pycbc.inference.models package¶
Submodules¶
pycbc.inference.models.analytic module¶
This modules provides models that have analytic solutions for the log likelihood.
- class pycbc.inference.models.analytic.TestEggbox(variable_params, **kwargs)[source]¶
Bases:
BaseModel
The test distribution is an ‘eggbox’ function:
\[\log \mathcal{L}(\Theta) = \left[ 2+\prod_{i=1}^{n}\cos\left(\frac{\theta_{i}}{2}\right)\right]^{5}\]The number of dimensions is set by the number of
variable_params
that are passed.- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied.
**kwargs – All other keyword arguments are passed to
BaseModel
.
- name = 'test_eggbox'¶
- class pycbc.inference.models.analytic.TestNormal(variable_params, mean=None, cov=None, **kwargs)[source]¶
Bases:
BaseModel
The test distribution is an multi-variate normal distribution.
The number of dimensions is set by the number of
variable_params
that are passed. For details on the distribution used, seescipy.stats.multivariate_normal
.- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied.
mean (array-like, optional) – The mean values of the parameters. If None provide, will use 0 for all parameters.
cov (array-like, optional) – The covariance matrix of the parameters. If None provided, will use unit variance for all parameters, with cross-terms set to 0.
**kwargs – All other keyword arguments are passed to
BaseModel
.
Examples
Create a 2D model with zero mean and unit variance:
>>> m = TestNormal(['x', 'y'])
Set the current parameters and evaluate the log posterior:
>>> m.update(x=-0.2, y=0.1) >>> m.logposterior -1.8628770664093453
See the current stats that were evaluated:
>>> m.current_stats {'logjacobian': 0.0, 'loglikelihood': -1.8628770664093453, 'logprior': 0.0}
- name = 'test_normal'¶
- class pycbc.inference.models.analytic.TestPosterior(variable_params, posterior_file, nsamples, **kwargs)[source]¶
Bases:
BaseModel
Build a test posterior from a set of samples using a kde
- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied.
posterior_file (hdf file) – A compatible pycbc inference output file which posterior samples can be read from.
nsamples (int) – Number of samples to draw from posterior file to build KDE.
**kwargs – All other keyword arguments are passed to
BaseModel
.
- name = 'test_posterior'¶
- class pycbc.inference.models.analytic.TestPrior(variable_params, **kwargs)[source]¶
Bases:
BaseModel
Uses the prior as the test distribution.
- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied. Must have length 2.
**kwargs – All other keyword arguments are passed to
BaseModel
.
- name = 'test_prior'¶
- class pycbc.inference.models.analytic.TestRosenbrock(variable_params, **kwargs)[source]¶
Bases:
BaseModel
The test distribution is the Rosenbrock function:
\[\log \mathcal{L}(\Theta) = -\sum_{i=1}^{n-1}[ (1-\theta_{i})^{2}+100(\theta_{i+1} - \theta_{i}^{2})^{2}]\]The number of dimensions is set by the number of
variable_params
that are passed.- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied.
**kwargs – All other keyword arguments are passed to
BaseModel
.
- name = 'test_rosenbrock'¶
- class pycbc.inference.models.analytic.TestVolcano(variable_params, **kwargs)[source]¶
Bases:
BaseModel
The test distribution is a two-dimensional ‘volcano’ function:
\[\Theta = \sqrt{\theta_{1}^{2} + \theta_{2}^{2}} \log \mathcal{L}(\Theta) = 25\left(e^{\frac{-\Theta}{35}} + \frac{1}{2\sqrt{2\pi}} e^{-\frac{(\Theta-5)^{2}}{8}}\right)\]- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied. Must have length 2.
**kwargs – All other keyword arguments are passed to
BaseModel
.
- name = 'test_volcano'¶
pycbc.inference.models.base module¶
Base class for models.
- class pycbc.inference.models.base.BaseModel(variable_params, static_params=None, prior=None, sampling_transforms=None, waveform_transforms=None, **kwargs)[source]¶
Bases:
object
Base class for all models.
Given some model \(h\) with parameters \(\Theta\), Bayes Theorem states that the probability of observing parameter values \(\vartheta\) is:
\[p(\vartheta|h) = \frac{p(h|\vartheta) p(\vartheta)}{p(h)}.\]Here:
\(p(\vartheta|h)\) is the posterior probability;
\(p(h|\vartheta)\) is the likelihood;
\(p(\vartheta)\) is the prior;
\(p(h)\) is the evidence.
This class defines properties and methods for evaluating the log likelihood, log prior, and log posteror. A set of parameter values is set using the
update
method. Calling the class’slog(likelihood|prior|posterior)
properties will then evaluate the model at those parameter values.Classes that inherit from this class must implement a
_loglikelihood
function that can be called byloglikelihood
.- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied.
static_params (dict, optional) – A dictionary of parameter names -> values to keep fixed.
prior (callable, optional) – A callable class or function that computes the log of the prior. If None provided, will use
_noprior
, which returns 0 for all parameter values.sampling_params (list, optional) – Replace one or more of the
variable_params
with the given parameters for sampling.replace_parameters (list, optional) – The
variable_params
to replace with sampling parameters. Must be the same length assampling_params
.sampling_transforms (list, optional) – List of transforms to use to go between the
variable_params
and the sampling parameters. Required ifsampling_params
is not None.waveform_transforms (list, optional) – A list of transforms to convert the
variable_params
into something understood by the likelihood model. This is useful if the prior is more easily parameterized in parameters that are different than what the likelihood is most easily defined in. Since these are used solely for converting parameters, and not for rescaling the parameter space, a Jacobian is not required for these transforms.
- property current_params¶
- property current_stats¶
Return the
default_stats
as a dict.This does no computation. It only returns what has already been calculated. If a stat hasn’t been calculated, it will be returned as
numpy.nan
.- Returns:
Dictionary of stat names -> current stat values.
- Return type:
- property default_stats¶
The stats that
get_current_stats
returns by default.
- static extra_args_from_config(cp, section, skip_args=None, dtypes=None)[source]¶
Gets any additional keyword in the given config file.
- Parameters:
cp (WorkflowConfigParser) – Config file parser to read.
section (str) – The name of the section to read.
skip_args (list of str, optional) – Names of arguments to skip.
dtypes (dict, optional) – A dictionary of arguments -> data types. If an argument is found in the dict, it will be cast to the given datatype. Otherwise, the argument’s value will just be read from the config file (and thus be a string).
- Returns:
Dictionary of keyword arguments read from the config file.
- Return type:
- classmethod from_config(cp, **kwargs)[source]¶
Initializes an instance of this class from the given config file.
- Parameters:
cp (WorkflowConfigParser) – Config file parser to read.
**kwargs – All additional keyword arguments are passed to the class. Any provided keyword will over ride what is in the config file.
- get_current_stats(names=None)[source]¶
Return one or more of the current stats as a tuple.
This function does no computation. It only returns what has already been calculated. If a stat hasn’t been calculated, it will be returned as
numpy.nan
.
- property logjacobian¶
The log jacobian of the sampling transforms at the current postion.
If no sampling transforms were provided, will just return 0.
- Parameters:
**params – The keyword arguments should specify values for all of the variable args and all of the sampling args.
- Returns:
The value of the jacobian.
- Return type:
- property loglikelihood¶
The log likelihood at the current parameters.
This will initially try to return the
current_stats.loglikelihood
. If that raises anAttributeError
, will call _loglikelihood` to calculate it and store it tocurrent_stats
.
- property logposterior¶
Returns the log of the posterior of the current parameter values.
The logprior is calculated first. If the logprior returns
-inf
(possibly indicating a non-physical point), then theloglikelihood
is not called.
- property logprior¶
Returns the log prior at the current parameters.
- name = None¶
- static prior_from_config(cp, variable_params, static_params, prior_section, constraint_section)[source]¶
Gets arguments and keyword arguments from a config file.
- Parameters:
cp (WorkflowConfigParser) – Config file parser to read.
variable_params (list) – List of variable model parameter names.
static_params (dict) – Dictionary of static model parameters and their values.
prior_section (str) – Section to read prior(s) from.
constraint_section (str) – Section to read constraint(s) from.
- Returns:
The prior.
- Return type:
pycbc.distributions.JointDistribution
- prior_rvs(size=1, prior=None)[source]¶
Returns random variates drawn from the prior.
If the
sampling_params
are different from thevariable_params
, the variates are transformed to the sampling_params parameter space before being returned.- Parameters:
size (int, optional) – Number of random values to return for each parameter. Default is 1.
prior (JointDistribution, optional) – Use the given prior to draw values rather than the saved prior.
- Returns:
A field array of the random values.
- Return type:
- property sampling_params¶
Returns the sampling parameters.
If
sampling_transforms
is None, this is the same as thevariable_params
.
- property static_params¶
Returns the model’s static arguments.
- update(**params)[source]¶
Updates the current parameter positions and resets stats.
If any sampling transforms are specified, they are applied to the params before being stored.
- property variable_params¶
Returns the model parameters.
- write_metadata(fp, group=None)[source]¶
Writes metadata to the given file handler.
- Parameters:
fp (pycbc.inference.io.BaseInferenceFile instance) – The inference file to write to.
group (str, optional) – If provided, the metadata will be written to the attrs specified by group, i.e., to
fp[group].attrs
. Otherwise, metadata is written to the top-level attrs (fp.attrs
).
- class pycbc.inference.models.base.ModelStats[source]¶
Bases:
object
Class to hold model’s current stat values.
- getstats(names, default=nan)[source]¶
Get the requested stats as a tuple.
If a requested stat is not an attribute (implying it hasn’t been stored), then the default value is returned for that stat.
- getstatsdict(names, default=nan)[source]¶
Get the requested stats as a dictionary.
If a requested stat is not an attribute (implying it hasn’t been stored), then the default value is returned for that stat.
- property statnames¶
Returns the names of the stats that have been stored.
- class pycbc.inference.models.base.SamplingTransforms(variable_params, sampling_params, replace_parameters, sampling_transforms)[source]¶
Bases:
object
Provides methods for transforming between sampling parameter space and model parameter space.
- apply(samples, inverse=False)[source]¶
Applies the sampling transforms to the given samples.
- Parameters:
samples (dict or FieldArray) – The samples to apply the transforms to.
inverse (bool, optional) – Whether to apply the inverse transforms (i.e., go from the sampling args to the
variable_params
). Default is False.
- Returns:
The transformed samples, along with the original samples.
- Return type:
dict or FieldArray
- classmethod from_config(cp, variable_params)[source]¶
Gets sampling transforms specified in a config file.
Sampling parameters and the parameters they replace are read from the
sampling_params
section, if it exists. Sampling transforms are read from thesampling_transforms
section(s), usingtransforms.read_transforms_from_config
.An
AssertionError
is raised if nosampling_params
section exists in the config file.- Parameters:
cp (WorkflowConfigParser) – Config file parser to read.
variable_params (list) – List of parameter names of the original variable params.
- Returns:
A sampling transforms class.
- Return type:
- logjacobian(**params)[source]¶
Returns the log of the jacobian needed to transform pdfs in the
variable_params
parameter space to thesampling_params
parameter space.Let \(\mathbf{x}\) be the set of variable parameters, \(\mathbf{y} = f(\mathbf{x})\) the set of sampling parameters, and \(p_x(\mathbf{x})\) a probability density function defined over \(\mathbf{x}\). The corresponding pdf in \(\mathbf{y}\) is then:
\[p_y(\mathbf{y}) = p_x(\mathbf{x})\left|\mathrm{det}\,\mathbf{J}_{ij}\right|,\]where \(\mathbf{J}_{ij}\) is the Jacobian of the inverse transform \(\mathbf{x} = g(\mathbf{y})\). This has elements:
\[\mathbf{J}_{ij} = \frac{\partial g_i}{\partial{y_j}}\]This function returns \(\log \left|\mathrm{det}\,\mathbf{J}_{ij}\right|\).
- Parameters:
**params – The keyword arguments should specify values for all of the variable args and all of the sampling args.
- Returns:
The value of the jacobian.
- Return type:
- pycbc.inference.models.base.check_for_cartesian_spins(which, variable_params, static_params, waveform_transforms, cp, ignore)[source]¶
Checks that if any spin parameters exist, cartesian spins also exist.
This looks for parameters starting with
spinN
in the variable and static params, whereN
is either 1 or 2 (specified by thewhich
argument). If any parameters are found with those names, the params and the output of the waveform transforms are checked to see that there is at least one ofspinN(x|y|z)
. If not, aValueError
is raised.This check will not be done if the config file has an section given by the ignore argument.
- Parameters:
which ({1, 2}) – Which component to check for. Must be either 1 or 2.
variable_params (list) – List of the variable parameters.
static_params (dict) – The dictionary of static params.
waveform_transforms (list) – List of the transforms that will be applied to the variable and static params before being passed to the waveform generator.
cp (ConfigParser) – The config file.
ignore (str) – The section to check for in the config file. If the section is present in the config file, the check will not be done.
- pycbc.inference.models.base.read_sampling_params_from_config(cp, section_group=None, section='sampling_params')[source]¶
Reads sampling parameters from the given config file.
Parameters are read from the [({section_group}_){section}] section. The options should list the variable args to transform; the parameters they point to should list the parameters they are to be transformed to for sampling. If a multiple parameters are transformed together, they should be comma separated. Example:
[sampling_params] mass1, mass2 = mchirp, logitq spin1_a = logitspin1_a
Note that only the final sampling parameters should be listed, even if multiple intermediate transforms are needed. (In the above example, a transform is needed to go from mass1, mass2 to mchirp, q, then another one needed to go from q to logitq.) These transforms should be specified in separate sections; see
transforms.read_transforms_from_config
for details.- Parameters:
cp (WorkflowConfigParser) – An open config parser to read from.
section_group (str, optional) – Append {section_group}_ to the section name. Default is None.
section (str, optional) – The name of the section. Default is ‘sampling_params’.
- Returns:
sampling_params (list) – The list of sampling parameters to use instead.
replaced_params (list) – The list of variable args to replace in the sampler.
pycbc.inference.models.base_data module¶
Base classes for mofdels with data.
- class pycbc.inference.models.base_data.BaseDataModel(variable_params, data, recalibration=None, gates=None, injection_file=None, no_save_data=False, **kwargs)[source]¶
Bases:
BaseModel
Base class for models that require data and a waveform generator.
This adds propeties for the log of the likelihood that the data contain noise,
lognl
, and the log likelihood ratiologlr
.Classes that inherit from this class must define
_loglr
and_lognl
functions, in addition to the_loglikelihood
requirement inherited fromBaseModel
.- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied.
data (dict) – A dictionary of data, in which the keys are the detector names and the values are the data.
recalibration (dict of pycbc.calibration.Recalibrate, optional) – Dictionary of detectors -> recalibration class instances for recalibrating data.
gates (dict of tuples, optional) – Dictionary of detectors -> tuples of specifying gate times. The sort of thing returned by pycbc.gate.gates_from_cli.
injection_file (str, optional) – If an injection was added to the data, the name of the injection file used. If provided, the injection parameters will be written to file when
write_metadata
is called.**kwargs – All other keyword arguments are passed to
BaseModel
.
See
BaseModel
for additional attributes and properties.- property loglr¶
The log likelihood ratio at the current parameters, or the inner product <s|h> and <h|h> if set the flag self.return_sh_hh to be True.
This will initially try to return the
current_stats.loglr
. If that raises anAttributeError
, will call _loglr` to calculate it and store it tocurrent_stats
.
- property lognl¶
The log likelihood of the model assuming the data is noise.
This will initially try to return the
current_stats.lognl
. If that raises anAttributeError
, will call _lognl` to calculate it and store it tocurrent_stats
.
- property logplr¶
Returns the log of the prior-weighted likelihood ratio at the current parameter values.
The logprior is calculated first. If the logprior returns
-inf
(possibly indicating a non-physical point), thenloglr
is not called.
- write_metadata(fp, group=None)[source]¶
Adds data to the metadata that’s written.
- Parameters:
fp (pycbc.inference.io.BaseInferenceFile instance) – The inference file to write to.
group (str, optional) – If provided, the metadata will be written to the attrs specified by group, i.e., to
fp[group].attrs
. Otherwise, metadata is written to the top-level attrs (fp.attrs
).
pycbc.inference.models.brute_marg module¶
This module provides model classes that do brute force marginalization using at the likelihood level.
- class pycbc.inference.models.brute_marg.BruteLISASkyModesMarginalize(variable_params, cores=1, loop_polarization=False, base_model=None, **kwds)[source]¶
Bases:
BaseGaussianNoise
- classmethod from_config(cp, **kwargs)[source]¶
Initializes an instance of this class from the given config file.
In addition to
[model]
, adata_section
(default[data]
) must be in the configuration file. The data section specifies settings for loading data and estimating PSDs. See the online documentation for more details.The following options are read from the
[model]
section, in addition toname
(which must be set):{{DET}}-low-frequency-cutoff = FLOAT
: The low frequency cutoff to use for each detector {{DET}}. A cutoff must be provided for every detector that may be analyzed (any additional detectors are ignored).{{DET}}-high-frequency-cutoff = FLOAT
: (Optional) A high frequency cutoff for each detector. If not provided, the Nyquist frequency is used.check-for-valid-times =
: (Optional) If provided, will check that there are no data quality flags on during the analysis segment and the segment used for PSD estimation in each detector. To check for flags,pycbc.dq.query_flag()
is used, with settings pulled from thedq-*
options in the[data]
section. If a detector has bad data quality during either the analysis segment or PSD segment, it will be removed from the analysis.shift-psd-times-to-valid =
: (Optional) If provided, the segment used for PSD estimation will automatically be shifted left or right until a continous block of data with no data quality issues can be found. If no block can be found with a maximum shift of +/- the requested psd segment length, the detector will not be analyzed.err-on-missing-detectors =
: Raises an error if any detector is removed from the analysis because a valid time could not be found. Otherwise, a warning is printed to screen and the detector is removed from the analysis.normalize =
: (Optional) Turn on the normalization factor.ignore-failed-waveforms =
: Sets theignore_failed_waveforms
attribute.
- Parameters:
cp (WorkflowConfigParser) – Config file parser to read.
data_section (str, optional) – The name of the section to load data options from.
**kwargs – All additional keyword arguments are passed to the class. Any provided keyword will override what is in the config file.
- name = 'brute_lisa_sky_modes_marginalize'¶
- class pycbc.inference.models.brute_marg.BruteParallelGaussianMarginalize(variable_params, cores=10, base_model=None, marginalize_phase=None, **kwds)[source]¶
Bases:
BaseGaussianNoise
- name = 'brute_parallel_gaussian_marginalize'¶
pycbc.inference.models.data_utils module¶
Utilities for loading data for models.
- exception pycbc.inference.models.data_utils.NoValidDataError[source]¶
Bases:
Exception
This should be raised if a continous segment of valid data could not be found.
- pycbc.inference.models.data_utils.check_for_nans(strain_dict)[source]¶
Checks if any data in a dictionary of strains has NaNs.
If any NaNs are found, a
ValueError
is raised.- Parameters:
strain_dict (dict) – Dictionary of detectors ->
pycbc.types.timeseries.TimeSeries
.
- pycbc.inference.models.data_utils.check_validtimes(detector, gps_start, gps_end, shift_to_valid=False, max_shift=None, segment_name='DATA', **kwargs)[source]¶
Checks DQ server to see if the given times are in a valid segment.
If the
shift_to_valid
flag is provided, the times will be shifted left or right to try to find a continous valid block nearby. The shifting starts by shifting the times left by 1 second. If that does not work, it shifts the times right by one second. This continues, increasing the shift time by 1 second, until a valid block could be found, or until the shift size exceedsmax_shift
.If the given times are not in a continuous valid segment, or a valid block cannot be found nearby, a
NoValidDataError
is raised.- Parameters:
detector (str) – The name of the detector to query; e.g., ‘H1’.
gps_start (int) – The GPS start time of the segment to query.
gps_end (int) – The GPS end time of the segment to query.
shift_to_valid (bool, optional) – If True, will try to shift the gps start and end times to the nearest continous valid segment of data. Default is False.
max_shift (int, optional) – The maximum number of seconds to try to shift left or right to find a valid segment. Default is
gps_end - gps_start
.segment_name (str, optional) – The status flag to query; passed to
pycbc.dq.query_flag()
. Default is “DATA”.**kwargs – All other keyword arguments are passed to
pycbc.dq.query_flag()
.
- Returns:
use_start (int) – The start time to use. If
shift_to_valid
is True, this may differ from the given GPS start time.use_end (int) – The end time to use. If
shift_to_valid
is True, this may differ from the given GPS end time.
- pycbc.inference.models.data_utils.create_data_parser()[source]¶
Creates an argument parser for loading GW data.
- pycbc.inference.models.data_utils.data_from_cli(opts, check_for_valid_times=False, shift_psd_times_to_valid=False, err_on_missing_detectors=False)[source]¶
Loads the data needed for a model from the given command-line options.
Gates specifed on the command line are also applied.
- Parameters:
opts (ArgumentParser parsed args) – Argument options parsed from a command line string (the sort of thing returned by parser.parse_args).
check_for_valid_times (bool, optional) – Check that valid data exists in the requested gps times. Default is False.
shift_psd_times_to_valid (bool, optional) – If estimating the PSD from data, shift the PSD times to a valid segment if needed. Default is False.
err_on_missing_detectors (bool, optional) – Raise a NoValidDataError if any detector does not have valid data. Otherwise, a warning is printed, and that detector is skipped.
- Returns:
strain_dict (dict) – Dictionary of detectors -> time series strain.
psd_strain_dict (dict or None) – If
opts.psd_(start|end)_time
were set, a dctionary of detectors -> time series data to use for PSD estimation. Otherwise,None
.
- pycbc.inference.models.data_utils.data_opts_from_config(cp, section, filter_flow)[source]¶
Loads data options from a section in a config file.
- Parameters:
cp (WorkflowConfigParser) – Config file to read.
section (str) – The section to read. All options in the section will be loaded as-if they wre command-line arguments.
filter_flow (dict) – Dictionary of detectors -> inner product low frequency cutoffs. If a data-conditioning-low-freq cutoff wasn’t provided for any of the detectors, these values will be used. Otherwise, the data-conditioning-low-freq must be less than the inner product cutoffs. If any are not, a
ValueError
is raised.
- Returns:
opts – An argument parser namespace that was constructed as if the options were specified on the command line.
- Return type:
parsed argparse.ArgumentParser
- pycbc.inference.models.data_utils.detectors_with_valid_data(detectors, gps_start_times, gps_end_times, pad_data=None, err_on_missing_detectors=False, **kwargs)[source]¶
Determines which detectors have valid data.
- Parameters:
detectors (list of str) – Names of the detector names to check.
gps_start_times (dict) – Dictionary of detector name -> start time listing the GPS start times of the segment to check for each detector.
gps_end_times (dict) – Dictionary of detector name -> end time listing the GPS end times of the segment to check for each detector.
pad_data (dict, optional) – Dictionary of detector name -> pad time to add to the beginning/end of the GPS start/end times before checking. A pad time for every detector in
detectors
must be given. Default (None) is to apply no pad to the times.err_on_missing_detectors (bool, optional) – If True, a
NoValidDataError
will be raised if any detector does not have continous valid data in its requested segment. Otherwise, the detector will not be included in the returned list of detectors with valid data. Default is False.**kwargs – All other keyword arguments are passed to
check_validtimes
.
- Returns:
A dictionary of detector name -> valid times giving the detectors with valid data and their segments. If
shift_to_valid
was passed tocheck_validtimes
this may not be the same as the input segments. If no valid times could be found for a detector (anderr_on_missing_detectors
is False), it will not be included in the returned dictionary.- Return type:
- pycbc.inference.models.data_utils.fd_data_from_strain_dict(opts, strain_dict, psd_strain_dict=None)[source]¶
Converts a dictionary of time series to the frequency domain, and gets the PSDs.
- Parameters:
opts (ArgumentParser parsed args) – Argument options parsed from a command line string (the sort of thing returned by parser.parse_args).
strain_dict (dict) – Dictionary of detectors -> time series data.
psd_strain_dict (dict, optional) – Dictionary of detectors -> time series data to use for PSD estimation. If not provided, will use the
strain_dict
. This is ignored ifopts.psd_estimation
is not set. Seepycbc.psd.psd_from_cli_multi_ifos()
for details.
- Returns:
stilde_dict (dict) – Dictionary of detectors -> frequency series data.
psd_dict (dict) – Dictionary of detectors -> frequency-domain PSDs.
- pycbc.inference.models.data_utils.gate_overwhitened_data(stilde_dict, psd_dict, gates)[source]¶
Applies gates to overwhitened data.
- Parameters:
- Returns:
Dictionary of detectors -> frequency series data with the gates applied after overwhitening. The returned data is not overwhitened.
- Return type:
- pycbc.inference.models.data_utils.strain_from_cli_multi_ifos(*args, **kwargs)[source]¶
Wrapper around strain.from_cli_multi_ifos that tries a few times before quiting.
When running in a parallel environment, multiple concurrent queries to the segment data base can cause time out errors. If that happens, this will sleep for a few seconds, then try again a few times before giving up.
pycbc.inference.models.gated_gaussian_noise module¶
This module provides model classes that assume the noise is Gaussian and introduces a gate to remove given times from the data, using the inpainting method to fill the removed part such that it does not enter the likelihood.
- class pycbc.inference.models.gated_gaussian_noise.BaseGatedGaussian(variable_params, data, low_frequency_cutoff, psds=None, high_frequency_cutoff=None, normalize=False, static_params=None, highpass_waveforms=False, **kwargs)[source]¶
Bases:
BaseGaussianNoise
Base model for gated gaussian.
Provides additional routines for applying a time-domain gate to data. See
GatedGaussianNoise
for more details.- det_lognl(det)[source]¶
Returns the log likelihood of the noise in the given detector:
\[\log p(d_i|n_i) = \log \alpha_i - \frac{1}{2} \left<d_i | d_i\right>.\]
- det_lognorm(det)[source]¶
The log of the likelihood normalization in the given detector.
If
self.normalize
is False, will just return 0.
- classmethod from_config(cp, data_section='data', data=None, psds=None, **kwargs)[source]¶
Adds highpass filtering to keyword arguments based on config file.
- get_data()[source]¶
Return a copy of the data.
- Returns:
Dictionary of detector names -> FrequencySeries.
- Return type:
- get_gate_times()[source]¶
Gets the time to apply a gate based on the current sky position.
If the parameter
gatefunc
is set to'hmeco'
, the gate times will be calculated based on the hybrid MECO of the given set of parameters; seeget_gate_times_hmeco
for details. Otherwise, the gate times will just be retrieved from thet_gate_start
andt_gate_end
parameters.Warning
Since the normalization of the likelihood is currently not being calculated, it is recommended that you do not use
gatefunc
, instead using fixed gate times.- Returns:
Dictionary of detector names -> (gate start, gate width)
- Return type:
- get_gate_times_hmeco()[source]¶
Gets the time to apply a gate based on the current sky position. :returns: Dictionary of detector names -> (gate start, gate width) :rtype: dict
- get_gated_data()[source]¶
Return a copy of the gated data.
The gated data will be cached for faster retrieval.
- Returns:
Dictionary of detector names -> FrequencySeries.
- Return type:
- abstract get_gated_waveforms()[source]¶
Generates and gates waveforms using the current parameters.
- Returns:
Dictionary of detector names -> FrequencySeries.
- Return type:
- get_residuals()[source]¶
Generates the residuals
d-h
using the current parameters.- Returns:
Dictionary of detector names -> FrequencySeries.
- Return type:
- get_waveforms()[source]¶
The waveforms generated using the current parameters.
If the waveforms haven’t been generated yet, they will be generated, resized to the same length as the data, and cached. If the
highpass_waveforms
attribute is set, a highpass filter will also be applied to the waveforms.- Returns:
Dictionary of detector names -> FrequencySeries.
- Return type:
- property normalize¶
Determines if the loglikelihood includes the normalization term.
- property psds¶
Dictionary of detectors -> PSD frequency series.
If no PSD was provided for a detector, this will just be a frequency series of ones.
- property td_data¶
The data in the time domain.
- whiten(data, whiten, inplace=False)[source]¶
Whitens the given data.
- Parameters:
data (dict) – Dictionary of detector names -> FrequencySeries.
whiten ({0, 1, 2}) – Integer indicating what level of whitening to apply. Levels are: 0: no whitening; 1: whiten; 2: overwhiten.
inplace (bool, optional) – If True, modify the data in place. Otherwise, a copy will be created for whitening.
- Returns:
Dictionary of FrequencySeries after the requested whitening has been applied.
- Return type:
- write_metadata(fp, group=None)[source]¶
Adds writing the psds, and analyzed detectors.
The analyzed detectors, their analysis segments, and the segments used for psd estimation are written as
analyzed_detectors
,{{detector}}_analysis_segment
, and{{detector}}_psd_segment
, respectively. These are either written to the specifiedgroup
’s attrs, or to the top level attrs ifgroup
is None.- Parameters:
fp (pycbc.inference.io.BaseInferenceFile instance) – The inference file to write to.
group (str, optional) – If provided, the metadata will be written to the attrs specified by group, i.e., to
fp[group].attrs
. Otherwise, metadata is written to the top-level attrs (fp.attrs
).
- class pycbc.inference.models.gated_gaussian_noise.GatedGaussianMargPol(variable_params, data, low_frequency_cutoff, psds=None, high_frequency_cutoff=None, normalize=False, static_params=None, polarization_samples=1000, **kwargs)[source]¶
Bases:
BaseGatedGaussian
Gated gaussian model with numerical marginalization over polarization.
This implements the GatedGaussian likelihood with an explicit numerical marginalization over polarization angle. This is accomplished using a fixed set of integration points distribution uniformation between 0 and 2pi. By default, 1000 integration points are used. The ‘polarization_samples’ argument can be passed to set an alternate number of integration points.
- get_gated_waveforms()[source]¶
Generates and gates waveforms using the current parameters.
- Returns:
Dictionary of detector names -> FrequencySeries.
- Return type:
- get_waveforms()[source]¶
The waveforms generated using the current parameters.
If the waveforms haven’t been generated yet, they will be generated, resized to the same length as the data, and cached. If the
highpass_waveforms
attribute is set, a highpass filter will also be applied to the waveforms.- Returns:
Dictionary of detector names -> FrequencySeries.
- Return type:
- name = 'gated_gaussian_margpol'¶
- class pycbc.inference.models.gated_gaussian_noise.GatedGaussianNoise(variable_params, data, low_frequency_cutoff, psds=None, high_frequency_cutoff=None, normalize=False, static_params=None, **kwargs)[source]¶
Bases:
BaseGatedGaussian
Model that applies a time domain gate, assuming stationary Gaussian noise.
The gate start and end times are set by providing
t_gate_start
andt_gate_end
parameters, respectively. This will cause the gated times to be excised from the analysis. For more details on the likelihood function and its derivation, see arXiv:2105.05238.Warning
The normalization of the likelihood depends on the gate times. However, at the moment, the normalization is not calculated, as it depends on the determinant of the truncated covariance matrix (see Eq. 4 of arXiv:2105.05238). For this reason it is recommended that you only use this model for fixed gate times.
- get_gated_residuals()[source]¶
Generates the gated residuals
d-h
using the current parameters.- Returns:
Dictionary of detector names -> FrequencySeries.
- Return type:
- get_gated_waveforms()[source]¶
Generates and gates waveforms using the current parameters.
- Returns:
Dictionary of detector names -> FrequencySeries.
- Return type:
- name = 'gated_gaussian_noise'¶
pycbc.inference.models.gaussian_noise module¶
This module provides model classes that assume the noise is Gaussian.
- class pycbc.inference.models.gaussian_noise.BaseGaussianNoise(variable_params, data, low_frequency_cutoff, psds=None, high_frequency_cutoff=None, normalize=False, static_params=None, ignore_failed_waveforms=False, no_save_data=False, **kwargs)[source]¶
Bases:
BaseDataModel
Model for analyzing GW data with assuming a wide-sense stationary Gaussian noise model.
This model will load gravitational wave data and calculate the log noise likelihood
_lognl
and normalization. It also implements the_loglikelihood
function as the sum of the log likelihood ratio and thelognl
. It does not implement a log likelihood ratio function_loglr
, however, since that can differ depending on the signal model. Models that analyze GW data assuming it is stationary Gaussian should therefore inherit from this class and implement their own_loglr
function.For more details on the inner product used, the log likelihood of the noise, and the normalization factor, see
GaussianNoise
.- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied.
data (dict) – A dictionary of data, in which the keys are the detector names and the values are the data (assumed to be unwhitened). All data must have the same frequency resolution.
low_frequency_cutoff (dict) – A dictionary of starting frequencies, in which the keys are the detector names and the values are the starting frequencies for the respective detectors to be used for computing inner products.
psds (dict, optional) – A dictionary of FrequencySeries keyed by the detector names. The dictionary must have a psd for each detector specified in the data dictionary. If provided, the inner products in each detector will be weighted by 1/psd of that detector.
high_frequency_cutoff (dict, optional) – A dictionary of ending frequencies, in which the keys are the detector names and the values are the ending frequencies for the respective detectors to be used for computing inner products. If not provided, the minimum of the largest frequency stored in the data and a given waveform will be used.
normalize (bool, optional) – If True, the normalization factor \(alpha\) will be included in the log likelihood. See
GaussianNoise
for details. Default is to not include it.static_params (dict, optional) – A dictionary of parameter names -> values to keep fixed.
ignore_failed_waveforms (bool, optional) – If the waveform generator raises an error when it tries to generate, treat the point as having zero likelihood. This allows the parameter estimation to continue. Otherwise, an error will be raised, stopping the run. Default is False.
**kwargs – All other keyword arguments are passed to
BaseDataModel
.
- ignore_failed_waveforms¶
If True, points in parameter space that cause waveform generation to fail (i.e., they raise a
FailedWaveformError
) will be treated as points with zero likelihood. Otherwise, such points will cause the model to raise aFailedWaveformError
.- Type:
- det_lognl(det)[source]¶
Returns the log likelihood of the noise in the given detector:
\[\log p(d_i|n_i) = \log \alpha_i - \frac{1}{2} \left<d_i | d_i\right>.\]
- det_lognorm(det)[source]¶
The log of the likelihood normalization in the given detector.
If
self.normalize
is False, will just return 0.
- classmethod from_config(cp, data_section='data', data=None, psds=None, **kwargs)[source]¶
Initializes an instance of this class from the given config file.
In addition to
[model]
, adata_section
(default[data]
) must be in the configuration file. The data section specifies settings for loading data and estimating PSDs. See the online documentation for more details.The following options are read from the
[model]
section, in addition toname
(which must be set):{{DET}}-low-frequency-cutoff = FLOAT
: The low frequency cutoff to use for each detector {{DET}}. A cutoff must be provided for every detector that may be analyzed (any additional detectors are ignored).{{DET}}-high-frequency-cutoff = FLOAT
: (Optional) A high frequency cutoff for each detector. If not provided, the Nyquist frequency is used.check-for-valid-times =
: (Optional) If provided, will check that there are no data quality flags on during the analysis segment and the segment used for PSD estimation in each detector. To check for flags,pycbc.dq.query_flag()
is used, with settings pulled from thedq-*
options in the[data]
section. If a detector has bad data quality during either the analysis segment or PSD segment, it will be removed from the analysis.shift-psd-times-to-valid =
: (Optional) If provided, the segment used for PSD estimation will automatically be shifted left or right until a continous block of data with no data quality issues can be found. If no block can be found with a maximum shift of +/- the requested psd segment length, the detector will not be analyzed.err-on-missing-detectors =
: Raises an error if any detector is removed from the analysis because a valid time could not be found. Otherwise, a warning is printed to screen and the detector is removed from the analysis.normalize =
: (Optional) Turn on the normalization factor.ignore-failed-waveforms =
: Sets theignore_failed_waveforms
attribute.
- Parameters:
cp (WorkflowConfigParser) – Config file parser to read.
data_section (str, optional) – The name of the section to load data options from.
**kwargs – All additional keyword arguments are passed to the class. Any provided keyword will override what is in the config file.
- property high_frequency_cutoff¶
The high frequency cutoff of the inner product.
- property kmax¶
Dictionary of ending indices for the inner product.
This is determined from the high frequency cutoff and the
delta_f
of the data usingpycbc.filter.matchedfilter.get_cutoff_indices()
. If no high frequency cutoff was provided, this will be the indice corresponding to the Nyquist frequency.
- property kmin¶
Dictionary of starting indices for the inner product.
This is determined from the lower frequency cutoff and the
delta_f
of the data usingpycbc.filter.matchedfilter.get_cutoff_indices()
.
- property lognorm¶
The log of the normalization of the log likelihood.
- property low_frequency_cutoff¶
The low frequency cutoff of the inner product.
- property normalize¶
Determines if the loglikelihood includes the normalization term.
- property psd_segments¶
Dictionary giving times used for PSD estimation for each detector.
If a detector’s PSD was not estimated from data, or the segment wasn’t provided, that detector will not be in the dictionary.
- property psds¶
Dictionary of detectors -> PSD frequency series.
If no PSD was provided for a detector, this will just be a frequency series of ones.
- set_psd_segments(psds)[source]¶
Sets the PSD segments from a dictionary of PSDs.
This attempts to get the PSD segment from a
psd_segment
attribute of each detector’s PSD frequency series. If that attribute isn’t set, then that detector is not added to the dictionary of PSD segments.- Parameters:
psds (dict) – Dictionary of detector name -> PSD frequency series. The segment used for each PSD will try to be retrieved from the PSD’s
.psd_segment
attribute.
- update(**params)[source]¶
Updates the current parameter positions and resets stats.
If any sampling transforms are specified, they are applied to the params before being stored.
- property weight¶
Dictionary of detectors -> frequency series of inner-product weights.
The weights are \(\sqrt{4 \Delta f / S_n(f)}\). This is set when the PSDs are set.
- property whitened_data¶
Dictionary of detectors -> whitened data frequency series.
The whitened data is the data multiplied by the inner-product weight. Note that this includes the \(\sqrt{4 \Delta f}\) factor. This is set when the PSDs are set.
- write_metadata(fp, group=None)[source]¶
Adds writing the psds, analyzed detectors, and lognl.
The analyzed detectors, their analysis segments, and the segments used for psd estimation are written as
analyzed_detectors
,{{detector}}_analysis_segment
, and{{detector}}_psd_segment
, respectively. These are either written to the specifiedgroup
’s attrs, or to the top level attrs ifgroup
is None.The total and each detector’s lognl is written to the sample group’s
attrs
. If a group is specified, the group name will be prependend to the lognl labels with{group}__
, with any/
in the group path replaced with__
. For example, if group is/a/b
, thelognl
will be written asa__b__lognl
in the sample’s group attrs.- Parameters:
fp (pycbc.inference.io.BaseInferenceFile instance) – The inference file to write to.
group (str, optional) – If provided, the metadata will be written to the attrs specified by group, i.e., to
fp[group].attrs
. Otherwise, metadata is written to the top-level attrs (fp.attrs
).
- class pycbc.inference.models.gaussian_noise.GaussianNoise(variable_params, data, low_frequency_cutoff, psds=None, high_frequency_cutoff=None, normalize=False, static_params=None, det_frame_waveform=False, **kwargs)[source]¶
Bases:
BaseGaussianNoise
Model that assumes data is stationary Gaussian noise.
With Gaussian noise the log likelihood functions for signal \(\log p(d|\Theta, h)\) and for noise \(\log p(d|n)\) are given by:
\[\begin{split}\log p(d|\Theta, h) &= \log\alpha -\frac{1}{2} \sum_i \left< d_i - h_i(\Theta) | d_i - h_i(\Theta) \right> \\ \log p(d|n) &= \log\alpha -\frac{1}{2} \sum_i \left<d_i | d_i\right>\end{split}\]where the sum is over the number of detectors, \(d_i\) is the data in each detector, and \(h_i(\Theta)\) is the model signal in each detector. The (discrete) inner product is given by:
\[\left<a_i | b_i\right> = 4\Re \Delta f \sum_{k=k_{\mathrm{min}}}^{k_{\mathrm{max}}} \frac{\tilde{a}_i^{*}[k] \tilde{b}_i[k]}{S^{(i)}_n[k]},\]where \(\Delta f\) is the frequency resolution (given by 1 / the observation time \(T\)), \(k\) is an index over the discretely sampled frequencies \(f = k \Delta_f\), and \(S^{(i)}_n[k]\) is the PSD in the given detector. The upper cutoff on the inner product \(k_{\max}\) is by default the Nyquist frequency \(k_{\max} = N/2+1\), where \(N = \lfloor T/\Delta t \rfloor\) is the number of samples in the time domain, but this can be set manually to a smaller value.
The normalization factor \(\alpha\) is:
\[\alpha = \prod_{i} \frac{1}{\left(\pi T\right)^{N/2} \prod_{k=k_\mathrm{min}}^{k_{\mathrm{max}}} S^{(i)}_n[k]},\]where the product is over the number of detectors. By default, the normalization constant is not included in the log likelihood, but it can be turned on using the
normalize
keyword argument.Note that the log likelihood ratio has fewer terms than the log likelihood, since the normalization and \(\left<d_i|d_i\right>\) terms cancel:
\[\log \mathcal{L}(\Theta) = \sum_i \left[ \left<h_i(\Theta)|d_i\right> - \frac{1}{2} \left<h_i(\Theta)|h_i(\Theta)\right> \right]\]Upon initialization, the data is whitened using the given PSDs. If no PSDs are given the data and waveforms returned by the waveform generator are assumed to be whitened.
For more details on initialization parameters and definition of terms, see
models.BaseDataModel
.- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied.
data (dict) – A dictionary of data, in which the keys are the detector names and the values are the data (assumed to be unwhitened). The list of keys must match the waveform generator’s detectors keys, and the epoch of every data set must be the same as the waveform generator’s epoch.
low_frequency_cutoff (dict) – A dictionary of starting frequencies, in which the keys are the detector names and the values are the starting frequencies for the respective detectors to be used for computing inner products.
psds (dict, optional) – A dictionary of FrequencySeries keyed by the detector names. The dictionary must have a psd for each detector specified in the data dictionary. If provided, the inner products in each detector will be weighted by 1/psd of that detector.
high_frequency_cutoff (dict, optional) – A dictionary of ending frequencies, in which the keys are the detector names and the values are the ending frequencies for the respective detectors to be used for computing inner products. If not provided, the minimum of the largest frequency stored in the data and a given waveform will be used.
normalize (bool, optional) – If True, the normalization factor \(alpha\) will be included in the log likelihood. Default is to not include it.
static_params (dict, optional) – A dictionary of parameter names -> values to keep fixed.
det_frame_waveform (bool) – If True, the waveform will be generated directly in the detector frame using the
FDomainDirectDetFrameGenerator
. This requires the approximant be implemented inget_fd_det_waveform()
. If False, theFDomainDetFrameGenerator
will be used instead. Defaults toFalse
.**kwargs – All other keyword arguments are passed to
BaseDataModel
.
Examples
Create a signal, and set up the model using that signal:
>>> from pycbc import psd as pypsd >>> from pycbc.inference.models import GaussianNoise >>> from pycbc.waveform.generator import (FDomainDetFrameGenerator, ... FDomainCBCGenerator) >>> seglen = 4 >>> sample_rate = 2048 >>> N = seglen*sample_rate/2+1 >>> fmin = 30. >>> static_params = {'approximant': 'IMRPhenomD', 'f_lower': fmin, ... 'mass1': 38.6, 'mass2': 29.3, ... 'spin1z': 0., 'spin2z': 0., 'ra': 1.37, 'dec': -1.26, ... 'polarization': 2.76, 'distance': 3*500.} >>> variable_params = ['tc'] >>> tsig = 3.1 >>> generator = FDomainDetFrameGenerator( ... FDomainCBCGenerator, 0., detectors=['H1', 'L1'], ... variable_args=variable_params, ... delta_f=1./seglen, **static_params) >>> signal = generator.generate(tc=tsig) >>> psd = pypsd.aLIGOZeroDetHighPower(N, 1./seglen, 20.) >>> psds = {'H1': psd, 'L1': psd} >>> low_frequency_cutoff = {'H1': fmin, 'L1': fmin} >>> model = GaussianNoise(variable_params, signal, low_frequency_cutoff, psds=psds, static_params=static_params)
Set the current position to the coalescence time of the signal:
>>> model.update(tc=tsig)
Now compute the log likelihood ratio and prior-weighted likelihood ratio; since we have not provided a prior, these should be equal to each other:
>>> print('{:.2f}'.format(model.loglr)) 282.43 >>> print('{:.2f}'.format(model.logplr)) 282.43
Print all of the default_stats:
>>> print(',\n'.join(['{}: {:.2f}'.format(s, v) ... for (s, v) in sorted(model.current_stats.items())])) H1_cplx_loglr: 177.76+0.00j, H1_optimal_snrsq: 355.52, L1_cplx_loglr: 104.67+0.00j, L1_optimal_snrsq: 209.35, logjacobian: 0.00, loglikelihood: 0.00, loglr: 282.43, logprior: 0.00
Compute the SNR; for this system and PSD, this should be approximately 24:
>>> from pycbc.conversions import snr_from_loglr >>> x = snr_from_loglr(model.loglr) >>> print('{:.2f}'.format(x)) 23.77
Since there is no noise, the SNR should be the same as the quadrature sum of the optimal SNRs in each detector:
>>> x = (model.det_optimal_snrsq('H1') + ... model.det_optimal_snrsq('L1'))**0.5 >>> print('{:.2f}'.format(x)) 23.77
Toggle on the normalization constant:
>>> model.normalize = True >>> model.loglikelihood 835397.8757405131
Using the same model, evaluate the log likelihood ratio at several points in time and check that the max is at tsig:
>>> import numpy >>> times = numpy.linspace(tsig-1, tsig+1, num=101) >>> loglrs = numpy.zeros(len(times)) >>> for (ii, t) in enumerate(times): ... model.update(tc=t) ... loglrs[ii] = model.loglr >>> print('tsig: {:.2f}, time of max loglr: {:.2f}'.format( ... tsig, times[loglrs.argmax()])) tsig: 3.10, time of max loglr: 3.10
Create a prior and use it (see distributions module for more details):
>>> from pycbc import distributions >>> uniform_prior = distributions.Uniform(tc=(tsig-0.2,tsig+0.2)) >>> prior = distributions.JointDistribution(variable_params, uniform_prior) >>> model = GaussianNoise(variable_params, ... signal, low_frequency_cutoff, psds=psds, prior=prior, ... static_params=static_params) >>> model.update(tc=tsig) >>> print('{:.2f}'.format(model.logplr)) 283.35 >>> print(',\n'.join(['{}: {:.2f}'.format(s, v) ... for (s, v) in sorted(model.current_stats.items())])) H1_cplx_loglr: 177.76+0.00j, H1_optimal_snrsq: 355.52, L1_cplx_loglr: 104.67+0.00j, L1_optimal_snrsq: 209.35, logjacobian: 0.00, loglikelihood: 0.00, loglr: 282.43, logprior: 0.92
- det_cplx_loglr(det)[source]¶
Returns the complex log likelihood ratio in the given detector.
- Parameters:
det (str) – The name of the detector.
- Returns:
The complex log likelihood ratio.
- Return type:
complex float
- get_waveforms()[source]¶
The waveforms generated using the current parameters.
If the waveforms haven’t been generated yet, they will be generated.
- Returns:
Dictionary of detector names -> FrequencySeries.
- Return type:
- property multi_signal_support¶
The list of classes that this model supports in a multi-signal likelihood
- name = 'gaussian_noise'¶
- pycbc.inference.models.gaussian_noise.create_waveform_generator(variable_params, data, waveform_transforms=None, recalibration=None, gates=None, generator_class=<class 'pycbc.waveform.generator.FDomainDetFrameGenerator'>, **static_params)[source]¶
Creates a waveform generator for use with a model.
- Parameters:
variable_params (list of str) – The names of the parameters varied.
data (dict) – Dictionary mapping detector names to either a
<pycbc.types.TimeSeries TimeSeries>
or<pycbc.types.FrequencySeries FrequencySeries>
.waveform_transforms (list, optional) – The list of transforms applied to convert variable parameters into parameters that will be understood by the waveform generator.
recalibration (dict, optional) – Dictionary mapping detector names to
<pycbc.calibration.Recalibrate>
instances for recalibrating data.gates (dict of tuples, optional) – Dictionary of detectors -> tuples of specifying gate times. The sort of thing returned by
pycbc.gate.gates_from_cli()
.generator_class (detector-frame fdomain generator, optional) – Class to use for generating waveforms. Default is
waveform.generator.FDomainDetFrameGenerator
.**static_params – All other keyword arguments are passed as static parameters to the waveform generator.
- Returns:
A waveform generator for frequency domain generation.
- Return type:
pycbc.waveform.FDomainDetFrameGenerator
- pycbc.inference.models.gaussian_noise.get_values_from_injection(cp, injection_file, update_cp=True)[source]¶
Replaces all FROM_INJECTION values in a config file with the corresponding value from the injection.
This looks for any options that start with
FROM_INJECTION[:ARG]
in a config file. It then replaces that value with the corresponding value from the injection file. An argument may be optionally provided, in which case the argument will be retrieved from the injection file. Functions of parameters in the injection file may be used; the syntax and functions available is the same as the--parameters
argument in executables such aspycbc_inference_extract_samples
. If noARG
is provided, then the option name will try to be retrieved from the injection.For example,
mass1 = FROM_INJECTION
will cause
mass1
to be retrieved from the injection file, while:mass1 = FROM_INJECTION:'primary_mass(mass1, mass2)'
will cause the larger of mass1 and mass2 to be retrieved from the injection file. Note that if spaces are in the argument, it must be encased in single quotes.
The injection file may contain only one injection. Otherwise, a ValueError will be raised.
- Parameters:
cp (ConfigParser) – The config file within which to replace values.
injection_file (str or None) – The injection file to get values from. A ValueError will be raised if there are any
FROM_INJECTION
values in the config file, and injection file is None, or if there is more than one injection.update_cp (bool, optional) – Update the config parser with the replaced parameters. If False, will just retrieve the parameter values to update, without updating the config file. Default is True.
- Returns:
The parameters that were replaced, as a tuple of section name, option, value.
- Return type:
pycbc.inference.models.hierarchical module¶
Hierarchical model definitions.
- class pycbc.inference.models.hierarchical.HierarchicalModel(variable_params, submodels, **kwargs)[source]¶
Bases:
BaseModel
Model that is a combination of other models.
Sub-models are treated as being independent of each other, although they can share parameters. In other words, the hierarchical likelihood is:
\[p(\mathbf{D}|\mathbf{\vartheta}, \mathbf{H}) = \prod_{I}^{K} p(\mathbf{d}_I|\mathbf{\vartheta}, H_{I})\]Submodels are provided as a dictionary upon initialization with a unique label assigned to each model, e.g.,
{'event1' -> model1, 'event2' -> model2}
. Variable and static parameters that are specific to each submodel should be prepended with{label}__
, where{label}__
is the label associated with the given submodel. Shared parameters across multiple models have no labels prepended. To specify shared models over a subset of models, separate models with an underscore. For example,event1_event2__foo
will result infoo
being common between modelsevent1
andevent2
. For more details on parameter naming seeHierarchicalParam
.All waveform and sampling transforms, as well as prior evaluation, are handled by this model, not the sub-models. Parameters created by waveform transforms should therefore also have sub-model names prepended to them, to indicate which models they should be provided to for likelihood evaluation.
- Parameters:
- classmethod from_config(cp, **kwargs)[source]¶
Initializes an instance of this class from the given config file.
Sub-models are initialized before initializing this class. The model section must have a
submodels
argument that lists the names of all the submodels to generate as a space-separated list. Each sub-model should have its own[{label}__model]
section that sets up the model for that sub-model. For example:[model] name = hierarchical submodels = event1 event2 [event1__model] <event1 model options> [event2__model] <event2 model options>
Similarly, all other sections that are specific to a model should start with the model’s label. All sections starting with a model’s label will be passed to that model’s
from_config
method with the label removed from the section name. For example, if a sub-model requires a data section to be specified, it should be titled[{label}__data]
. Upon initialization, the{label}__
will be stripped from the section header and passed to the model.No model labels should preceed the
variable_params
,static_params
,waveform_transforms
, orsampling_transforms
sections. Instead, the parameters specified in these sections should follow the naming conventions described inHierachicalParam
to determine which sub-model(s) they belong to. (Sampling parameters can follow any naming convention, as they are only handled by the hierarchical model.) This is because the hierarchical model handles all transforms, communication with the sampler, file IO, and prior calculation. Only sub-model’s loglikelihood functions are called.Metadata for each sub-model is written to the output hdf file under groups given by the sub-model label. For example, if we have two submodels labelled
event1
andevent2
, there will be groups with the same names in the top level of the output that contain that model’s subdata. For instance, if event1 used thegaussian_noise
model, the GW data and PSDs will be found inevent1/data
and the low frequency cutoff used for that model will be in theattrs
of theevent1
group.- Parameters:
cp (WorkflowConfigParser) – Config file parser to read.
**kwargs – All additional keyword arguments are passed to the class. Any provided keyword will override what is in the config file.
- property hstatic_params¶
The static params with
HierarchicalParam
instances used as dictionary keys.
- property hvariable_params¶
The variable params as a tuple of
HierarchicalParam
instances.
- name = 'hierarchical'¶
- property static_params¶
Returns the model’s static arguments.
- property variable_params¶
Returns the model parameters.
- write_metadata(fp, group=None)[source]¶
Adds data to the metadata that’s written.
- Parameters:
fp (pycbc.inference.io.BaseInferenceFile instance) – The inference file to write to.
group (str, optional) – If provided, the metadata will be written to the attrs specified by group, i.e., to
fp[group].attrs
. Otherwise, metadata is written to the top-level attrs (fp.attrs
).
- class pycbc.inference.models.hierarchical.HierarchicalParam(fullname, possible_models)[source]¶
Bases:
str
Sub-class of str for hierarchical parameter names.
This adds attributes that keep track of the model label(s) the parameter is associated with, along with the name that is passed to the models.
The following conventions are used for parsing parameter names:
Model labels and parameter names are separated by the
delim
class attribute, which by default is__
, e.g.,event1__mass
.Multiple model labels can be provided by separating the model labels with the
model_delim
class attribute, which by default is_
, e.g.,event1_event2__mass
. Note that this means that individual model labels cannot contain_
, else they’ll be parsed as separate models.Parameters that have no model labels prepended to them (i.e., there is no
__
in the name) are common to all models.
These parsing rules are applied by the
HierarchicalParam.parse()
method.- Parameters:
- fullname¶
The full name of the parameter, including model labels. For example,
e1_e2__foo
.- Type:
- models¶
The model labels the parameter is associated with. For example,
e1_e2__foo
yields modelse1, e2
.- Type:
- subname¶
The name of the parameter without the model labels prepended to it. For example,
e1_e2__foo
yieldsfoo
.- Type:
- delim = '__'¶
- classmethod from_subname(model_label, subname)[source]¶
Creates a HierarchicalParam from the given subname and model label.
- model_delim = '_'¶
- classmethod parse(fullname, possible_models)[source]¶
Parses the full parameter name into the models the parameter is associated with and the parameter name that is passed to the models.
- Parameters:
- Returns:
models (list) – List of the model labels the parameter is associated with.
subp (str) – Parameter name that is passed to the models. This is the parameter name with the model label(s) stripped from it.
- class pycbc.inference.models.hierarchical.JointPrimaryMarginalizedModel(variable_params, submodels, **kwargs)[source]¶
Bases:
HierarchicalModel
Hierarchical heterodyne likelihood for coherent multiband parameter estimation which combines data from space-borne and ground-based GW detectors coherently. Currently, this only supports LISA as the space-borne GW detector.
Sub models are treated as if the same GW source (such as a GW from stellar-mass BBH) is observed in different frequency bands by space-borne and ground-based GW detectors, then transform all the parameters into the same frame in the sub model level, use HierarchicalModel to get the joint likelihood, and marginalize over all the extrinsic parameters supported by RelativeTimeDom or its variants. Note that LISA submodel only supports the Relative for now, for ground-based detectors, please use RelativeTimeDom or its variants.
Although this likelihood model is used for multiband parameter estimation, users can still use it for other purposes, such as GW + EM parameter estimation, in this case, please use RelativeTimeDom or its variants for the GW data, for the likelihood of EM data, there is no restrictions.
- classmethod from_config(cp, **kwargs)[source]¶
Initializes an instance of this class from the given config file. For more details, see from_config in HierarchicalModel.
- Parameters:
cp (WorkflowConfigParser) – Config file parser to read.
**kwargs – All additional keyword arguments are passed to the class. Any provided keyword will override what is in the config file.
- name = 'joint_primary_marginalized'¶
- reconstruct(rec=None, seed=None)[source]¶
Reconstruct marginalized parameters by using the primary model’s reconstruct method, total_loglr, and others_lognl.
- total_loglr()[source]¶
Computes the total log likelihood ratio,
\[\log \mathcal{L}(\Theta) = \sum_i \left<h_i(\Theta)|d_i\right> - \frac{1}{2}\left<h_i(\Theta)|h_i(\Theta)\right>,\]at the current parameter values \(\Theta\).
- Returns:
The value of the log likelihood ratio.
- Return type:
- update_all_models(**params)[source]¶
This update method is also useful for loglr checking, the original update method in base module can’t update parameters in submodels correctly in loglr checking.
- write_metadata(fp, group=None)[source]¶
Adds metadata to the output files
- Parameters:
fp (pycbc.inference.io.BaseInferenceFile instance) – The inference file to write to.
group (str, optional) – If provided, the metadata will be written to the attrs specified by group, i.e., to
fp[group].attrs
. Otherwise, metadata is written to the top-level attrs (fp.attrs
).
- class pycbc.inference.models.hierarchical.MultiSignalModel(variable_params, submodels, **kwargs)[source]¶
Bases:
HierarchicalModel
Model for multiple signals which share data
Sub models are treated as if the signals overlap in data. This requires constituent models to implement a specific method to handle this case. All models must be of the same type or the specific model is responsible for implement cross-compatibility with another model. Each model h_i is responsible for calculating its own loglikelihood ratio for itself, and must also implement a method to calculate crossterms of the form <h_i | h_j> which arise from the full calculation of <d - h|d - h>. This model inherits from the HierarchicalModel so the syntax for configuration files is the same. The primary model is used to determine the noise terms <d | d>, which by default will be the first model used.
- name = 'multi_signal'¶
- write_metadata(fp, group=None)[source]¶
Adds metadata to the output files
- Parameters:
fp (pycbc.inference.io.BaseInferenceFile instance) – The inference file to write to.
group (str, optional) – If provided, the metadata will be written to the attrs specified by group, i.e., to
fp[group].attrs
. Otherwise, metadata is written to the top-level attrs (fp.attrs
).
- pycbc.inference.models.hierarchical.hpiter(params, possible_models)[source]¶
Turns a list of parameter strings into a list of HierarchicalParams.
- Parameters:
- Returns:
Iterator of
HierarchicalParam
instances.- Return type:
iterator
pycbc.inference.models.marginalized_gaussian_noise module¶
This module provides model classes that assume the noise is Gaussian and allows for the likelihood to be marginalized over phase and/or time and/or distance.
- class pycbc.inference.models.marginalized_gaussian_noise.MarginalizedHMPolPhase(variable_params, data, low_frequency_cutoff, psds=None, high_frequency_cutoff=None, normalize=False, polarization_samples=100, coa_phase_samples=100, static_params=None, **kwargs)[source]¶
Bases:
BaseGaussianNoise
Numerically marginalizes waveforms with higher modes over polarization and phase.
This class implements the Gaussian likelihood with an explicit numerical marginalization over polarization angle and orbital phase. This is accomplished using a fixed set of integration points distributed uniformly between 0 and 2:math:pi for both the polarization and phase. By default, 100 integration points are used for each parameter, giving \(10^4\) evaluation points in total. This can be modified using the
polarization_samples
andcoa_phase_samples
arguments.This only works with waveforms that return separate spherical harmonic modes for each waveform. For a list of currently supported approximants, see
pycbc.waveform.waveform_modes.fd_waveform_mode_approximants()
andpycbc.waveform.waveform_modes.td_waveform_mode_approximants()
.- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied.
data (dict) – A dictionary of data, in which the keys are the detector names and the values are the data (assumed to be unwhitened). All data must have the same frequency resolution.
low_frequency_cutoff (dict) – A dictionary of starting frequencies, in which the keys are the detector names and the values are the starting frequencies for the respective detectors to be used for computing inner products.
psds (dict, optional) – A dictionary of FrequencySeries keyed by the detector names. The dictionary must have a psd for each detector specified in the data dictionary. If provided, the inner products in each detector will be weighted by 1/psd of that detector.
high_frequency_cutoff (dict, optional) – A dictionary of ending frequencies, in which the keys are the detector names and the values are the ending frequencies for the respective detectors to be used for computing inner products. If not provided, the minimum of the largest frequency stored in the data and a given waveform will be used.
normalize (bool, optional) – If True, the normalization factor \(alpha\) will be included in the log likelihood. See
GaussianNoise
for details. Default is to not include it.polarization_samples (int, optional) – How many points to use in polarization. Default is 100.
coa_phase_samples (int, optional) – How many points to use in phase. Defaults is 100.
**kwargs – All other keyword arguments are passed to
BaseGaussianNoise
.
- name = 'marginalized_hmpolphase'¶
- class pycbc.inference.models.marginalized_gaussian_noise.MarginalizedPhaseGaussianNoise(variable_params, data, low_frequency_cutoff, psds=None, high_frequency_cutoff=None, normalize=False, static_params=None, **kwargs)[source]¶
Bases:
GaussianNoise
The likelihood is analytically marginalized over phase.
This class can be used with signal models that can be written as:
\[\tilde{h}(f; \Theta, \phi) = A(f; \Theta)e^{i\Psi(f; \Theta) + i \phi},\]where \(\phi\) is an arbitrary phase constant. This phase constant can be analytically marginalized over with a uniform prior as follows: assuming the noise is stationary and Gaussian (see GaussianNoise for details), the posterior is:
\[\begin{split}p(\Theta,\phi|d) &\propto p(\Theta)p(\phi)p(d|\Theta,\phi) \\ &\propto p(\Theta)\frac{1}{2\pi}\exp\left[ -\frac{1}{2}\sum_{i}^{N_D} \left< h_i(\Theta,\phi) - d_i, h_i(\Theta,\phi) - d_i \right>\right].\end{split}\]Here, the sum is over the number of detectors \(N_D\), \(d_i\) and \(h_i\) are the data and signal in detector \(i\), respectively, and we have assumed a uniform prior on \(\phi \in [0, 2\pi)\). With the form of the signal model given above, the inner product in the exponent can be written as:
\[\begin{split}-\frac{1}{2}\left<h_i - d_i, h_i- d_i\right> &= \left<h_i, d_i\right> - \frac{1}{2}\left<h_i, h_i\right> - \frac{1}{2}\left<d_i, d_i\right> \\ &= \Re\left\{O(h^0_i, d_i)e^{-i\phi}\right\} - \frac{1}{2}\left<h^0_i, h^0_i\right> - \frac{1}{2}\left<d_i, d_i\right>,\end{split}\]where:
\[\begin{split}h_i^0 &\equiv \tilde{h}_i(f; \Theta, \phi=0); \\ O(h^0_i, d_i) &\equiv 4 \int_0^\infty \frac{\tilde{h}_i^*(f; \Theta,0)\tilde{d}_i(f)}{S_n(f)}\mathrm{d}f.\end{split}\]Gathering all of the terms that are not dependent on \(\phi\) together:
\[\alpha(\Theta, d) \equiv \exp\left[-\frac{1}{2}\sum_i \left<h^0_i, h^0_i\right> + \left<d_i, d_i\right>\right],\]we can marginalize the posterior over \(\phi\):
\[\begin{split}p(\Theta|d) &\propto p(\Theta)\alpha(\Theta,d)\frac{1}{2\pi} \int_{0}^{2\pi}\exp\left[\Re \left\{ e^{-i\phi} \sum_i O(h^0_i, d_i) \right\}\right]\mathrm{d}\phi \\ &\propto p(\Theta)\alpha(\Theta, d)\frac{1}{2\pi} \int_{0}^{2\pi}\exp\left[ x(\Theta,d)\cos(\phi) + y(\Theta, d)\sin(\phi) \right]\mathrm{d}\phi.\end{split}\]The integral in the last line is equal to \(2\pi I_0(\sqrt{x^2+y^2})\), where \(I_0\) is the modified Bessel function of the first kind. Thus the marginalized posterior is:
\[p(\Theta|d) \propto I_0\left(\left|\sum_i O(h^0_i, d_i)\right|\right) p(\Theta)\exp\left[\frac{1}{2}\sum_i\left( \left<h^0_i, h^0_i\right> - \left<d_i, d_i\right> \right)\right]\]- name = 'marginalized_phase'¶
- class pycbc.inference.models.marginalized_gaussian_noise.MarginalizedPolarization(variable_params, data, low_frequency_cutoff, psds=None, high_frequency_cutoff=None, normalize=False, polarization_samples=1000, **kwargs)[source]¶
Bases:
DistMarg
,BaseGaussianNoise
This likelihood numerically marginalizes over polarization angle
This class implements the Gaussian likelihood with an explicit numerical marginalization over polarization angle. This is accomplished using a fixed set of integration points distribution uniformation between 0 and 2pi. By default, 1000 integration points are used. The ‘polarization_samples’ argument can be passed to set an alternate number of integration points.
- name = 'marginalized_polarization'¶
- class pycbc.inference.models.marginalized_gaussian_noise.MarginalizedTime(variable_params, data, low_frequency_cutoff, psds=None, high_frequency_cutoff=None, normalize=False, **kwargs)[source]¶
Bases:
DistMarg
,BaseGaussianNoise
This likelihood numerically marginalizes over time
This likelihood is optimized for marginalizing over time, but can also handle marginalization over polarization, phase (where appropriate), and sky location. The time series is interpolated using a quadratic apparoximation for sub-sample times.
- name = 'marginalized_time'¶
pycbc.inference.models.relbin module¶
This module provides model classes and functions for implementing a relative binning likelihood for parameter estimation.
- class pycbc.inference.models.relbin.Relative(variable_params, data, low_frequency_cutoff, fiducial_params=None, gammas=None, epsilon=0.5, earth_rotation=False, earth_rotation_mode=2, marginalize_phase=True, **kwargs)[source]¶
Bases:
DistMarg
,BaseGaussianNoise
Model that assumes the likelihood in a region around the peak is slowly varying such that a linear approximation can be made, and likelihoods can be calculated at a coarser frequency resolution. For more details on the implementation, see https://arxiv.org/abs/1806.08792.
This model requires the use of a fiducial waveform whose parameters are near the peak of the likelihood. The fiducial waveform and all template waveforms used in likelihood calculation are currently generated using the SPAtmplt approximant.
For more details on initialization parameters and definition of terms, see
BaseGaussianNoise
.- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied.
data (dict) – A dictionary of data, in which the keys are the detector names and the values are the data (assumed to be unwhitened). All data must have the same frequency resolution.
low_frequency_cutoff (dict) – A dictionary of starting frequencies, in which the keys are the detector names and the values are the starting frequencies for the respective detectors to be used for computing inner products.
figucial_params (dict) – A dictionary of waveform parameters to be used for generating the fiducial waveform. Keys must be parameter names in the form ‘PARAM_ref’ where PARAM is a recognized extrinsic parameter or an intrinsic parameter compatible with the chosen approximant.
gammas (array of floats, optional) – Frequency powerlaw indices to be used in computing frequency bins.
epsilon (float, optional) – Tuning parameter used in calculating the frequency bins. Lower values will result in higher resolution and more bins.
earth_rotation (boolean, optional) – Default is False. If True, then vary the fp/fc polarization values as a function of frequency bin, using a predetermined PN approximation for the time offsets.
**kwargs – All other keyword arguments are passed to
BaseGaussianNoise
.
- static extra_args_from_config(cp, section, skip_args=None, dtypes=None)[source]¶
Adds reading fiducial waveform parameters from config file.
- property likelihood_function¶
- max_curvature_from_reference()[source]¶
Return the maximum change in slope between frequency bins relative to the reference waveform.
- property multi_signal_support¶
The list of classes that this model supports in a multi-signal likelihood
- name = 'relative'¶
- summary_product(h1, h2, bins, ifo)[source]¶
Calculate the summary values for the inner product <h1|h2>
- write_metadata(fp, group=None)[source]¶
Adds writing the fiducial parameters and epsilon to file’s attrs.
- Parameters:
fp (pycbc.inference.io.BaseInferenceFile instance) – The inference file to write to.
group (str, optional) – If provided, the metadata will be written to the attrs specified by group, i.e., to
fp[group].attrs
. Otherwise, metadata is written to the top-level attrs (fp.attrs
).
- class pycbc.inference.models.relbin.RelativeTime(*args, sample_rate=4096, **kwargs)[source]¶
Bases:
Relative
Heterodyne likelihood optimized for time marginalization. In addition it supports phase (dominant-mode), sky location, and polarization marginalization.
- name = 'relative_time'¶
- property ref_snr¶
- class pycbc.inference.models.relbin.RelativeTimeDom(*args, sample_rate=4096, **kwargs)[source]¶
Bases:
RelativeTime
Heterodyne likelihood optimized for time marginalization and only dominant-mode waveforms. This enables the ability to do inclination marginalization in addition to the other forms supportedy by RelativeTime.
- name = 'relative_time_dom'¶
- pycbc.inference.models.relbin.setup_bins(f_full, f_lo, f_hi, chi=1.0, eps=0.1, gammas=None)[source]¶
Construct frequency bins for use in a relative likelihood model. For details, see [Barak, Dai & Venumadhav 2018].
- Parameters:
f_full (array) – The full resolution array of frequencies being used in the analysis.
f_lo (float) – The starting frequency used in matched filtering. This will be the left edge of the first frequency bin.
f_hi (float) – The ending frequency used in matched filtering. This will be the right edge of the last frequency bin.
chi (float, optional) – Tunable parameter, see [Barak, Dai & Venumadhav 2018]
eps (float, optional) – Tunable parameter, see [Barak, Dai & Venumadhav 2018]. Lower values result in larger number of bins.
gammas (array, optional) – Frequency powerlaw indices to be used in computing bins.
- Returns:
nbin (int) – Number of bins.
fbin (numpy.array of floats) – Bin edge frequencies.
fbin_ind (numpy.array of ints) – Indices of bin edges in full frequency array.
pycbc.inference.models.relbin_cpu module¶
Optimized inner loop functions for the relative likelihood model
- pycbc.inference.models.relbin_cpu.likelihood_parts(freqs, fp, fc, dtc, hp, hc, h00, a0, a1, b0, b1)¶
- pycbc.inference.models.relbin_cpu.likelihood_parts_det(freqs, dtc, hp, h00, a0, a1, b0, b1)¶
- pycbc.inference.models.relbin_cpu.likelihood_parts_det_multi(freqs, dtc, hp, h00, dtc2, hp2, h002, a0, a1)¶
- pycbc.inference.models.relbin_cpu.likelihood_parts_multi(freqs, fp, fc, dtc, hp, hc, h00, fp2, fc2, dtc2, hp2, hc2, h002, a0, a1)¶
- pycbc.inference.models.relbin_cpu.likelihood_parts_multi_v(freqs, fp, fc, dtc, hp, hc, h00, fp2, fc2, dtc2, hp2, hc2, h002, a0, a1)¶
- pycbc.inference.models.relbin_cpu.likelihood_parts_v(freqs, fp, fc, dtc, hp, hc, h00, a0, a1, b0, b1)¶
- pycbc.inference.models.relbin_cpu.likelihood_parts_v_pol(freqs, fp, fc, dtc, pol_phase, hp, hc, h00, a0, a1, b0, b1)¶
- pycbc.inference.models.relbin_cpu.likelihood_parts_v_pol_time(freqs, fp, fc, times, dtc, pol_phase, hp, hc, h00, a0, a1, b0, b1)¶
- pycbc.inference.models.relbin_cpu.likelihood_parts_v_time(freqs, fp, fc, times, dtc, hp, hc, h00, a0, a1, b0, b1)¶
- pycbc.inference.models.relbin_cpu.likelihood_parts_vector(freqs, fp, fc, dtc, hp, hc, h00, a0, a1, b0, b1)¶
- pycbc.inference.models.relbin_cpu.likelihood_parts_vectorp(freqs, fp, fc, dtc, hp, hc, h00, a0, a1, b0, b1)¶
- pycbc.inference.models.relbin_cpu.likelihood_parts_vectort(freqs, fp, fc, dtc, hp, hc, h00, a0, a1, b0, b1)¶
- pycbc.inference.models.relbin_cpu.snr_predictor(freqs, tstart, delta_t, num_samples, hp, hc, h00, a0, a1, b0, b1)¶
- pycbc.inference.models.relbin_cpu.snr_predictor_dom(freqs, tstart, delta_t, num_samples, hp, h00, a0, a1, b0, b1)¶
pycbc.inference.models.single_template module¶
This module provides model classes that assume the noise is Gaussian.
- class pycbc.inference.models.single_template.SingleTemplate(variable_params, data, low_frequency_cutoff, sample_rate=32768, marginalize_phase=True, **kwargs)[source]¶
Bases:
DistMarg
,BaseGaussianNoise
Model that assumes we know all the intrinsic parameters.
This model assumes we know all the intrinsic parameters, and are only maximizing over the extrinsic ones. We also assume a dominant mode waveform approximant only and non-precessing.
- Parameters:
variable_params ((tuple of) string(s)) – A tuple of parameter names that will be varied.
data (dict) – A dictionary of data, in which the keys are the detector names and the values are the data (assumed to be unwhitened). All data must have the same frequency resolution.
low_frequency_cutoff (dict) – A dictionary of starting frequencies, in which the keys are the detector names and the values are the starting frequencies for the respective detectors to be used for computing inner products.
sample_rate (int, optional) – The sample rate to use. Default is 32768.
polarization_samples (int, optional) – Parameter to specify how finely to marginalize over polarization angle. If None, then polarization must be a parameter.
**kwargs – All other keyword arguments are passed to
BaseGaussianNoise
; see that class for details.
- property multi_signal_support¶
The list of classes that this model supports in a multi-signal likelihood
- name = 'single_template'¶
pycbc.inference.models.tools module¶
Common utility functions for calculation of likelihoods
- class pycbc.inference.models.tools.DistMarg[source]¶
Bases:
object
Help class to add bookkeeping for likelihood marginalization
- property current_params¶
The current parameters
If a parameter has been vector marginalized, the likelihood should expect an array for the given parameter. This allows transparent vectorization for many models.
- distance_interpolator = None¶
- distance_marginalization = None¶
- draw_ifos(snrs, peak_snr_threshold=4.0, log=True, precalculate_marginalization_points=False, **kwargs)[source]¶
Helper utility to determine which ifos we should use based on the reference SNR time series.
- draw_sky_times(snrs, size=None)[source]¶
Draw ra, dec, and tc together using SNR timeseries to determine monte-carlo weights.
- draw_times(snrs, size=None)[source]¶
Draw times consistent with the incoherent network SNR
- Parameters:
snrs (dist of TimeSeries) –
- get_precalc_antenna_factors(ifo)[source]¶
Get the antenna factors for marginalized samples if they exist
- marginalize_loglr(sh_total, hh_total, skip_vector=False, return_peak=False)[source]¶
Return the marginal likelihood
- Parameters:
sh_total (float or ndarray) – The total <s|h> inner product summed over detectors
hh_total (float or ndarray) – The total <h|h> inner product summed over detectors
skip_vector (bool, False) – If true, and input is a vector, do not marginalize over that vector, instead return the likelihood values as a vector.
- marginalize_phase = None¶
- reconstruct(rec=None, seed=None, set_loglr=None)[source]¶
Reconstruct the distance or vectored marginalized parameter of this class.
- setup_marginalization(variable_params, marginalize_phase=False, marginalize_distance=False, marginalize_distance_param='distance', marginalize_distance_samples=10000, marginalize_distance_interpolator=False, marginalize_distance_snr_range=None, marginalize_distance_density=None, marginalize_vector_params=None, marginalize_vector_samples=1000.0, marginalize_sky_initial_samples=1000000.0, **kwargs)[source]¶
Setup the model for use with distance marginalization
This function sets up precalculations for distance / phase marginalization. For distance margininalization it modifies the model to internally remove distance as a parameter.
- Parameters:
variable_params (list of strings) – The set of variable parameters
marginalize_phase (bool, False) – Do analytic marginalization (appopriate only for 22 mode waveforms)
marginalize_distance (bool, False) – Marginalize over distance
marginalize_distance_param (str) – Name of the parameter that is used to determine the distance. This might be ‘distance’ or a parameter which can be converted to distance by a provided univariate transformation.
marginalize_distance_interpolator (bool) – Use a pre-calculated interpolating function for the distance marginalized likelihood.
marginalize_distance_snr_range (tuple of floats, (1, 50)) – The SNR range for the interpolating function to be defined in. If a sampler goes outside this range, the logl will be returned as -numpy.inf.
marginalize_distance_density (tuple of intes, (1000, 1000)) – The dimensions of the interpolation grid over (sh, hh).
- Returns:
variable_params (list of strings) – Set of variable params (missing distance-related parameter).
kwags (dict) – The keyword arguments to the model initialization, may be modified from the original set by this function.
- setup_peak_lock(sample_rate=4096, snrs=None, peak_lock_snr=None, peak_lock_ratio=10000.0, peak_lock_region=4, **kwargs)[source]¶
Determine where to constrain marginalization based on the observed reference SNR peaks.
- Parameters:
sample_rate (float) – The SNR sample rate
snrs (Dict of SNR time series) – Either provide this or the model needs a function to get the reference SNRs.
peak_lock_snr (float) – The minimum SNR to bother restricting from the prior range
peak_lock_ratio (float) – The likelihood ratio (not log) relative to the peak to act as a threshold bounding region.
peak_lock_region (int) – Number of samples to inclue beyond the strict region determined by the relative likelihood
- pycbc.inference.models.tools.draw_sample(loglr, size=None)[source]¶
Draw a random index from a 1-d vector with loglr weights
- pycbc.inference.models.tools.marginalize_likelihood(sh, hh, logw=None, phase=False, distance=False, skip_vector=False, interpolator=None, return_peak=False, return_complex=False)[source]¶
Return the marginalized likelihood.
Apply various marginalizations to the data, including phase, distance, and brute-force vector marginalizations. Several options relate to how the distance marginalization is approximated and others allow for special return products to aid in parameter reconstruction.
- Parameters:
sh (complex float or numpy.ndarray) – The data-template inner product
hh (complex float or numpy.ndarray) – The template-template inner product
logw – log weighting factors if vector marginalization is used, if not given, each sample is assumed to be equally weighted
phase (bool, False) – Enable phase marginalization. Only use if orbital phase can be related to just a single overall phase (e.g. not true for waveform with sub-dominant modes)
skip_vector (bool, False) – Don’t apply marginalization of vector component of input (i.e. leave as vector).
interpolator (function, None) – If provided, internal calculation is skipped in favor of a precalculated interpolating function which takes in sh/hh and returns the likelihood.
return_peak (bool, False) – Return the peak likelihood and index if using passing an array as input in addition to the marginalized over the array likelihood.
return_complex (bool, False) – Return the sh / hh data products before applying phase marginalization. This option is intended to aid in reconstucting phase marginalization and is unlikely to be useful for other purposes.
- Returns:
loglr – The marginalized loglikehood ratio
- Return type:
- pycbc.inference.models.tools.setup_distance_marg_interpolant(dist_marg, phase=False, snr_range=(1, 50), density=(1000, 1000))[source]¶
Create the interpolant for distance marginalization
- Parameters:
dist_marg (tuple of two arrays) – The (dist_loc, dist_weight) tuple which defines the grid for integrating over distance
snr_range (tuple of (float, float)) – Tuple of min, max SNR that the interpolant is expected to work for.
density (tuple of (float, float)) – The number of samples in either dimension of the 2d interpolant
- Returns:
interp – Function which returns the precalculated likelihood for a given inner product sh/hh.
- Return type:
function
Module contents¶
This package provides classes and functions for evaluating Bayesian statistics assuming various noise models.
- class pycbc.inference.models.CallModel(model, callstat, return_all_stats=True)[source]¶
Bases:
object
Wrapper class for calling models from a sampler.
This class can be called like a function, with the parameter values to evaluate provided as a list in the same order as the model’s
variable_params
. In that case, the model is updated with the provided parameters and then thecallstat
retrieved. Ifreturn_all_stats
is set toTrue
, then all of the stats specified by the model’sdefault_stats
will be returned as a tuple, in addition to the stat value.The model’s attributes are promoted to this class’s namespace, so that any attribute and method of
model
may be called directly from this class.This class must be initalized prior to the creation of a
Pool
object.- Parameters:
Examples
Create a wrapper around an instance of the
TestNormal
model, with thecallstat
set tologposterior
:>>> from pycbc.inference.models import TestNormal, CallModel >>> model = TestNormal(['x', 'y']) >>> call_model = CallModel(model, 'logposterior')
Now call on a set of parameter values:
>>> call_model([0.1, -0.2]) (-1.8628770664093453, (0.0, 0.0, -1.8628770664093453))
Note that a tuple of all of the model’s
default_stats
were returned in addition to thelogposterior
value. We can shut this off by togglingreturn_all_stats
:>>> call_model.return_all_stats = False >>> call_model([0.1, -0.2]) -1.8628770664093453
Attributes of the model can be called from the call model. For example:
>>> call_model.variable_params ('x', 'y')
- pycbc.inference.models.get_model(model_name)[source]¶
Retrieve the given model.
- Parameters:
model_name (str) – The name of the model to get.
- Returns:
The requested model.
- Return type:
model
- pycbc.inference.models.get_models()[source]¶
Returns the dictionary of current models.
Ensures that plugins are added to the dictionary first.
- pycbc.inference.models.read_from_config(cp, **kwargs)[source]¶
Initializes a model from the given config file.
The section must have a
name
argument. The name argument corresponds to the name of the class to initialize.- Parameters:
cp (WorkflowConfigParser) – Config file parser to read.
**kwargs – All other keyword arguments are passed to the
from_config
method of the class specified by the name argument.
- Returns:
The initialized model.
- Return type:
cls
- pycbc.inference.models.register_model(model)[source]¶
Makes a custom model available to PyCBC.
The provided model will be added to the dictionary of models that PyCBC knows about, using the model’s
name
attribute. If thename
is the same as a model that already exists in PyCBC, a warning will be printed.- Parameters:
model (pycbc.inference.models.base.BaseModel) – The model to use. The model should be a sub-class of
BaseModel
to ensure it has the correct API for use withinpycbc_inference
.