petitRADTRANS.retrieval.psis
Pareto smoothed importance sampling (PSIS)
This module implements Pareto smoothed importance sampling (PSIS) and PSIS leave-one-out (LOO) cross-validation for Python (Numpy).
Included functions
- psisloo
Pareto smoothed importance sampling leave-one-out log predictive densities.
- psislw
Pareto smoothed importance sampling.
- gpdfitnew
Estimate the paramaters for the Generalized Pareto Distribution (GPD).
- gpinv
Inverse Generalised Pareto distribution function.
- sumlogs
Sum of vector where numbers are represented by their logarithms.
References
Aki Vehtari, Andrew Gelman and Jonah Gabry (2017). Practical Bayesian model evaluation using leave-one-out cross-validation and WAIC. Statistics and Computing, 27(5):1413–1432. doi:10.1007/s11222-016-9696-4. https://arxiv.org/abs/1507.04544
Aki Vehtari, Andrew Gelman and Jonah Gabry (2017). Pareto smoothed importance sampling. https://arxiv.org/abs/arXiv:1507.02646v5
Module Contents
Functions
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PSIS leave-one-out log predictive densities. |
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Pareto smoothed importance sampling (PSIS). |
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Estimate the paramaters for the Generalized Pareto Distribution (GPD) |
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Inverse Generalised Pareto distribution function. |
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Sum of vector where numbers are represented by their logarithms. |
- petitRADTRANS.retrieval.psis.psisloo(log_lik, **kwargs)
PSIS leave-one-out log predictive densities.
Computes the log predictive densities given posterior samples of the log likelihood terms \(p(y_i|\theta^s)\) in input parameter log_lik. Returns a sum of the leave-one-out log predictive densities loo, individual leave-one-out log predictive density terms loos and an estimate of Pareto tail indeces ks. The estimates are unreliable if tail index
k > 0.7(see more in the references listed in the module docstring).Additional keyword arguments are passed to the
psislw()function (see the corresponding documentation).Parameters
- log_likndarray
Array of size n x m containing n posterior samples of the log likelihood terms \(p(y_i|\theta^s)\).
Returns
- looscalar
sum of the leave-one-out log predictive densities
- loosndarray
individual leave-one-out log predictive density terms
- ksndarray
estimated Pareto tail indeces
- petitRADTRANS.retrieval.psis.psislw(lw, Reff=1.0, overwrite_lw=False)
Pareto smoothed importance sampling (PSIS).
Parameters
- lwndarray
Array of size n x m containing m sets of n log weights. It is also possible to provide one dimensional array of length n.
- Reffscalar, optional
relative MCMC efficiency
N_eff / N- overwrite_lwbool, optional
If True, the input array lw is smoothed in-place, assuming the array is F-contiguous. By default, a new array is allocated.
Returns
- lw_outndarray
smoothed log weights
- kssndarray
Pareto tail indices
- petitRADTRANS.retrieval.psis.gpdfitnew(x, sort=True, sort_in_place=False, return_quadrature=False)
Estimate the paramaters for the Generalized Pareto Distribution (GPD)
Returns empirical Bayes estimate for the parameters of the two-parameter generalized Parato distribution given the data.
Parameters
- xndarray
One dimensional data array
- sortbool or ndarray, optional
If known in advance, one can provide an array of indices that would sort the input array x. If the input array is already sorted, provide False. If True (default behaviour), the array is sorted internally.
- sort_in_placebool, optional
If sort is True and sort_in_place is True, the array is sorted in-place (False by default).
- return_quadraturebool, optional
If True, quadrature points and weight ks and w of the marginal posterior distribution of k are also calculated and returned. False by default.
Returns
- k, sigmafloat
estimated parameter values
- ks, wndarray
Quadrature points and weights of the marginal posterior distribution of k. Returned only if return_quadrature is True.
Notes
This function returns a negative of Zhang and Stephens’s k, because it is more common parameterisation.
- petitRADTRANS.retrieval.psis.gpinv(p, k, sigma)
Inverse Generalised Pareto distribution function.
- petitRADTRANS.retrieval.psis.sumlogs(x, axis=None, out=None)
Sum of vector where numbers are represented by their logarithms.
Calculates
np.log(np.sum(np.exp(x), axis=axis))in such a fashion that it works even when elements have large magnitude.