spey 0.1.0

Smooth inference for reinterpretation studies

Spey: smooth inference for reinterpretation studies

A universal statistics package for reinterpretation studies. See the documentation for details.

Outline

• Installation
• What is Spey?
• Quick start

Installation

If you are using a specific branch you can either use make install or pip install -e .. Note that main branch is not the stable version. Stable version can either be downloaded from releases section or via pypi using the following command

pip install spey

What is Spey?

Spey is a plug-in based statistics tool which aims to collect all likelihood prescriptions under one roof. This provides user the workspace to freely combine different statistical models and study them through a single interface. In order to achieve a module that can be used both with statistical model prescriptions which has been proposed in the past and will be used in the future, Spey uses so-called plug-in system where developers can propose their own statistical model prescription and allow spey to use them.

What a plugin provides

A quick intro on terminology of spey plugins in this section:

• A plugin is an external Python package that provides additional statistical model prescriptions to spey.
• Each plugin may provide one (or more) statistical model prescription, that are accessible directly through spey.
• Depending on the scope of the plugin, you may wish to provide additional (custom) operations and differentiability through various autodif packages such as autograd or jax. As long as they are implemented through set of predefined function names spey can automatically detect and use them within the interface.

Finally, the name "Spey" originally comes from the Spey river, a river in mid-Highlands of Scotland. The area "Speyside" is famous for its smooth whiskey.

Currently available plug-ins

Accessor	Description
"default_pdf.uncorrelated_background"	Constructs uncorrelated multi-bin statistical model.
"default_pdf.correlated_background"	Constructs correlated multi-bin statistical model with Gaussian nuisances.
"default_pdf.third_moment_expansion"	Implements the skewness of the likelihood by using third moments.
"default_pdf.effective_sigma"	Implements the skewness of the likelihood by using asymmetric uncertainties.
"pyhf.uncorrelated_background"	Uses uncorrelated background functionality of pyhf (see spey-phyf plugin).
"pyhf"	Uses generic likelihood structure of pyhf (see spey-phyf plugin)

For details on all the backends, see the Plug-ins section of the documentation.

Quick Start

First one needs to choose which backend to work with. By default, spey is shipped with various types of likelihood prescriptions which can be checked via AvailableBackends function

import spey
print(spey.AvailableBackends())
# ['default_pdf.correlated_background',
#  'default_pdf.effective_sigma',
#  'default_pdf.third_moment_expansion',
#  'default_pdf.uncorrelated_background']

Using 'default_pdf.uncorrelated_background' one can simply create single or multi-bin statistical models:

pdf_wrapper = spey.get_backend('default_pdf.uncorrelated_background')

data = [1]
signal_yields = [0.5]
background_yields = [2.0]
background_unc = [1.1]

stat_model = pdf_wrapper(
    signal_yields=signal_yields,
    background_yields=background_yields,
    data=data,
    absolute_uncertainties=background_unc,
    analysis="single_bin",
    xsection=0.123,
)

where data indicates the observed events, signal_yields and background_yields represents yields for signal and background samples and background_unc shows the absolute uncertainties on the background events i.e. :math:2.0\pm1.1 in this particular case. Note that we also introduced analysis and xsection information which are optional where the analysis indicates a unique identifier for the statistical model and xsection is the cross-section value of the signal which is only used for the computation of the excluded cross section value.

During computation of any probability distribution Spey relies on so-called "expectation type". This can be set via spey.ExpectationType which includes three different expectation mode.

• spey.ExpectationType.observed : Indicates that the computation of the log-probability will be achieved by fitting the statistical model on the experimental data. For the exclusion limit computation this will tell package to compute observed :math:1-CL_s values. spey.ExpectationType.observed has been set as default through out the package.

• spey.ExpectationType.aposteriori: This command will result with the same log-probability computation as spey.ExpectationType.observed. However, expected exclusion limit will be computed by centralising the statistical model on the background and checking :math:\pm1\sigma and :math:\pm2\sigma fluctuations.

• spey.ExpectationType.apriori : Indicates that the obseravation has never take place and the theoretical SM computation is the absolute truth. Thus it replaces observed values in the statistical model with the background values and computes the log-probability accordingly. Similar to spey.ExpectationType.aposteriori exclusion limit computation will return expected limits.

To compute the observed exclusion limit for the above example one can type

for expectation in spey.ExpectationType:
    print(f"1-CLs ({expectation}): {stat_model.exclusion_confidence_level(expected=expectation)}")
# 1-CLs (apriori): [0.49026742260475775, 0.3571003642744075, 0.21302512037071475, 0.1756147641077802, 0.1756147641077802]
# 1-CLs (aposteriori): [0.6959976874809755, 0.5466491036450178, 0.3556261845401908, 0.2623335168616665, 0.2623335168616665]
# 1-CLs (observed): [0.40145846656558726]

Note that spey.ExpectationType.apriori and spey.ExpectationType.aposteriori expectation types resulted in a list of 5 elements which indicates $-2\sigma,\ -1\sigma,\ 0,\ +1\sigma,\ +2\sigma$ standard deviations from the background hypothesis. spey.ExpectationType.observed on the other hand resulted in single value which is observed exclusion limit. Notice that the bounds on spey.ExpectationType.aposteriori are slightly stronger than spey.ExpectationType.apriori this is due to the data value has been replaced with background yields, which is larger than the observations. spey.ExpectationType.apriori is mostly used in theory collaborations to estimate the difference from the Standard Model rather than the experimental observations.

One can play the same game using the same backend for multi-bin histograms as follows;

pdf_wrapper = spey.get_backend('default_pdf.uncorrelated_background')

data = [36, 33]
signal = [12.0, 15.0]
background = [50.0,48.0]
background_unc = [12.0,16.0]

stat_model = pdf_wrapper(
    signal_yields=signal_yields,
    background_yields=background_yields,
    data=data,
    absolute_uncertainties=background_unc,
    analysis="multi_bin",
    xsection=0.123,
)

Note that our statistical model still represents individual bins of the histograms independently however it sums up the log-likelihood of each bin. Hence all bins are completely uncorrelated from each other. Computing the exclusion limits for each spey.ExpectationType will yield

for expectation in spey.ExpectationType:
    print(f"1-CLs ({expectation}): {stat_model.exclusion_confidence_level(expected=expectation)}")
# 1-CLs (apriori): [0.971099302028661, 0.9151646569018123, 0.7747509673901924, 0.5058089246145081, 0.4365406649302913]
# 1-CLs (aposteriori): [0.9989818194986659, 0.9933308419577298, 0.9618669253593897, 0.8317680908087413, 0.5183060229282643]
# 1-CLs (observed): [0.9701795436411219]

It is also possible to compute $1-CL_s$ value with respect to the parameter of interest, $\mu$. This can be achieved by including a value for poi_test argument

import matplotlib.pyplot as plt
import numpy as np

poi = np.linspace(0,10,20)
poiUL = np.array([stat_model.exclusion_confidence_level(poi_test=p, expected=spey.ExpectationType.aposteriori) for p in poi])
plt.plot(poi, poiUL[:,2], color="tab:red")
plt.fill_between(poi, poiUL[:,1], poiUL[:,3], alpha=0.8, color="green", lw=0)
plt.fill_between(poi, poiUL[:,0], poiUL[:,4], alpha=0.5, color="yellow", lw=0)
plt.plot([0,10], [.95,.95], color="k", ls="dashed")
plt.xlabel(r"${\rm signal\ strength}\ (\mu)$")
plt.ylabel("$1-CL_s$")
plt.xlim([0,10])
plt.ylim([0.6,1.01])
plt.text(0.5,0.96, r"$95\%\ {\rm CL}$")
plt.show()

Here in the first line we extract $1-CL_s$ values per POI for spey.ExpectationType.aposteriori expectation type and we plot specific standard deviations which provides following plot:

The excluded value of POI can also be retreived by spey.StatisticalModel.poi_upper_limit function

print("POI UL: %.3f" % stat_model.poi_upper_limit(expected=spey.ExpectationType.aposteriori))
# POI UL:  0.920

which is exact point where red-curve and black dashed line meets. The upper limit for the $\pm1\sigma$ or $\pm2\sigma$ bands can be extracted by setting expected_pvalue to "1sigma" or "2sigma" respectively, e.g.

stat_model.poi_upper_limit(expected=spey.ExpectationType.aposteriori, expected_pvalue="1sigma")
# [0.5507713378348318, 0.9195052042538805, 1.4812721449679866]

At a more lower level, one can extract the likelihood information for the statistical model by calling spey.StatisticalModel.likelihood and spey.StatisticalModel.maximize_likelihood functions. By default these will return negative log-likelihood values but this can be changed via return_nll=False argument.

muhat_obs, maxllhd_obs = stat_model.maximize_likelihood(return_nll=False, )
muhat_apri, maxllhd_apri = stat_model.maximize_likelihood(return_nll=False, expected=spey.ExpectationType.apriori)

poi = np.linspace(-3,4,60)

llhd_obs = np.array([stat_model.likelihood(p, return_nll=False) for p in poi])
llhd_apri = np.array([stat_model.likelihood(p, expected=spey.ExpectationType.apriori, return_nll=False) for p in poi])

Here in first two lines we extracted maximum likelihood and the POI value that maximizes the likelihood for two different expectation type. In the following we computed likelihood distribution for various POI values which then can be plotted as follows

plt.plot(poi, llhd_obs/maxllhd_obs, label=r"${\rm observed\ or\ aposteriori}$")
plt.plot(poi, llhd_apri/maxllhd_apri, label=r"${\rm apriori}$")
plt.scatter(muhat_obs, 1)
plt.scatter(muhat_apri, 1)
plt.legend(loc="upper right")
plt.ylabel(r"$\mathcal{L}(\mu,\theta_\mu)/\mathcal{L}(\hat\mu,\hat\theta)$")
plt.xlabel(r"${\rm signal\ strength}\ (\mu)$")
plt.ylim([0,1.3])
plt.xlim([-3,4])
plt.show()

Notice the slight difference between likelihood distributions, this is because of the use of different expectation types. The dots on the likelihood distribution represents the point where likelihood is maximized. Since for an spey.ExpectationType.apriori likelihood distribution observed and background values are the same, the likelihood should peak at $\mu=0$.