Skip to content

kcrum/toy_2D_fit

Repository files navigation

#Toy 2-D Fit Tests

This contains code that runs fits to fake data where each event has an energy and deltaT. The fake data comes from two "isotopes," both of which have different energy end points and exponential decay time constants. The fit will attempt to measure the normalizations of these two spectra (so there will be two free parameters).

I want to test whether simultaneously fitting both of the 1-D distributions is unbiased; I also want to observe the behavior of the chi^2 for many fake fits. I will also fit the (presumably correct) 2-D distribution, checking again for unbiased estimators and proper chi^2 behavior. The relevant source code is contained in physicsPDFs.py and toy_2D_fits.py. You can ignore the file called class_tests.py.

Also I wrote a blog post which uses this code.

Running fake fits

The fake data in the fits done here are pulled from energy and time distributions, much like if one were observing Li-9 or He-8 decays. The energy spectrum form is specified in physicsPDFs.py by the "ParabolicPDF" class, and it is a parabola of the form ~x*(x-endpoint), where the user specifies the endpoint. The time spectrum is an exponential from the "TruncatedExponentialPDF" class with user-specified lifetime, as well as a user-specified maximum time. We generate fake data pulling from energy and time distributions for two 'isotopes,' each with its own spectral endpoint and lifetime.

Fake data is generated and then fit by the "mainloop" function in toy_2D_fits.py. Four different fits are run to extract the normalization of the two isotopes in each fake experiment:

  • A least-squares fit to the 4 energy bins and 4 time bins, using the Pearson treatment for statistical errors.
  • A least-squares fit to the combined 16 (4x4) energy and time bins, using the Pearson treatment for statistical errors.
  • A maximum likelihood fit to the 4 energy bins and 4 time bins, using a Poisson pdf for each of the 8 bins.
  • A maximum likelihood fit to the combined 16 (4x4) energy and time bins, using a Poisson pdf for each of the 16 bins.

By default the endpoints are 12 and 8 (arb. units) for isotope0 and isotope1, respectively. The four energy bins span the range from 0 to 12. Isotope0 has a default lifetime of 260, while isotope1 has a default lifetime of 170 (arb. units). The time bins span 0 to 260.

By making the following call from the command line:

python toy_2D_fits.py 1000 1000 100 toyfits_1000exp_1000n0_100n1.txt

you should be able to reproduce the output in toyfits_1000exp_1000n0_100n1.txt. This contains the fits of 1,000 fake experiments, each having 1,000 events pulled from isotope0 and 100 events pulled from isotope1. N.B.: this will take an hour or two to run.

What to do with fake data

You can read the fake data in toyfits_1000exp_1000n0_100n1.txt into a pandas data frame with the following call:

data = pandas.read_csv('toy_fits_1000exp_1000n0_100n1.txt')

One point this code is meant to illustrate is that the naive definition of degrees of freedom = # of bins - # of free parameters is not always correct. If you histogram the calculated p-values of the 2-D fits (calling plt.hist(data.pval_2D)), you'll correctly see a uniform distribution (what one expects in a well behaved chi^2 fit), as the p-values were calculated assuming 16 - 2 = 14 degrees of freedom. If you histogram the calculated p-values of the 1-D fits (calling plt.hist(data.pval_1D)), you'll see a non-uniform distribution, as the p-values were calculated assuming 8 - 2 = 6 degrees of freedom.

The reason the 1-D fits don't yield uniform p-values is due to the fact that the two 4-bin data vectors have the same total number of entries. This effectively removes one data bin, since if you know the contents of 7 out of the 8 bins, there is no freedom in the number of events of that 8th bin. This isn't the case in the 4 x 4 2-D fits, since each bin is truly a unique observation.

You can also histogram the best fit values from the various fits for n0 (normalization of isotope 0) and n1 (normalization of isotope 1). Comparing the best fit values gives you an idea of, e.g., whether or not an estimator is biased.

About

No description, website, or topics provided.

Resources

Stars

Watchers

Forks

Releases

No releases published

Packages

No packages published

Languages