Classy non-linear optimisation
Project description
PyAutoFit
PyAutoFit is a Python-based probablistic programming language that allows Bayesian inference techniques to be straightforwardly integrated into scientific modeling software. PyAutoFit specializes in:
- Black box models with complex and expensive likelihood functions.
- Fitting many different model parametrizations to a data-set.
- Modeling extremely large-datasets with a homogenous fitting procedure.
- Automating complex model-fitting tasks via transdimensional model-fitting pipelines.
API Overview
PyAutoFit interfaces with Python classes and non-linear sampling packages such as PyMultiNest. Lets take a two-dimensional Gaussian as our moodel:
class Gaussian:
def __init__(
self,
centre = (0.0, 0.0), # <- PyAutoFit recognises these constructor arguments are the model
intensity = 0.1, # <- parameters of the Gaussian.
sigma = 0.01,
):
self.centre = centre
self.intensity = intensity
self.sigma = sigma
PyAutoFit recognises that this Gaussian may be treated as a model component whose parameters could be fitted for by a non-linear search. To fit this Gaussian to some data we can create and run a PyAutoFit phase:
import autofit as af
# To perform the analysis we set up a phase, which takes the Gaussian as the
# model & fits its parameters using the non-linear search MultiNest.
phase = af.Phase(model=af.Gaussian, phase_name="phase_example", non_linear_class=af.MultiNest)
# We pass a dataset to the phase, fitting it with the model above.
phase.run(dataset=dataset)
By interfacing with Python classes PyAutoFit takes care of the 'heavy lifting' that comes with parametrizing and fitting the model. This includes interfacing with the non-linear search, storing results in structured directories and providing on-the-fly output and visusalization.
Features
Model Customization
PyAutoFit makes it straight forward to parameterize, customize and fit models made of multiple components. Below, we extend the example above to include a second Gaussian, with user-specified priors and a centre aligned with the first Gaussian:
import autofit as af
# The model can be setup with multiple classes and before passing it to a phase and
# we can customize the model parameters.
model = af.CollectionPriorModel(
gaussian_0=af.Gaussian, gaussian_1=af.Gaussian, exponential=af.Exponential
)
# This aligns the centres of the Gaussian and Exponential, reducing the number of free parameters by 1.
model.gaussian_0.centre = model.exponential.centre
# This fixes the Gaussian's sigma value to 0.5, reducing the number of free parameters by 1.
model.gaussian_1.sigma = 0.5
# We can customize the priors on any model parameter.
model.gaussian_0.intensity = af.LogUniformPrior(lower_limit=1e-6, upper_limit=1e6)
model.exponential.rate = af.GaussianPrior(mean=0.1, sigma=0.05)
# We can make assertions on parameters which remove regions of parameter space where these are not valid
model.add_assertion(model.exponential.intensity > 0.5)
# We pass the customized model to a phase to fit it via a non-linear search.
phase = af.Phase(model=model, phase_name="phase_example", non_linear_class=af.MultiNest)
Aggregation
For fits to large data-sets PyAutoFit provides tools to manipulate the vast library of results output.
Lets pretend we performed the Gaussian fit above to 100 indepedent data-sets. Every PyAutoFit output contains metadata meaning that we can immediately load it via the aggregator into a Python script or Jupyter notebook:
import autofit as af
# Lets pretend we've used a Phase object to fit 100 different datasets with the same model. The results of these 100
# fits are in a structured output format in this folder.
output_path = "/path/to/gaussian_x100_fits/"
# To create an instance of the aggregator, we pass it the output path above. The aggregator will detect that
# 100 fits using a specific phase have been performed and that their results are in this folder.
aggregator = af.Aggregator(directory=str(output_path))
# The aggregator can now load results from these fits. The command below loads results as instances of the
# NonLinearOutput class which provides an interface to the non-linear search output of every phase's fit.
non_linear_outputs = aggregator.output
# The results of all 100 non-linear searches are now available. The command below creates a list of instances of the
# best-fit model parameters of all 100 model fits (many other results are available, e.g. marginalized 1D parameter
# estimates, errors, Bayesian evidences, etc.).
instances = [output.most_likely_instance for output in non_linear_outputs]
# These are instances of the 'model-components' defined using the PyAutoFit Python class format illustrated in figure 1.
# For the Gaussian class, each instance in this list is an instance of this class and its parameters are accessible.
print("Instance Parameters \n")
print("centre = ", instances[0].centre)
print("intensity = ", instances[0].intensity)
print("sigma = ", instances[0].sigma)
# The aggregator can be customized to interface with model-specific aspects of a project like the data and fitting
# procedure. Below, the aggregator has been set up to provide instances of of all 100 datasets, masks and fits.
datasets = aggregator.dataset
masks = aggregator.mask
fits = aggregator.fit
# If the datasets are fitted with many different phases (e.g. with different models), the aggregator's filter tool can
# be used to load results of a specific phase (and therefore model).
phase_name = "phase_example"
non_linear_outputs = aggregator.filter(phase=phase_name).output
If many different phases are used to perform different model-fits to a data-set, the aggregator provides tools to filter out results.
Transdimensional Modeling
In transdimensional modeling many different models are paramertized and fitted to the same data-set.
This is performed using transdimensional model-fitting pipelines, which break the model-fit into a series of linked non-linear searches, or phases. Initial phases fit simplified realizations of the model, whose results are used to initialize fits using more complex models in later phases.
Fits of complex models with large dimensionality can therefore be broken down into a series of bite-sized model fits, allowing even the most complex model fitting problem to be fully automated.
Lets illustrate this with an example fitting two 2D Gaussians:
We're going to fit each with the 2D Gaussian profile above. Traditional approaches would fit both Gaussians simultaneously, making parameter space more complex, slower to sample and increasing the risk that we fail to locate the global maxima solution. With PyAutoFit we can instead build a transdimensional model fitting pipeline which breaks the the analysis down into 3 phases:
- Fit only the left Gaussian.
- Fit only the right Gaussian, using the model of the left Gaussian from phase 1 to reduce blending.
- Fit both Gaussians simultaneously, using the results of phase 1 & 2 to initialize where the non-linear optimizer searches parameter space.
import autofit as af
def make_pipeline():
# In phase 1, we will fit the Gaussian on the left.
phase1 = af.Phase(
phase_name="phase_1__left_gaussian",
gaussians=af.CollectionPriorModel(gaussian_0=af.profiles.Gaussian),
non_linear_class=af.MultiNest,
)
# In phase 2, we will fit the Gaussian on the right, where the best-fit Gaussian
# resulting from phase 1 above fits the left-hand Gaussian.
phase2 = af.Phase(
phase_name="phase_2__right_gaussian",
phase_folders=phase_folders,
gaussians=af.CollectionPriorModel(
gaussian_0=phase1.result.instance.gaussians.gaussian_0, # <- Use the Gaussian fitted in phase 1
gaussian_1=gaussian_1,
),
non_linear_class=af.MultiNest,
)
# In phase 3, we fit both Gaussians, using the results of phases 1 and 2 to
# initialize their model parameters.
phase3 = af.Phase(
phase_name="phase_3__both_gaussian",
phase_folders=phase_folders,
gaussians=af.CollectionPriorModel(
gaussian_0=phase1.result.model.gaussians.gaussian_0, # <- use phase 1 Gaussian results.
gaussian_1=phase2.result.model.gaussians.gaussian_1, # <- use phase 2 Gaussian results.
),
non_linear_class=af.MultiNest,
)
return toy.Pipeline(pipeline_name, phase1, phase2, phase3)
Althoguh somewhat trivial, this example illustrates how easily a model-fit can be broken down with PyAutoFit.
PyAutoLens shows a real-use case of transdimensional modeling, fitting galaxy-scale strong gravitational lenses. In this example pipeline, a 5-phase PyAutoFit pipeline breaks-down the fit of 5 diferent models composed of over 10 unique model components and 10-30 free parameters.
Future
The following features are planned for 2020:
- Bayesian Model Comparison - Determine the most probable model via the Bayesian evidence.
- Generalized Linear Models - Fit for global trends to model fits to large data-sets.
- Hierarchical modeling - Combine fits over multiple data-sets to perform hierarchical inference.
- Time series modelling - Fit temporally varying models using fits which marginalize over time.
- Approximate Bayesian Computation - Likelihood-free modeling.
- Transdimensional Sampling - Sample non-linear parameter spaces with variable numbers of model components and parameters.
Slack
We're building a PyAutoFit community on Slack, so you should contact us on our Slack channel before getting started. Here, I will give you the latest updates on the software & discuss how best to use PyAutoFit for your science case.
Unfortunately, Slack is invitation-only, so first send me an email requesting an invite.
Depedencies
PyAutoFit requires PyMultiNest.
Installation with conda
We recommend installation using a conda environment as this circumvents a number of compatibility issues when installing PyMultiNest.
First, install conda.
Create a conda environment:
conda create -n autofit python=3.7 anaconda
Activate the conda environment:
conda activate autofit
Install multinest:
conda install -c conda-forge multinest
Install autofit:
pip install autofit
Installation with pip
Installation is also available via pip, however there are reported issues with installing PyMultiNest that can make installation difficult, see the file INSTALL.notes
$ pip install autofit
Support & Discussion
If you're having difficulty with installation, lens modeling, or just want a chat, feel free to message us on our Slack channel.
Contributing
If you have any suggestions or would like to contribute please get in touch.
Credits
Developers
Richard Hayes - Lead developer
James Nightingale - Lead developer
Project details
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