pint.mcmc_fitter.MCMCFitterAnalyticTemplate
- class pint.mcmc_fitter.MCMCFitterAnalyticTemplate(toas, model, sampler, template, **kwargs)[source]
Bases:
MCMCFitter
A subclass of MCMCFitter, designed to use an analytic template rather than a binned one that uses interpolation.
Methods
auto
(toas, model[, downhill, track_mode, ...])Automatically return the proper
pint.fitter.Fitter
object depending on the TOAs and model.clip_template_params
(pos)If template parameters are changeable, ensure that they are within bounds Any passing the template bounds will be clipped to the edges.
fit_toas
([maxiter, pos, errfact, priorerrfact])Fitting function - calls sampler.run_mcmc to converge using MCMC approach
ftest
(parameter, component[, remove, ...])Compare the significance of adding/removing parameters to a timing model.
Read the model to determine fitted keys and their values and errors from the par file
Return a dict of all param names and values.
get_derived_params
([returndict])Return a string with various derived parameters from the fitted model
Return the model's design matrix for these TOAs.
Get errors associated with all fit parameters
Return pulse phases based on the current model
Basic getter, useful in event_optimize script
Return a dict of fittable param names and quantity.
Return a dict of fittable param names and numeric values.
Return a dict of fittable param names and numeric values.
get_model_parameters
(theta)Split the parameters related to the model
Show the parameter correlation matrix post-fit.
Show the parameter covariance matrix post-fit.
Get parameter names for this fitter
Get all parameters for this fitter
get_params_dict
([which, kind])Return a dict mapping parameter names to values.
get_summary
([nodmx])Return a human-readable summary of the Fitter results.
get_template_parameters
(theta)Split the parameters related to the template
get_template_vals
(phases)Use the template (if it exists) to get probabilities for given phases
get_weights
()lnposterior
(theta)The log posterior (priors * likelihood)
make_resids
(model)minimize_func
(theta)Override superclass minimize_func to make compatible with scipy.optimize
phaseogram
([weights, bins, rotate, size, ...])Make a nice 2-panel phaseogram for the current model
plot
()Make residuals plot.
plot_priors
(chains, burnin[, bins, scale])Write a summary of the TOAs to stdout.
prof_vs_weights
([nbins, use_weights])Show binned profiles (and H-test values) as a function of the minimum weight used.
Reset the current model to the initial model.
set_fitparams
(*params)Update the "frozen" attribute of model parameters.
set_param_uncertainties
(fitp)Set the model parameters to the value contained in the input dict.
set_parameters
(theta)Set timing and template parameters as necessary
set_params
(fitp)Set the model parameters to the value contained in the input dict.
set_template
(template)Metadata for analytic template
update_model
([chi2])Update the model to reflect fit results and TOA properties.
Update the residuals.
Attributes
covariance_matrix
- get_template_vals(phases)[source]
Use the template (if it exists) to get probabilities for given phases
- clip_template_params(pos)[source]
If template parameters are changeable, ensure that they are within bounds Any passing the template bounds will be clipped to the edges. If template is not being fit to, then this does nothing
- classmethod auto(toas, model, downhill=True, track_mode=None, residuals=None, **kwargs)
Automatically return the proper
pint.fitter.Fitter
object depending on the TOAs and model.In general the downhill fitters are to be preferred. See https://github.com/nanograv/PINT/wiki/How-To#choose-a-fitter for the logic used.
- Parameters:
toas (a pint TOAs instance) – The input toas.
model (a pint timing model instance) – The initial timing model for fitting.
downhill (bool, optional) – Whether or not to use the downhill fitter variant
track_mode (str, optional) – How to handle phase wrapping. This is used when creating
pint.residuals.Residuals
objects, and its meaning is defined there.residuals (
pint.residuals.Residuals
) – Initial residuals. This argument exists to support an optimization, whereGLSFitter
is used to computechi2
for appropriate Residuals objects.
- Returns:
Returns appropriate subclass
- Return type:
- fit_toas(maxiter=100, pos=None, errfact=0.1, priorerrfact=10.0)
Fitting function - calls sampler.run_mcmc to converge using MCMC approach
- Parameters:
- ftest(parameter, component, remove=False, full_output=False, maxiter=1)
Compare the significance of adding/removing parameters to a timing model.
- Parameters:
parameter (PINT parameter object) – (may be a list of parameter objects)
component (String) – Name of component of timing model that the parameter should be added to (may be a list) The number of components must equal number of parameters.
remove (Bool) – If False, will add the listed parameters to the model. If True will remove the input parameters from the timing model.
full_output (Bool) – If False, just returns the result of the F-Test. If True, will also return the new model’s residual RMS (us), chi-squared, and number of degrees of freedom of new model.
maxiter (int) – How many times to run the linear least-squares fit, re-evaluating the derivatives at each step for the F-tested model. Default is one.
- Returns:
- ftFloat
F-test significance value for the model with the larger number of components over the other. Computed with pint.utils.FTest().
- resid_rms_testFloat (Quantity)
If full_output is True, returns the RMS of the residuals of the tested model fit. Will be in units of microseconds as an astropy quantity. If wideband fitter this will be the time residuals.
- resid_wrms_testFloat (Quantity)
If full_output is True, returns the Weighted RMS of the residuals of the tested model fit. Will be in units of microseconds as an astropy quantity. If wideband fitter this will be the time residuals.
- chi2_testFloat
If full_output is True, returns the chi-squared of the tested model. If wideband fitter this will be the total chi-squared of the combined residual.
- dof_testInt
If full_output is True, returns the degrees of freedom of the tested model. If wideband fitter this will be the total chi-squared of the combined residual.
- dm_resid_rms_testFloat (Quantity)
If full_output is True and a wideband timing fitter is used, returns the RMS of the DM residuals of the tested model fit. Will be in units of pc/cm^3 as an astropy quantity.
- dm_resid_wrms_testFloat (Quantity)
If full_output is True and a wideband timing fitter is used, returns the Weighted RMS of the DM residuals of the tested model fit. Will be in units of pc/cm^3 as an astropy quantity.
- Return type:
dictionary
- generate_fit_keyvals()
Read the model to determine fitted keys and their values and errors from the par file
- get_allparams()
Return a dict of all param names and values. Deprecated.
- get_derived_params(returndict=False)
Return a string with various derived parameters from the fitted model
- Parameters:
returndict (bool, optional) – Whether to only return the string of results or also a dictionary
- Returns:
results (str)
parameters (dict, optional)
- get_designmatrix()
Return the model’s design matrix for these TOAs.
- get_event_phases()
Return pulse phases based on the current model
- get_fit_keyvals()
Basic getter, useful in event_optimize script
- get_fitparams()
Return a dict of fittable param names and quantity. Deprecated.
- get_fitparams_num()
Return a dict of fittable param names and numeric values. Deprecated.
- get_fitparams_uncertainty()
Return a dict of fittable param names and numeric values. Deprecated.
- get_parameter_correlation_matrix(with_phase=False, pretty_print=False, prec=3, usecolor=True)
Show the parameter correlation matrix post-fit.
If with_phase, then show and return the phase column as well. If pretty_print, then also pretty-print on stdout the matrix. prec is the precision of the floating point results. If usecolor is True, then pretty printing will have color.
- get_parameter_covariance_matrix(with_phase=False, pretty_print=False, prec=3)
Show the parameter covariance matrix post-fit.
If with_phase, then show and return the phase column as well. If pretty_print, then also pretty-print on stdout the matrix. prec is the precision of the floating point results.
- get_params_dict(which='free', kind='quantity')
Return a dict mapping parameter names to values.
- get_summary(nodmx=False)
Return a human-readable summary of the Fitter results.
- Parameters:
nodmx (bool) – Set to True to suppress printing DMX parameters in summary
- lnposterior(theta)
The log posterior (priors * likelihood)
- minimize_func(theta)
Override superclass minimize_func to make compatible with scipy.optimize
- phaseogram(weights=None, bins=100, rotate=0.0, size=5, alpha=0.25, plotfile=None)
Make a nice 2-panel phaseogram for the current model
- plot()
Make residuals plot.
This produces a time residual plot.
- print_summary()
Write a summary of the TOAs to stdout.
- prof_vs_weights(nbins=50, use_weights=False)
Show binned profiles (and H-test values) as a function of the minimum weight used. nbins is only for the plots.
- reset_model()
Reset the current model to the initial model.
- set_fitparams(*params)
Update the “frozen” attribute of model parameters. Deprecated.
- set_param_uncertainties(fitp)
Set the model parameters to the value contained in the input dict.
See
pint.models.timing_model.TimingModel.set_param_uncertainties()
.
- set_params(fitp)
Set the model parameters to the value contained in the input dict.
See
pint.models.timing_model.TimingModel.set_param_values()
.
- update_model(chi2=None)
Update the model to reflect fit results and TOA properties.
This is called by
fit_toas
to ensure that parameters likeSTART
,FINISH
,EPHEM
, andDMDATA
are set in the model to reflect the TOAs in actual use.
- update_resids()
Update the residuals.
Run after updating a model parameter.