Skip to main content

Classy Probabilistic Programming

Project description

binder Tests Build Documentation Status JOSS

Installation Guide | readthedocs | Introduction on Binder | HowToFit

PyAutoFit is a Python based probabilistic programming language for model fitting and Bayesian inference of large datasets.

The basic PyAutoFit API allows us a user to quickly compose a probabilistic model and fit it to data via a log likelihood function, using a range of non-linear search algorithms (e.g. MCMC, nested sampling).

Users can then set up PyAutoFit scientific workflow, which enables streamlined modeling of small datasets with tools to scale up to large datasets.

PyAutoFit supports advanced statistical methods, most notably a big data framework for Bayesian hierarchical analysis.

Getting Started

The following links are useful for new starters:

Support

Support for installation issues, help with Fit modeling and using PyAutoFit is available by raising an issue on the GitHub issues page.

We also offer support on the PyAutoFit Slack channel, where we also provide the latest updates on PyAutoFit. Slack is invitation-only, so if you’d like to join send an email requesting an invite.

HowToFit

For users less familiar with Bayesian inference and scientific analysis you may wish to read through the HowToFits lectures. These teach you the basic principles of Bayesian inference, with the content pitched at undergraduate level and above.

A complete overview of the lectures is provided on the HowToFit readthedocs page

API Overview

To illustrate the PyAutoFit API, we use an illustrative toy model of fitting a one-dimensional Gaussian to noisy 1D data. Here’s the data (black) and the model (red) we’ll fit:

https://raw.githubusercontent.com/rhayes777/PyAutoFit/main/files/toy_model_fit.png

We define our model, a 1D Gaussian by writing a Python class using the format below:

class Gaussian:

    def __init__(
        self,
        centre=0.0,        # <- PyAutoFit recognises these
        normalization=0.1, # <- constructor arguments are
        sigma=0.01,        # <- the Gaussian's parameters.
    ):
        self.centre = centre
        self.normalization = normalization
        self.sigma = sigma

    """
    An instance of the Gaussian class will be available during model fitting.

    This method will be used to fit the model to data and compute a likelihood.
    """

    def model_data_from(self, xvalues):

        transformed_xvalues = xvalues - self.centre

        return (self.normalization / (self.sigma * (2.0 * np.pi) ** 0.5)) * \
                np.exp(-0.5 * (transformed_xvalues / self.sigma) ** 2.0)

PyAutoFit recognises that this Gaussian may be treated as a model component whose parameters can be fitted for via a non-linear search like emcee.

To fit this Gaussian to the data we create an Analysis object, which gives PyAutoFit the data and a log_likelihood_function describing how to fit the data with the model:

class Analysis(af.Analysis):

    def __init__(self, data, noise_map):

        self.data = data
        self.noise_map = noise_map

    def log_likelihood_function(self, instance):

        """
        The 'instance' that comes into this method is an instance of the Gaussian class
        above, with the parameters set to values chosen by the non-linear search.
        """

        print("Gaussian Instance:")
        print("Centre = ", instance.centre)
        print("normalization = ", instance.normalization)
        print("Sigma = ", instance.sigma)

        """
        We fit the ``data`` with the Gaussian instance, using its
        "model_data_from" function to create the model data.
        """

        xvalues = np.arange(self.data.shape[0])

        model_data = instance.model_data_from(xvalues=xvalues)
        residual_map = self.data - model_data
        chi_squared_map = (residual_map / self.noise_map) ** 2.0
        log_likelihood = -0.5 * sum(chi_squared_map)

        return log_likelihood

We can now fit our model to the data using a non-linear search:

model = af.Model(Gaussian)

analysis = Analysis(data=data, noise_map=noise_map)

emcee = af.Emcee(nwalkers=50, nsteps=2000)

result = emcee.fit(model=model, analysis=analysis)

The result contains information on the model-fit, for example the parameter samples, maximum log likelihood model and marginalized probability density functions.

Project details


Release history Release notifications | RSS feed

Download files

Download the file for your platform. If you're not sure which to choose, learn more about installing packages.

Source Distribution

autofit-2024.11.13.2.tar.gz (277.6 kB view details)

Uploaded Source

Built Distribution

autofit-2024.11.13.2-py3-none-any.whl (389.2 kB view details)

Uploaded Python 3

File details

Details for the file autofit-2024.11.13.2.tar.gz.

File metadata

  • Download URL: autofit-2024.11.13.2.tar.gz
  • Upload date:
  • Size: 277.6 kB
  • Tags: Source
  • Uploaded using Trusted Publishing? No
  • Uploaded via: twine/5.1.1 CPython/3.10.12

File hashes

Hashes for autofit-2024.11.13.2.tar.gz
Algorithm Hash digest
SHA256 1bb2b42d4136924a756a9f6d5f8c7463fad09dd60c429198efe51158b0359ea1
MD5 b49269e6c6682c1ad19b83b60b535744
BLAKE2b-256 99f552bde1d129aa8bee82515742167d3fd2655d9b9bcffcb4ee0a8fbee07ffe

See more details on using hashes here.

File details

Details for the file autofit-2024.11.13.2-py3-none-any.whl.

File metadata

File hashes

Hashes for autofit-2024.11.13.2-py3-none-any.whl
Algorithm Hash digest
SHA256 303abd6faa7b416e702d344892bd1afc8e1f7272a8ddcac120a9e1db91f3c563
MD5 e1de98d22628c8723a311bac0d62dccc
BLAKE2b-256 24ab7de7bf885b9ac78bc568acc4ba38c7ee33cae09bdf552636387870e7c24d

See more details on using hashes here.

Supported by

AWS AWS Cloud computing and Security Sponsor Datadog Datadog Monitoring Fastly Fastly CDN Google Google Download Analytics Microsoft Microsoft PSF Sponsor Pingdom Pingdom Monitoring Sentry Sentry Error logging StatusPage StatusPage Status page