Simulation Tools
TOAST contains a variety of Operators and other tools for simulating telescope observations and different detector signals.
Simulated Observing
When designing new telescopes or observing strategies the TOAST scheduler can be used to
create schedule files that can be passed to the SimGround and SimSatellite
operators.
Ground-Based Schedules
Sky Patches
To-Do
We can't add docs for the patch types, because they have no docstrings...
Scheduling Utilities
To-Do
Do we want more of the low-level tools here?
toast.schedule_sim_ground.parse_patches(args, observer, sun, moon, start_timestamp, stop_timestamp)
Source code in toast/schedule_sim_ground.py
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toast.schedule_sim_ground.build_schedule(args, start_timestamp, stop_timestamp, patches, observer, sun, moon)
Source code in toast/schedule_sim_ground.py
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Generating the Schedule
toast.schedule_sim_ground.run_scheduler(opts=None)
Source code in toast/schedule_sim_ground.py
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Space-Based Schedules
Generating schedules for a satellite is conceptually simpler due to the constraints on spacecraft dynamics.
toast.schedule_sim_satellite.create_satellite_schedule(prefix='', mission_start=None, observation_time=10 * u.minute, gap_time=0 * u.minute, num_observations=1, prec_period=10 * u.minute, spin_period=2 * u.minute, site_name='space', telescope_name='satellite')
Generate a satellite observing schedule.
This creates a series of scans with identical lengths and rotation rates, as well as optional gaps between.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
prefix
|
str
|
The prefix for the name of each scan. |
''
|
mission_start
|
datetime
|
The overall start time of the schedule. |
None
|
observation_time
|
Quantity
|
The length of each observation. |
10 * minute
|
gap_time
|
Quantity
|
The time between observations. |
0 * minute
|
num_observations
|
int
|
The number of observations. |
1
|
prec_period
|
Quantity
|
The time for one revolution about the precession axis. |
10 * minute
|
spin_period
|
Quantity
|
The time for one revolution about the spin axis. |
2 * minute
|
site_name
|
str
|
The name of the site to include in the schedule. |
'space'
|
telescope_name
|
str
|
The name of the telescope to include in the schedule. |
'satellite'
|
Returns:
| Type | Description |
|---|---|
SatelliteSchedule
|
The resulting schedule. |
Source code in toast/schedule_sim_satellite.py
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Creating Observations
toast.ops.SimGround
Bases: Operator
Simulate a generic ground-based telescope scanning.
This simulates ground-based pointing in constant elevation scans for a telescope located at a particular site and using an pre-created schedule.
The created observations define several interval lists to describe regions where the telescope is scanning left, right or in a turnaround or El-nod. A shared flag array is also created with bits sets for these same properties.
The telescope file, if specified, can reference an HDF5 data dump by specifying the internal path within the file. For example:
telescope_file="/path/to/data.h5:/obs1/instrument"
Source code in toast/ops/sim_ground.py
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toast.ops.SimSatellite
Bases: Operator
Simulate a generic satellite motion.
This simulates satellite pointing in regular intervals ("science scans") that may have some gaps in between for cooler cycles or other events. The precession axis (anti-sun direction) is continuously slewed.
To be consistent with the ground simulation facilities, the satellite pointing is expressed in the ICRS (equatorial) system by default. Detector pointing expansion can rotate the output pointing to any other reference frame.
The telescope file, if specified, can reference an HDF5 data dump by specifying the internal path within the file. For example:
telescope_file="/path/to/data.h5:/obs1/instrument"
Source code in toast/ops/sim_satellite.py
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Sky Signals
These operators generate detector data containing sources of power from outside the Earth's atmosphere.
toast.ops.SimDipole
Bases: Operator
Operator which generates dipole signal for detectors.
This uses the detector pointing, the telescope velocity vectors, and the solar system motion with respect to the CMB rest frame to compute the observed CMB dipole signal. The dipole timestream is either added (default) or subtracted from the specified detector data.
The telescope velocity and detector quaternions are assumed to be in the same coordinate system.
The "mode" trait determines what components of the telescope motion are included in the observed dipole. Valid options are 'solar' for just the solar system motion, 'orbital' for just the motion of the telescope with respect to the solarsystem barycenter, and 'total' which is the sum of both (and the default).
Source code in toast/ops/sim_tod_dipole.py
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Beam-Convolved Sky
toast.ops.SimConviqt
Bases: Operator
Operator which uses libconviqt to generate beam-convolved timestreams.
Source code in toast/ops/conviqt.py
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available
property
Return True if libconviqt is found in the library search path.
calibrate_signal(data, det, beam, convolved_data, verbose)
By default, libConviqt results returns a signal that conforms to TOD = (1 + epsilon) / 2 * intensity + (1 - epsilon) / 2 * polarization.
When calibrate = True, we rescale the TOD to TOD = intensity + (1 - epsilon) / (1 + epsilon) * polarization
Source code in toast/ops/conviqt.py
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get_buffer(theta, phi, psi, det, verbose)
Pack the pointing into the conviqt pointing array
Source code in toast/ops/conviqt.py
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get_detector(det)
We always create the detector with zero leakage and scale the returned TOD ourselves
Source code in toast/ops/conviqt.py
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get_pointing(data, det, verbose)
Return the detector pointing as ZYZ Euler angles without the polarization sensitive angle. These angles are to be compatible with Pxx or Dxx frame beam products
Source code in toast/ops/conviqt.py
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save(data, det, convolved_data, verbose)
Store the convolved data.
Source code in toast/ops/conviqt.py
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toast.ops.SimTEBConviqt
Bases: SimConviqt
Operator that uses libconviqt to generate beam-convolved timestreams. This operator should be used in presence of a spinning HWP which makes the beam time-dependent, constantly mapping the co- and cross-polar responses on to each other. In the parent class OpSimConviqt we assume the beam to be static.
The convolution is performed by coupling each IQU component of the signal propertly as:
:math:skyT_lm * beamT_lm, skyE_lm * Re{P}, skyB_lm * Im{P}.
FIXME : check above math
For extra details please refer to this note
Source code in toast/ops/conviqt.py
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toast.ops.SimWeightedConviqt
Bases: SimConviqt
Operator which uses libconviqt to generate beam-convolved timestreams. This operator should be used in presence of a spinning HWP which makes the beam time-dependent, constantly mapping the co- and cross polar responses on to each other. In OpSimConviqt we assume the beam to be static.
Source code in toast/ops/conviqt.py
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toast.ops.SimTotalconvolve
Bases: Operator
Operator which uses ducc0.totalconvolve to generate beam-convolved timestreams.
Source code in toast/ops/totalconvolve.py
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available
property
Return True if ducc0.totalconvolve is found in the library search path.
calibrate_signal(data, det, beam, convolved_data, verbose)
By default, libConviqt results returns a signal that conforms to TOD = (1 + epsilon) / 2 * intensity + (1 - epsilon) / 2 * polarization.
When calibrate = True, we rescale the TOD to TOD = intensity + (1 - epsilon) / (1 + epsilon) * polarization
Source code in toast/ops/totalconvolve.py
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get_buffer(theta, phi, psi, det, verbose)
Pack the pointing into the pointing array
Source code in toast/ops/totalconvolve.py
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get_lmmax(skyfile, beamfile)
Determine the actual lmax and beammmax to use for the convolution from class parameters and values in the files.
Source code in toast/ops/totalconvolve.py
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get_pointing(data, det, verbose)
Return the detector pointing as ZYZ Euler angles without the polarization sensitive angle. These angles are to be compatible with Pxx or Dxx frame beam products
Source code in toast/ops/totalconvolve.py
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save(data, det, convolved_data, verbose)
Store the convolved data.
Source code in toast/ops/totalconvolve.py
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Scanning a Healpix Map
toast.ops.ScanHealpixMap
Bases: Operator
Operator which reads a HEALPix format map from disk and scans it to a timestream.
The map file is loaded and distributed among the processes. For each observation, the pointing model is used to expand the pointing and scan the map values into detector data.
Source code in toast/ops/scan_healpix.py
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toast.ops.ScanHealpixMask
Bases: Operator
Operator which reads a HEALPix format mask from disk and scans it to a timestream.
The mask file is loaded and distributed among the processes. For each observation, the pointing model is used to expand the pointing and scan the mask values into detector data.
Source code in toast/ops/scan_healpix.py
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toast.ops.InterpolateHealpixMap
Bases: Operator
Operator which reads a HEALPix format map from disk and interpolates it to a timestream.
The map file is loaded and placed in shared memory on every participating node. For each observation, the pointing model is used to expand the pointing and bilinearly interpolate the map values into detector data.
Source code in toast/ops/interpolate_healpix.py
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Scanning a WCS Projected Map
toast.ops.ScanWCSMap
Bases: Operator
Operator which reads a WCS format map from disk and scans it to a timestream.
The map file is loaded and distributed among the processes. For each observation, the pointing model is used to expand the pointing and scan the map values into detector data.
Source code in toast/ops/scan_wcs.py
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toast.ops.ScanWCSMask
Bases: Operator
Operator which reads a WCS mask from disk and scans it to a timestream.
The mask file is loaded and distributed among the processes. For each observation, the pointing model is used to expand the pointing and scan the mask values into detector data.
Source code in toast/ops/scan_wcs.py
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Scanning an Arbitrary Map
toast.ops.ScanMap
Bases: Operator
Operator which uses the pointing matrix to scan timestream values from a map.
The map must be a PixelData instance with either float32 or float64 values. The values can either be accumulated or subtracted from the input timestream, and the input timestream can be optionally zeroed out beforehand.
Source code in toast/ops/scan_map/scan_map.py
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toast.ops.ScanMask
Bases: Operator
Operator which uses the pointing matrix to set timestream flags from a mask.
The mask must be a PixelData instance with an integer data type. The data for each pixel is bitwise-and combined with the mask_bits to form a result. For each detector sample crossing a pixel with a non-zero result, the detector flag is bitwise-or'd with the specified value.
Source code in toast/ops/scan_map/scan_map.py
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toast.ops.ScanScale
Bases: Operator
Operator which uses the pointing matrix to apply pixel weights to timestreams.
The map must be a PixelData instance with either float32 or float64 values and one value per pixel. The timestream samples are multiplied by their corresponding pixel values.
Source code in toast/ops/scan_map/scan_map.py
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Point Sources
toast.ops.SimCatalog
Bases: Operator
Operator that generates variable and static point source signal.
Signal is generated by sampling the provided beam map at appropriate locations and scaling the resulting signal to match the perceived intensity of the source.
Source SED is convolved with the detector bandpass recorded in the focalplane table.
Example catalog entries:
.. highlight:: toml .. code-block:: toml
[example_static_source]
# Celestial coordinate are always given in degrees
ra_deg = 30
dec_deg = -30
# the SED can be specified using an arbitrary number of
# frequency bins. The SED is interpolated in log-log space to
# convolve with the detector bandpass
# Use either `flux_density_mJy` or `flux_density_Jy` and adjust
# the values accordingly
freqs_ghz = [ 1.0, 1000.0,]
flux_density_mJy = [ 10.0, 1.0,]
# Omitting polarization fraction results in an
# unpolarized source
pol_frac = 0.1
pol_angle_deg = 0
[example_variable_source]
ra_deg = 30
dec_deg = -25
freqs_ghz = [ 1.0, 1000.0,]
# An arbitrary number of SED vectors can be provided but the
# location of the frequency bins is fixed. Effective SED is
# interpolated between the specified epochs.
flux_density_Jy = [ [ 10.0, 1.0,], [ 30.0, 10.0,], [ 10.0, 1.0,],]
# Omitting the times_mjd entry resuls in a static source
times_mjd = [ 59000.0, 60000.0, 61000.0,]
# The polarization properties can also vary
pol_frac = [ 0.05, 0.15, 0.05,]
pol_angle_deg = [ 45, 45, 45,]
[example_transient_source]
ra_deg = 30
dec_deg = -20
freqs_ghz = [ 1.0, 1000.0,]
flux_density_Jy = [ [ 10.0, 1.0,], [ 30.0, 10.0,],]
# Difference between a variable and transient source is
# simply that the specified epochs do not cover the entire
# simulation time span. The operator will not extrapolate
# outside the epochs.
times_mjd = [ 59410.0, 59411.0,]
Source code in toast/ops/sim_catalog.py
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Terrestrial Signals
These operators generate detector signal from the Earth's atmosphere and other sources of power outside a ground-based telescope.
toast.ops.WeatherModel
Bases: Operator
Create a default weather model
The weather model is used to draw observing conditions such as temperature, wind and PWV.
Source code in toast/ops/weather_model.py
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toast.ops.SimAtmosphere
Bases: Operator
Operator which generates atmosphere timestreams for detectors.
All processes collectively generate the atmospheric realization. Then each process passes through its local data and observes the atmosphere.
Source code in toast/ops/sim_tod_atm.py
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toast.ops.SimScanSynchronousSignal
Bases: Operator
Operator which generates scan-synchronous signal timestreams.
Source code in toast/ops/sss.py
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Instrument Signals
These operators simulate instrumental effects from sources of power inside the telescope and receiver.
toast.ops.DefaultNoiseModel
Bases: Operator
Create a default noise model from focalplane parameters.
A noise model is used by other operations such as simulating noise timestreams and also map making. This operator uses the detector properties from the focalplane in each observation to create a simple AnalyticNoise model.
Source code in toast/ops/noise_model.py
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toast.ops.ElevationNoise
Bases: Operator
Modify detector noise model based on elevation. Optionally include PWV modulation.
This adjusts the detector PSDs in a noise model based on the median elevation of each detector in each observation.
The PSD value scaled by:
.. math:: PSD_{new} = PSD_{old} * (a / sin(el) + c)^2
NOTE: since this operator generates a new noise model for all detectors, you should specify all detectors you intend to use downstream when calling exec().
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.
If the output model is not specified, then the input is modified in place.
Source code in toast/ops/elevation_noise.py
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toast.ops.SimNoise
Bases: Operator
Operator which generates noise timestreams.
This passes through each observation and every process generates data for its assigned samples. The observation unique ID is used in the random number generation.
This operator intentionally does not provide a "view" trait. To avoid discontinuities, the full observation must be simulated regardless of any data views that will be used for subsequent analysis.
Source code in toast/ops/sim_tod_noise.py
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toast.ops.CommonModeNoise
Bases: Operator
Modify noise model to include common modes
If the output model is not specified, then the input is modified in place.
Source code in toast/ops/common_mode_noise.py
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toast.ops.TimeConstant
Bases: Operator
Simple time constant filtering without flag checks.
Source code in toast/ops/time_constant.py
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toast.ops.InjectCosmicRays
Bases: Operator
Inject the cosmic rays signal into the TOD. So far we inject two kinds of cosmic ray noise:
Wafer noise, due to ~400 impacts per second in the wafer undistinguishable individually. For each observation and for each detector we inject low noise component as a white noise signal, i.e. noraml distributed random samples following the observed properties from simulations and read from disc. This component is then coadded to the sky signal (as if it were a noise term) .
Common mode noise
A common mode noise within each detector pair can be simulated given the properties of the wafer noise. Will use the informations of correlations can be found in the file provided as an input to the simulations, if present, otherwise 50% detector correlation is assumed.
Direct hits (or Glitches)
Given the size of the detector we can derive the cosmic ray event rate and simulate the profile of a cosmic ray glitch. We assume the glitch to be described as
.. math:: \gamma (t) = C_1 +C_2 e^{-t/\tau }
where :math:C_1 and :math:C_2 and the time constant :math: au are drawn from a distribution of estimated values
from simulations. For each observation and each detector, we estimate the number of hits expected
theroretically and draw a random integer, N, with a Poissonian distribution given the expected number
of events, Nexp. We then select randomly N timestamps where the hits will be injected into the tod simulated in TOAST.
Evaluate the function :math:\gamma at a higher sampling rate (~150 Hz), decimate it to the TOD sample rate and coadd it.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
crfile
|
string
|
A |
required |
signal_name
|
string
|
the cache reference of the TOD data where the cosmic ray will be stored |
required |
realization
|
int
|
to run several Monte-Carlo realizations of cosmic ray noise |
required |
eventrate (float)
|
the expected event rate of hits in a detector |
required | |
inject_direct_hits
|
bool
|
will include also direct hits if set to True |
required |
conversion_factor
|
float
|
factor to convert the cosmic ray units to temperature units |
required |
common_mode (bool)
|
will include also common mode per pixel pair if set to True |
required |
Source code in toast/ops/sim_cosmic_rays.py
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toast.ops.GainDrifter
Bases: Operator
Operator which injects gain drifts to the signal.
The drift can be injected into 3 different ways:
- linear_drift: inject a linear drift with a random slope for each detector
- slow_drift: inject a drift signal with a 1/f PSD, simulated up to
the frequencies<cutoff_freq, in case cutoff_freq< (1/t_obs), cutoff_freq=1/t_obs.
- thermal_drift: inject a drift encoding frequencies up to the sampling rate, to simulate
the thermal fluctuations in the focalplane.
Both slow_drift and thermal_drift modes encode the possibility to inject a common mode drifts
to all the detectors belonging to a group of detectors identified the string focalplane_group ( can
be any string set by the user used to identify the groups in the detector table).
The amount of common mode contribution is set by setting detector_mismatch to a value <1, (with
0 being the case with only injecting common mode signal).
Source code in toast/ops/sim_gaindrifts.py
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toast.ops.GainScrambler
Bases: Operator
Apply random gain errors to detector data.
This operator draws random gain errors from a given distribution and applies them to the specified detectors.
Source code in toast/ops/gainscrambler.py
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toast.ops.PerturbHWP
Bases: Operator
Operator that adds irregularities to HWP rotation
Source code in toast/ops/sim_hwp.py
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toast.ops.CrossTalk
Bases: Operator
Simulate readout crosstalk between channels.
-
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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toast.ops.YieldCut
Bases: Operator
Operator that simulates non-perfect yield.
When TES detectors have their bias tuned, not all detectors have sufficient responsivity to be useful for science. This can be a temporary problem. This operator simulates a random loss in detector yield.
The det_mask trait is used to select incoming "good" detectors. This selection
of good detectors then has the yield cut applied.
Source code in toast/ops/yield_cut.py
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