toast/ops/pointing_detector/pointing_detector.py
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toast.ops.PixelsHealpix
Bases: Operator
Operator which generates healpix pixel numbers.
If the view trait is not specified, then this operator will use the same data view as the detector pointing operator when computing the pointing matrix pixels.
Any samples with "bad" pointing should have already been set to a "safe" quaternion value by the detector pointing operator. We use the same shared flags as the detector pointing operator.
Source code in toast/ops/pixels_healpix/pixels_healpix.py
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toast.ops.PixelsWCS
Bases: Operator
Operator which generates detector pixel indices defined on a flat projection.
When placing the projection on the sky, either the center or bounds
traits must be specified, but not both.
When determining the pixel density in the projection, exactly two traits from the
set of bounds, resolution and dimensions must be specified.
If the view trait is not specified, then this operator will use the same data view as the detector pointing operator when computing the pointing matrix pixels.
This uses the astropy wcs utilities to build the projection parameters. Eventually
this operator will use internal kernels for the projection unless use_astropy
is set to True.
Source code in toast/ops/pixels_wcs.py
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create_wcs(coord='EQU', proj='CAR', center_deg=None, bounds_deg=None, res_deg=None, dims=None)
classmethod
Create a WCS object given projection parameters.
Either the center_deg or bounds_deg parameters must be specified,
but not both.
When determining the pixel density in the projection, exactly two
parameters from the set of bounds_deg, res_deg and dims must be
specified.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
coord
|
str
|
The coordinate frame name. |
'EQU'
|
proj
|
str
|
The projection type. |
'CAR'
|
center_deg
|
tuple
|
The (lon, lat) projection center in degrees. |
None
|
bounds_deg
|
tuple
|
The (lon_min, lon_max, lat_min, lat_max) values in degrees. |
None
|
res_deg
|
tuple
|
The (lon, lat) resolution in degrees. |
None
|
dims
|
tuple
|
The (lon, lat) projection size in pixels. |
None
|
Returns:
| Type | Description |
|---|---|
(WCS, shape)
|
The instantiated WCS object and final shape. |
Source code in toast/ops/pixels_wcs.py
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toast.ops.StokesWeights
Bases: Operator
Operator which generates I/Q/U pointing weights.
Given the individual detector pointing, this computes the pointing weights assuming that the detector is a linear polarizer followed by a total power measurement. By definition, the detector coordinate frame has the X-axis aligned with the polarization sensitive direction. An optional dictionary of pointing weight calibration factors may be specified for each observation.
If the hwp_angle field is specified, then an ideal HWP Mueller matrix is inserted in the optics chain before the linear polarizer. In this case, the fp_gamma key name must be specified and each detector must have a value in the focalplane table.
The timestream model without a HWP in COSMO convention is:
.. math:: d = cal \left[I + \frac{1 - \epsilon}{1 + \epsilon} \left[Q \cos\left(2\alpha\right) + U \sin\left(2\alpha\right) \right] \right]
When a HWP is present, we have:
.. math:: d = cal \left[I + \frac{1 - \epsilon}{1 + \epsilon} \left[Q \cos\left(2(\alpha - 2\omega) \right) - U \sin\left(2(\alpha - 2\omega) \right) \right] \right]
The detector orientation angle "alpha" in COSMO convention is measured in a right-handed sense from the local meridian and the HWP angle "omega" is also measured from the local meridian. The omega value can be described in terms of alpha, a fixed per-detector offset gamma, and the time varying HWP angle measured from the focalplane coordinate frame X-axis:
.. math:: \omega = \alpha + {\gamma}{HWP}(t) - {\gamma}{DET}
See documentation for a full treatment of this math.
By default, this operator uses the "COSMO" convention for Q/U. If the "IAU" trait is set to True, then resulting weights will differ by the sign of the U Stokes weight.
If the view trait is not specified, then this operator will use the same data view as the detector pointing operator when computing the pointing matrix pixels and weights.
Source code in toast/ops/stokes_weights/stokes_weights.py
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Scan Strategy Characterization
toast.ops.CadenceMap
Bases: Operator
Tabulate which days each pixel on the map is visited.
Source code in toast/ops/cadence_map.py
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toast.ops.CrossLinking
Bases: Operator
Evaluate an ACT-style crosslinking map
The result is a 3-component map that needs to be processed as crosslinking = SQRT(map[1]2 + map[2]2) / map[0] for the crosslinking statistic. This is not done in the operator to allow adding crosslinking maps together.
Source code in toast/ops/crosslinking.py
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Noise Estimation
toast.ops.NoiseEstim
Bases: Operator
Noise estimation operator
Source code in toast/ops/noise_estimation.py
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decimate(signal, flags)
Downsample previously highpass-filtered signal
Source code in toast/ops/noise_estimation.py
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process_noise_estimate(obs, global_intervals, signal1, signal2, flags, timestamps, fsample, fileroot, det1, det2, lagmax)
Measure the sample (cross) covariance in the signal-subtracted TOD and Fourier-transform it for noise PSD.
Source code in toast/ops/noise_estimation.py
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toast.ops.FitNoiseModel
Bases: Operator
Perform a least squares fit to an existing noise model.
This takes an existing estimated noise model and attempts to fit each spectrum to 1/f parameters.
If the output model is not specified, then the input is modified in place.
If the data has been filtered with a low-pass, then the high frequency spectral points are not representative of the actual white noise plateau. In this case, The min / max frequencies to consider can be specified.
Source code in toast/ops/noise_model.py
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toast.ops.FlagNoiseFit
Bases: Operator
Operator which flags detectors that have outlier noise properties.
Source code in toast/ops/noise_model.py
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toast.ops.SignalDiffNoiseModel
Bases: Operator
Evaluate a simple white noise model based on consecutive sample differences.
Source code in toast/ops/signal_diff_noise_model.py
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Map Making
Utilities
toast.ops.BuildPixelDistribution
Bases: Operator
Operator which builds the pixel distribution information.
This operator runs the pointing operator and builds the PixelDist instance describing how submaps are distributed among processes. This requires expanding the full detector pointing once in order to compute the distribution. This is done one detector at a time unless the save_pointing trait is set to True.
NOTE: The pointing operator must have the "pixels" and "create_dist" traits, which will be set by this operator during execution.
Output PixelDistribution objects are stored in the Data dictionary.
Source code in toast/ops/pointing.py
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toast.ops.BuildHitMap
Bases: Operator
Operator which builds a hitmap.
Given the pointing matrix for each detector, accumulate the hit map. The PixelData object containing the hit map is returned by the finalize() method.
If any samples have compromised telescope pointing, those pixel indices should have already been set to a negative value by the operator that generated the pointing matrix.
Although individual detector flags do not impact the pointing per se, they can be used with this operator in order to produce a hit map that is consistent with other pixel space products. The detector mask defaults to cutting "non-science" samples.
Source code in toast/ops/mapmaker_utils/mapmaker_utils.py
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toast.ops.BuildInverseCovariance
Bases: Operator
Operator which builds a pixel-space diagonal inverse noise covariance.
Given the pointing matrix and noise model for each detector, accumulate the inverse noise covariance:
.. math:: N_pp'^{-1} = \left( P^T N_tt'^{-1} P \right)
The PixelData object containing this is returned by the finalize() method.
If any samples have compromised telescope pointing, those pixel indices should have already been set to a negative value by the operator that generated the pointing matrix. Individual detector flags can optionally be applied to timesamples when accumulating data. The detector mask defaults to cutting "non-science" samples.
Source code in toast/ops/mapmaker_utils/mapmaker_utils.py
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toast.ops.BuildNoiseWeighted
Bases: Operator
Operator which builds a noise-weighted map.
Given the pointing matrix and noise model for each detector, accumulate the noise weighted map:
.. math:: Z_p = P^T N_tt'^{-1} d
Which is the timestream data waited by the diagonal time domain noise covariance and projected into pixel space. The PixelData object containing this is returned by the finalize() method.
If any samples have compromised telescope pointing, those pixel indices should have already been set to a negative value by the operator that generated the pointing matrix. Individual detector flags can optionally be applied to timesamples when accumulating data. The detector mask defaults to cutting "non-science" samples.
Source code in toast/ops/mapmaker_utils/mapmaker_utils.py
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toast.ops.CovarianceAndHits
Bases: Operator
Operator which builds the pixel-space diagonal noise covariance and hit map.
Frequently the first step in map making is to determine what pixels on the sky have been covered and build the diagonal noise covariance. During the construction of the covariance we can cut pixels that are poorly conditioned.
This operator runs the pointing operator and builds the PixelDist instance describing how submaps are distributed among processes. It builds the hit map and the inverse covariance and then inverts this with a threshold on the condition number in each pixel. The detector flag mask defaults to cutting "non-science" samples.
NOTE: The pixel pointing operator must have the "pixels", "create_dist" traits, which will be set by this operator during execution.
Output PixelData objects are stored in the Data dictionary.
Source code in toast/ops/mapmaker_utils/mapmaker_utils.py
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toast.ops.NoiseWeight
Bases: Operator
Apply diagonal noise weighting to detector data.
This simple operator takes the detector weight from the specified noise model and applies it to the timestream values. We ignore all detector flags in this operator, since there is no harm in multiplying the noise weight by values in invalid samples.
Source code in toast/ops/noise_weight/noise_weight.py
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toast.ops.BinMap
Bases: Operator
Operator which bins a map.
Given a noise model and a pointing operator, build the noise weighted map and apply the noise covariance to get resulting binned map.
Source code in toast/ops/mapmaker_binning.py
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Observation Matrices
toast.ops.ObsMat
Bases: object
Observation Matrix class
Source code in toast/ops/obsmat.py
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toast.ops.FilterBin
Bases: Operator
FilterBin builds a template matrix and projects out compromised modes. It then bins the signal and optionally writes out the sparse observation matrix that matches the filtering operations. FilterBin supports deprojection templates.
THIS OPERATOR ASSUMES OBSERVATIONS ARE DISTRIBUTED BY DETECTOR WITHIN A GROUP
Source code in toast/ops/filterbin.py
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toast.ops.combine_observation_matrix(rootname)
Combine slices of the observation matrix into a single scipy sparse matrix file
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
rootname (str)
|
rootname of the matrix slices. Typically
|
required |
Returns:
filename_matrix (str) : Name of the composed matrix file,
{rootname}.npz.
Source code in toast/ops/filterbin.py
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toast.ops.coadd_observation_matrix(inmatrix, outmatrix, file_invcov=None, file_cov=None, nside_submap=16, rcond_limit=0.001, double_precision=False, comm=None)
Co-add noise-weighted observation matrices
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
inmatrix(iterable)
|
One or more noise-weighted observation
matrix files. If a matrix is used to model several similar
observations, append |
required | |
outmatrix(string)
|
Name of output file. If it includes the string 'noiseweighted', the output matrix will be noise-weighted like the inputs. |
required | |
file_invcov(string)
|
Name of output inverse covariance file |
required | |
file_cov(string)
|
Name of output covariance file |
required | |
nside_submap(int)
|
Submap size is 12 * nside_submap ** 2. Number of submaps is (nside / nside_submap) ** 2 |
required | |
rcond_limit(float)
|
"Reciprocal condition number limit |
required | |
double_precision(bool)
|
Output in double precision |
required |
Source code in toast/ops/obsmat.py
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Template Regression
toast.templates.Amplitudes
Bases: AcceleratorObject
Class for distributed template amplitudes.
In the general case, template amplitudes exist as sparse, non-unique values across all processes. This object provides methods for describing the local distribution of amplitudes and for doing global reductions and dot products.
There are 4 supported cases:
1. If n_global == n_local, then every process has a full copy of the amplitude
values.
2. If n_global != n_local and both local_indices and local_ranges are None,
then every process has a disjoint set of amplitudes. The sum of n_local
across all processes must equal n_global.
3. If n_global != n_local and local_ranges is not None, then local_ranges
specifies the contiguous global slices that are concatenated to form the
local data. The sum of the lengths of the slices must equal n_local.
4. If n_global != n_local and local_indices is not None, then local_indices
is an array of the global indices of all the local data. The length of
local_indices must equal n_local. WARNING: this case is more costly in
terms of storage and reduction. Avoid it if possible.
Because different process groups have different sets of observations, there are some types of templates which may only have shared amplitudes within the group communicator. If use_group is True, the group communicator is used instead of the world communicator, and n_global is interpreted as the number of amplitudes in the group. This information is needed whenever working with the full set of amplitudes (for example when doing I/O).
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
comm
|
Comm
|
The toast communicator. |
required |
n_global
|
int
|
The number of global values across all processes. |
required |
n_local
|
int
|
The number of values on this process. |
required |
local_indices
|
array
|
If not None, the explicit indices of the local amplitudes within the global array. |
None
|
local_ranges
|
list
|
If not None, a list of tuples with the (offset, n_amp) amplitude ranges stored locally. |
None
|
dtype
|
dtype
|
The amplitude dtype. |
float64
|
use_group
|
bool
|
If True, use the group rather than world communicator. |
False
|
Source code in toast/templates/amplitudes.py
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comm
property
The toast communicator in use.
local_indices
property
The global indices of the local amplitudes, or None.
local_ranges
property
The global slices covered by local amplitudes, or None.
n_global
property
The total number of amplitudes.
n_local
property
The number of locally stored amplitudes.
n_local_flagged
property
The number of local amplitudes that are flagged.
use_group
property
Whether to use the group communicator rather than the global one.
clear()
Delete the underlying memory.
This will forcibly delete the C-allocated memory and invalidate all python references to this object. DO NOT CALL THIS unless you are sure all references are no longer being used and you are about to delete the object.
Source code in toast/templates/amplitudes.py
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dot(other, comm_bytes=10000000)
Perform a dot product with another Amplitudes object.
The other instance must have the same data distribution. The two objects are assumed to have already been synchronized, so that any amplitudes that exist on multiple processes have the same values. This further assumes that any flagged amplitudes have been set to zero.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
other
|
Amplitudes
|
The other instance. |
required |
comm_bytes
|
int
|
The maximum number of bytes to communicate in each call to Allreduce. Only used in the case of explicitly indexed amplitudes on each process. |
10000000
|
Result
(float): The dot product.
Source code in toast/templates/amplitudes.py
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duplicate()
Return a copy of the data.
Source code in toast/templates/amplitudes.py
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reset()
Set all amplitude values to zero.
Source code in toast/templates/amplitudes.py
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reset_flags()
Set all flag values to zero.
Source code in toast/templates/amplitudes.py
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sync(comm_bytes=10000000)
Perform an Allreduce across all processes.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
comm_bytes
|
int
|
The maximum number of bytes to communicate in each call to Allreduce. |
10000000
|
Returns:
| Type | Description |
|---|---|
|
None |
Source code in toast/templates/amplitudes.py
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toast.templates.AmplitudesMap
Bases: MutableMapping, AcceleratorObject
Helper class to provide arithmetic operations on a collection of Amplitudes.
This simply provides syntactic sugar to reduce duplicated code when working with a collection of Amplitudes in the map making.
Source code in toast/templates/amplitudes.py
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dot(other)
Dot product of all corresponding Amplitudes.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
other
|
AmplitudesMap
|
The other instance. |
required |
Result
(float): The dot product.
Source code in toast/templates/amplitudes.py
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duplicate()
Return a copy of the data.
Source code in toast/templates/amplitudes.py
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reset()
Set all amplitude values to zero.
Source code in toast/templates/amplitudes.py
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reset_flags()
Set all flag values to zero.
Source code in toast/templates/amplitudes.py
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toast.templates.Template
Bases: TraitConfig
Base class for timestream templates.
A template defines a mapping to / from timestream values to a set of template amplitudes. These amplitudes are usually quantities being solved as part of the map-making. Examples of templates might be destriping baseline offsets, azimuthally binned ground pickup, etc.
The template amplitude data may be distributed in a variety of ways. For some types of templates, every process may have their own unique set of amplitudes based on the data that they have locally. In other cases, every process may have a full local copy of all template amplitudes. There might also be cases where each process has a non-unique subset of amplitude values (similar to the way that pixel domain quantities are distributed).
Source code in toast/templates/template.py
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add_prior(amplitudes_in, amplitudes_out, use_accel=None, **kwargs)
Apply the inverse amplitude covariance as a prior.
This performs:
.. math:: a' += {C_a}^{-1} \cdot a
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
amplitudes_in
|
Amplitudes
|
The input Amplitude values for this template. |
required |
amplitudes_out
|
Amplitudes
|
The input Amplitude values for this template. |
required |
Returns:
| Type | Description |
|---|---|
|
None |
Source code in toast/templates/template.py
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add_to_signal(detector, amplitudes, use_accel=None, **kwargs)
Accumulate the projected amplitudes to a timestream.
This performs the operation:
.. math:: s += F \cdot a
Where s is the det_data signal, F is the template and a is the amplitudes.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
detector
|
str
|
The detector name. |
required |
amplitudes
|
Amplitudes
|
The Amplitude values for this template. |
required |
Returns:
| Type | Description |
|---|---|
|
None |
Source code in toast/templates/template.py
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apply_precond(amplitudes_in, amplitudes_out, use_accel=None, **kwargs)
Apply the template preconditioner.
Formally, the preconditioner "M" is an approximation to the "design matrix" (the "A" matrix in "Ax = b"). This function applies the inverse preconditioner to the template amplitudes:
.. math:: a' += M^{-1} \cdot a
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
amplitudes_in
|
Amplitudes
|
The input Amplitude values for this template. |
required |
amplitudes_out
|
Amplitudes
|
The input Amplitude values for this template. |
required |
Returns:
| Type | Description |
|---|---|
|
None |
Source code in toast/templates/template.py
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detectors()
Return a list of detectors supported by the template.
This list will change whenever the data trait is set, which initializes
the template.
Returns:
| Type | Description |
|---|---|
list
|
The detectors with local amplitudes across all observations. |
Source code in toast/templates/template.py
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get_class_config(input=None)
classmethod
Return a dictionary of the default traits of an Template class.
This returns a new or appended dictionary. The class instance properties are contained in a dictionary found in result["templates"][cls.name].
If the specified named location in the input config already exists then an exception is raised.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
input
|
dict
|
The optional input dictionary to update. |
None
|
Returns:
| Type | Description |
|---|---|
dict
|
The created or updated dictionary. |
Source code in toast/templates/template.py
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get_config(input=None)
Return a dictionary of the current traits of a Template instance.
This returns a new or appended dictionary. The operator instance properties are contained in a dictionary found in result["templates"][self.name].
If the specified named location in the input config already exists then an exception is raised.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
input
|
dict
|
The optional input dictionary to update. |
None
|
Returns:
| Type | Description |
|---|---|
dict
|
The created or updated dictionary. |
Source code in toast/templates/template.py
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project_signal(detector, amplitudes, use_accel=None, **kwargs)
Project a timestream into template amplitudes.
This performs:
.. math:: a += F^T \cdot s
Where s is the det_data signal, F is the template and a is the amplitudes.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
detector
|
str
|
The detector name. |
required |
amplitudes
|
Amplitudes
|
The Amplitude values for this template. |
required |
Returns:
| Type | Description |
|---|---|
|
None |
Source code in toast/templates/template.py
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translate(props)
classmethod
Given a config dictionary, modify it to match the current API.
Source code in toast/templates/template.py
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zeros()
Return an Amplitudes object filled with zeros.
This returns an Amplitudes instance with appropriate dimensions for this
template. This will raise an exception if called before the data trait
is set.
Returns:
| Type | Description |
|---|---|
Amplitudes
|
Zero amplitudes. |
Source code in toast/templates/template.py
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toast.templates.Offset
Bases: Template
This class represents noise fluctuations as a step function.
Every process stores the amplitudes for its local data, which is disjoint from the amplitudes on other processes. We project amplitudes one detector at a time, and so we arrange our template amplitudes in "detector major" order and store offsets into this for each observation.
Source code in toast/templates/offset/offset.py
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clear()
Delete the underlying C-allocated memory.
Source code in toast/templates/offset/offset.py
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write(amplitudes, out)
Write out amplitude values.
This stores the amplitudes to files for debugging / plotting. Since the Offset amplitudes are unique on each process, we open one file per process group and each process in the group communicates their amplitudes to one writer.
Since this function is used mainly for debugging, we are a bit wasteful and duplicate the amplitudes in order to make things easier.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
amplitudes
|
Amplitudes
|
The amplitude data. |
required |
out
|
str
|
The output file root. |
required |
Returns:
| Type | Description |
|---|---|
|
None |
Source code in toast/templates/offset/offset.py
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toast.templates.Periodic
Bases: Template
This template represents amplitudes which are periodic in time.
The template amplitudes are modeled as a value for each detector of each observation in a "bin" of the specified data values. The min / max values of the periodic data are computed for each observation, and the binning between these min / max values is set by either the n_bins trait or by specifying the increment in the value to use for each bin.
Although the data values used do not have to be strictly periodic, this template works best if the values are varying in a regular way such that each bin has approximately the same number of hits.
The periodic quantity to consider can be either a shared or detdata field.
Source code in toast/templates/periodic.py
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write(amplitudes, out)
Write out amplitude values.
This stores the amplitudes to a file for debugging / plotting.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
amplitudes
|
Amplitudes
|
The amplitude data. |
required |
out
|
str
|
The output file. |
required |
Returns:
| Type | Description |
|---|---|
|
None |
Source code in toast/templates/periodic.py
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toast.templates.SubHarmonic
Bases: Template
This class represents sub-harmonic noise fluctuations.
Sub-harmonic means that the characteristic frequency of the noise modes is lower than 1/T where T is the length of the interval being fitted.
Every process stores the amplitudes for its local data, which is disjoint from the amplitudes on other processes. We project amplitudes one detector at a time, and so we arrange our template amplitudes in "detector major" order and store offsets into this for each observation.
Source code in toast/templates/subharmonic.py
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toast.templates.Fourier2D
Bases: Template
This class models 2D Fourier modes across the focalplane.
Since the modes are shared across detectors, our amplitudes are organized by observation and views within each observation. Each detector projection will traverse all the local amplitudes.
Source code in toast/templates/fourier2d.py
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clear()
Delete the underlying C-allocated memory.
Source code in toast/templates/fourier2d.py
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toast.templates.GainTemplate
Bases: Template
This class aims at fitting and mitigating gain fluctuations in the data.
The fluctuations are modeled as a linear combination of Legendre polynomials (up
to a given order, commonly n<5 ) weighted by the so called gain amplitudes.
The gain template is therefore obtained by estimating the polynomial amplitudes by
assuming a signal estimate provided by a template map (encoding a coarse estimate
of the underlying signal.)
Source code in toast/templates/gaintemplate.py
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toast.ops.TemplateMatrix
Bases: Operator
Operator for projecting or accumulating template amplitudes.
Source code in toast/ops/mapmaker_templates.py
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add_prior(amps_in, amps_out, use_accel=None, **kwargs)
Apply the noise prior from all templates to the amplitudes.
This can only be called after the operator has been used at least once so that the templates are initialized.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
amps_in
|
AmplitudesMap
|
The input amplitudes. |
required |
amps_out
|
AmplitudesMap
|
The output amplitudes, modified in place. |
required |
Returns:
| Type | Description |
|---|---|
|
None |
Source code in toast/ops/mapmaker_templates.py
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apply_precond(amps_in, amps_out, use_accel=None, **kwargs)
Apply the preconditioner from all templates to the amplitudes.
This can only be called after the operator has been used at least once so that the templates are initialized.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
amps_in
|
AmplitudesMap
|
The input amplitudes. |
required |
amps_out
|
AmplitudesMap
|
The output amplitudes, modified in place. |
required |
Returns:
| Type | Description |
|---|---|
|
None |
Source code in toast/ops/mapmaker_templates.py
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duplicate()
Make a shallow copy which contains the same list of templates.
This is useful when we want to use both a template matrix and its transpose in the same pipeline.
Returns:
| Type | Description |
|---|---|
TemplateMatrix
|
A new instance with the same templates. |
Source code in toast/ops/mapmaker_templates.py
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reset()
Reset templates to allow re-initialization on a new Data object.
Source code in toast/ops/mapmaker_templates.py
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reset_templates()
Mark templates to be re-initialized on next call to exec().
Source code in toast/ops/mapmaker_templates.py
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toast.ops.SolveAmplitudes
Bases: Operator
Solve for template amplitudes.
This operator solves for a maximum likelihood set of template amplitudes that model the timestream contributions from noise, systematics, etc:
.. math:: \left[ M^T N^{-1} Z M + M_p \right] a = M^T N^{-1} Z d
Where a are the solved amplitudes and d is the input data. N is the
diagonal time domain noise covariance. M is a matrix of templates that
project from the amplitudes into the time domain, and the Z operator is given
by:
.. math:: Z = I - P (P^T N^{-1} P)^{-1} P^T N^{-1}
or in terms of the binning operation:
.. math:: Z = I - P B
Where P is the pointing matrix. This operator takes one operator for the
template matrix M and one operator for the binning, B. It then
uses a conjugate gradient solver to solve for the amplitudes.
Source code in toast/ops/mapmaker_templates.py
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High Level Tools
toast.ops.Calibrate
Bases: Operator
Operator for calibrating timestreams using solved templates.
This operator first solves for a maximum likelihood set of template amplitudes that model the timestream contributions from noise, systematics, etc:
.. math:: \left[ M^T N^{-1} Z M + M_p \right] a = M^T N^{-1} Z d
Where a are the solved amplitudes and d is the input data. N is the
diagonal time domain noise covariance. M is a matrix of templates that
project from the amplitudes into the time domain, and the Z operator is given
by:
.. math:: Z = I - P (P^T N^{-1} P)^{-1} P^T N^{-1}
or in terms of the binning operation:
.. math:: Z = I - P B
Where P is the pointing matrix. This operator takes one operator for the
template matrix M and one operator for the binning, B. It then
uses a conjugate gradient solver to solve for the amplitudes.
After solving for the template amplitudes, they are projected into the time domain and the input data is element-wise divided by this.
If the result trait is not set, then the input is overwritten.
Source code in toast/ops/mapmaker.py
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toast.ops.MapMaker
Bases: Operator
Operator for making maps.
This operator first solves for a maximum likelihood set of template amplitudes that model the timestream contributions from noise, systematics, etc:
.. math:: \left[ M^T N^{-1} Z M + M_p \right] a = M^T N^{-1} Z d
Where a are the solved amplitudes and d is the input data. N is the
diagonal time domain noise covariance. M is a matrix of templates that
project from the amplitudes into the time domain, and the Z operator is given
by:
.. math:: Z = I - P (P^T N^{-1} P)^{-1} P^T N^{-1}
or in terms of the binning operation:
.. math:: Z = I - P B
Where P is the pointing matrix. This operator takes one operator for the
template matrix M and one operator for the binning, B. It then
uses a conjugate gradient solver to solve for the amplitudes.
After solving for the template amplitudes, a final map of the signal estimate is computed using a simple binning:
.. math:: MAP = ({P'}^T N^{-1} P')^{-1} {P'}^T N^{-1} (y - M a)
Where the "prime" indicates that this final map might be computed using a different pointing matrix than the one used to solve for the template amplitudes.
The template-subtracted detector timestreams are saved either in the input
det_data key of each observation, or (if overwrite == False) in an obs.detdata
key based on the name of this class instance.
Source code in toast/ops/mapmaker.py
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External Tools
toast.ops.Madam
Bases: Operator
Operator which passes data to libmadam for map-making.
Source code in toast/ops/madam.py
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clear()
Delete the underlying memory.
This will forcibly delete the C-allocated memory and invalidate all python references to the buffers.
Source code in toast/ops/madam.py
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toast.ops.madam_params_from_mapmaker(mapmaker)
Utility function that configures Madam to match the TOAST mapmaker
Source code in toast/ops/madam.py
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