fvGP#
- class fvgp.fvGP(x_data, y_data, init_hyperparameters=None, noise_variances=None, compute_device='cpu', kernel_function=None, kernel_function_grad=None, noise_function=None, noise_function_grad=None, prior_mean_function=None, prior_mean_function_grad=None, gp2Scale=False, dask_client=None, gp2Scale_batch_size=10000, linalg_mode=None, ram_economy=False, args=None)[source]#
This class provides all the tools for a multi-task Gaussian Process (GP). After initialization, this class provides all the methods described for the
fvgp.GPclass, including full HPC support via thehgdlpackage and large-scale sparse GPs viagp2Scale.V … number of input points
Di… input space dimensionality
No… number of outputs
N … arbitrary integers (N1, N2,…)
The main logic of fvGP is that any multi-task GP is just a single-task GP over a Cartesian product space of input and output space, as long as the kernel is flexible enough, so prepare to work on your kernel. This is the best way to give the user optimal control and power. At various instances, for example prior-mean function, noise function, and kernel function definitions, you will see that the input
xis defined over this combined space. For example, if your input space is a Euclidean 2d space and your output is labelled [0,1], the input to the mean, kernel, and noise functions might bex =
[[0.2, 0.3,0],[0.9,0.6,0],
[0.2, 0.3,1],[0.9,0.6,1]]
This has to be understood and taken into account when customizing fvGP for multi-task use. The examples will provide deeper insights.
- Parameters:
x_data (np.ndarray | list) – The input point positions. Shape (V x Di), where Di is the
fvgp.fvGP.input_set_dim. For multi-task GPs, the index set dimension = input space dimension + 1. If dealing with non-Euclidean inputs x_data should be a list, not a numpy array. In this case, both the index set and the input space dim are set to 1.y_data (np.ndarray) – The values of the data points. Shape (V,No). It is possible that not every entry in
x_datahas all corresponding tasks available. In that casey_datamay have np.nan as the corresponding entries.init_hyperparameters (np.ndarray, optional) – Vector of hyperparameters used to initiate the GP. The default is an array of ones with the right length for the anisotropic Matern kernel with automatic relevance determination (ARD). The task direction is simply considered a separate dimension. If
gp2Scaleis enabled, the default kernel changes to the anisotropic Wendland kernel. The full hyperparameter vector is passed to the kernel, mean, and noise callables, but the index ranges used by each callable are disjoint and user-defined. Each callable must only read the indices reserved for it. The gradient computation relies on this: when a hyperparameter index belongs to the mean function its kernel derivative is assumed zero, and vice versa.noise_variances (np.ndarray, optional) – A numpy array defining the uncertainties/noise in the
y_datain form of a point-wise variance. Shape (V, No). Ify_datahas np.nan entries, the correspondingnoise_varianceshave to be np.nan. Note: if no noise_variances are provided here, the noise_function callable will be used; if the callable is not provided, the noise variances will be set toabs(np.mean(y_data)) / 100.0. If noise covariances are required (correlated noise), make use of thenoise_function. Only provide a noise function ORnoise_variances, not both.compute_device (str, optional) – One of
cpuorgpu, determines how linear algebra computations are executed. The default iscpu. Forgpu, pytorch or cupy has to be installed manually. For advanced options seeargs. Ifgp2Scaleis enabled but no kernel is provided, the choice of thecompute_devicewill be particularly important. In that case, the default Wendland kernel will be computed on the cpu or the gpu which will significantly change the compute time depending on the compute architecture.kernel_function (Callable, optional) – A symmetric positive definite covariance function (a kernel) that calculates the covariance between data points. It is a function of the form k(x1,x2,hyperparameters, [args]).
argsis optional and is used to makefvgp.GP.argsavailable. The inputx1is a N1 x Di+1 array of positions,x2is a N2 x Di+1 array of positions, the hyperparameters argument is a 1d array of length N depending on how many hyperparameters are initialized. The default is a stationary anisotropic kernel (fvgp.GP.default_kernel()) which performs automatic relevance determination (ARD). The task direction is simply considered an additional dimension. This kernel should only be used for tests and in the simplest of cases. The output is a matrix, an N1 x N2 numpy array. This callable receives the full hyperparameter vector but must only use the indices reserved for the kernel (disjoint from mean and noise indices).kernel_function_grad (Callable, optional) – A function that calculates the derivative of the
kernel_functionwith respect to the hyperparameters. If provided, it will be used for local training (optimization) and can speed up the calculations. It accepts as inputx1(a N1 x Di + 1 array of positions),x2(a N2 x Di + 1 array of positions) andhyperparameters(a 1d array of length Di+2 for the default kernel). The default is an analytical gradient for the default kernel or a finite difference calculation otherwise. Ifram_economyis True, the function’s input is x1, x2, hyperparameters (numpy array), and a direction (int). The output is a numpy array of shape (len(hps) x N). Ifram_economyisFalse, the function’s input is x1, x2, and hyperparameters. The output is a numpy array of shape (len(hyperparameters) x N1 x N2). Seeram_economy.prior_mean_function (Callable, optional) – A function f(x, hyperparameters, [args]) that evaluates the prior mean at a set of input position. It accepts as input an array of positions (of shape N1 x Di+1) and hyperparameters (a 1d array of length Di+2 for the default kernel). Optionally, the third argument
argscan be defined. The return value is a 1d array of length N1. If None is provided,fvgp.GP._default_mean_function()is used, which is the average of they_data. This callable receives the full hyperparameter vector but must only use the indices reserved for the mean function (disjoint from kernel and noise indices).prior_mean_function_grad (Callable, optional) – A function that evaluates the gradient of the
prior_mean_functionat a set of input positions with respect to the hyperparameters. It accepts as input an array of positions (of size N1 x Di+1) and hyperparameters (a 1d array of length Di+2 for the default kernel). The return value is a 2d array of shape (len(hyperparameters) x N1). If None is provided, either zeros are returned since the default mean function does not depend on hyperparameters, or a finite-difference approximation is used ifprior_mean_functionis provided.noise_function (Callable, optional) – The noise function is a callable f(x,hyperparameters, [args]) that returns a vector (1d np.ndarray) of len(x), a matrix of shape (length(x),length(x)) or a sparse matrix of the same shape. The third argument
argsis optional. The inputxis a numpy array of shape (N x Di+1). The hyperparameter array is the same that is communicated to mean and kernel functions. Only provide a noise function OR a noise variance vector, not both. This callable receives the full hyperparameter vector but must only use the indices reserved for the noise function (disjoint from kernel and mean indices).noise_function_grad (Callable, optional) – A function that evaluates the gradient of the
noise_functionat an input position with respect to the hyperparameters. It accepts as input an array of positions (of size N x Di+1) and hyperparameters (a 1d array of length Di+1 for the default kernel). The return value is a 2d np.ndarray of shape (len(hyperparameters) x N) or a 3d np.ndarray of shape (len(hyperparameters) x N x N). If None is provided, either zeros are returned since the default noise function does not depend on hyperparameters, or, ifnoise_functionis provided but no noise function gradient, a finite-difference approximation will be used. The same rules regardingram_economyas for the kernel definition apply here. That means the function will have an additionaldirectionparameter.gp2Scale (bool, optional) – Turns on gp2Scale. This will distribute the covariance computations across multiple workers. This is an advanced feature for HPC GPs up to 10 million data points. If gp2Scale is used, the default kernel is an anisotropic Wendland kernel which is compactly supported. There are a few things to consider (read on); this is an advanced option. If no kernel is provided, the
compute_deviceoption should be revisited. The default kernel will use the specified device to compute covariances. The default is False.gp2Scale_batch_size (int, optional) – Matrix batch size for distributed computing in gp2Scale. The default is 10000.
dask_client (dask.distributed.Client, optional) – A dask client for gp2Scale, asynchronous training,a nd certain linear algebra operations. On HPC architecture, this client is provided by the job script. Please have a look at the examples. A local client is used as the default.
linalg_mode (str, optional) –
Controls the linear-algebra backend used to solve (K+V)x=b and compute log|K+V|. The default is
None, which selects"Chol"for standard GPs and automatically picks the best sparse mode for gp2Scale GPs.Recommended for standard (non-gp2Scale) GPs:
"Chol"(default) — Cholesky factorization; numerically stable and memory-efficient."CholInv"— Cholesky factorization, then explicitly stores the inverse; speeds up posterior covariance evaluation 3–10×. Avoid for datasets larger than ~5 000 points due to memory and numerical cost. Training always uses the Cholesky factor for stability."Inv"— computes and stores the explicit inverse directly (no Cholesky). Only suitable for very small datasets where posterior covariance is computed many times.
Specialized for gp2Scale (sparse covariance matrices):
"sparseLU"— sparse LU factorization; good default for sparse systems up to ~50 000 points."sparseCG"— sparse conjugate-gradient iterative solver."sparseMINRES"— sparse MINRES iterative solver."sparseSolve"— direct sparse solve via scipy."sparseCGpre"— preconditioned conjugate-gradient. The preconditioner type is selected byargs["sparse_preconditioner_type"](default"ilu"; also"ic"/"incomplete_cholesky","block_jacobi","schwarz"/"additive_schwarz", or"amg"(requires pyamg))."sparseMINRESpre"— preconditioned MINRES; same preconditioner choices."sparseCGpre_<type>"/"sparseMINRESpre_<type>"— shortcut that setsargs["sparse_preconditioner_type"]to<type>(e.g."sparseCGpre_amg").
Custom solver (any GP):
Pass an iterable of three callables
[f_factor, f_solve, f_logdet]:f_factor(K)— receives the covariance matrix and returns a factorization object (or the matrix itself if no factorization is needed).f_solve(obj, b)— solves the linear system and returns the solution vector.f_logdet(obj)— returns the log-determinant as a scalar.
ram_economy (bool, optional) – Only of interest if the gradient and/or Hessian of the log marginal likelihood is/are used for the training. If True, components of the derivative of the log marginal likelihood are calculated sequentially, leading to a slow-down but much less RAM usage. If the derivative of the kernel (and noise function) with respect to the hyperparameters (kernel_function_grad) is going to be provided, it has to be tailored: for
ram_economy=Trueit should be of the form f(x, hyperparameters, direction) and return a 2d numpy array of shape len(x1) x len(x2). Ifram_economy=False, the function should be of the form f(x, hyperparameters) and return a numpy array of shape H x len(x1) x len(x2), where H is the number of hyperparameters. CAUTION: This array will be stored and is very large.args (dict, optional) –
Advanced options. Recognized keys are:
Stochastic-Lanczos logdet (sparse modes):
”random_logdet_lanczos_degree” : int; default = 20
”random_logdet_error_rtol” : float; default = 0.01
”random_logdet_verbose” : True/False; default = False
”random_logdet_print_info” : True/False; default = False
”random_logdet_lanczos_compute_device” : str; default = “cpu”/”gpu”
Sparse iterative solver tolerances and iteration limits:
”sparse_cg_tol” : float; default = 1e-5
”sparse_minres_tol” : float; default = 1e-5
”sparse_cg_maxiter” : int; default = None (use scipy default)
”sparse_minres_maxiter” : int; default = None (use scipy default)
”sparse_krylov_maxiter” : int; default = None (applies to both if the solver-specific key is not set)
”sparse_block_krylov” : True/False; default = False — use a block CG variant when there are multiple RHS columns
”sparse_krylov_mode” : “single”/”block”; equivalent toggle
”sparse_krylov_block_size” : int — RHS block size for block CG
Iterative-solver acceleration (
sparseCG/sparseMINRESand the*prevariants):”sparse_krylov_warm_start” : True/False; default = False — feed the previous training iteration’s
KVinvYasx0to the next solve”sparse_preconditioner_type” : str; default = “ilu”. One of “ilu”, “ic”/”ichol”/”incomplete_cholesky”, “block_jacobi”, “schwarz”/ “additive_schwarz”, “amg” (requires pyamg)
”sparse_preconditioner_refresh_interval” : int; default = 1 — reuse the cached preconditioner for up to N consecutive solves before rebuilding.
set_KValways force-refreshes.”sparse_preconditioner_block_size” : int — block size for block_jacobi and additive_schwarz partitions
”sparse_preconditioner_schwarz_overlap” : int — overlap layers for additive Schwarz
”sparse_preconditioner_drop_tol” / “sparse_preconditioner_fill_factor” — forwarded to scipy
spilufor “ilu””sparse_preconditioner_amg_*” — forwarded to pyamg (
max_levels,max_coarse,strength,cycle, etc.)”sparse_preconditioner_shift” / “_growth” / “_attempts” — diagonal shift retry knobs for “ic” / “block_jacobi” / “additive_schwarz” when a local Cholesky encounters a non-PD block
Cholesky compute-device routing:
”Chol_factor_compute_device” : str; default = “cpu”/”gpu”
”update_Chol_factor_compute_device”: str; default = “cpu”/”gpu”
”Chol_solve_compute_device” : str; default = “cpu”/”gpu”
”Chol_logdet_compute_device” : str; default = “cpu”/”gpu”
GPU backend:
”GPU_engine” : “torch”/”cupy”; default = first available
”GPU_device” : str; e.g. “cuda:1” or “mps”
”GPU_device_index” : int — explicit CUDA device index
All other keys will be stored and are available as part of the object instance and in kernel, mean, and noise functions.
- y_data#
Datapoint values.
- Type:
np.ndarray
- noise_variances#
Datapoint observation variances.
- Type:
np.ndarray
- hyperparameters#
Current hyperparameters in use.
- Type:
np.ndarray
- K#
Current prior covariance matrix of the GP.
- Type:
np.ndarray
- m#
Current prior mean vector.
- Type:
np.ndarray
- V#
the noise covariance matrix or a vector.
- Type:
np.ndarray
This class inherits all capabilities from
fvgp.GP. Check there for a full list of capabilities. Here are the most important.Base-GP Methods:
fvgp.GP.update_hyperparameters()Posterior Evaluations:
fvgp.GP.posterior_covariance()fvgp.GP.posterior_covariance_grad()fvgp.GP.gp_mutual_information()fvgp.GP.gp_total_correlation()fvgp.GP.gp_relative_information_entropy()fvgp.GP.gp_relative_information_entropy_set()fvgp.GP.posterior_probability()Validation Methods:
fvgp.GP.test_log_likelihood_gradient()- property fvgp_x_data#
Multi-task input data including the output-index column, shape (N, D+1).
- property fvgp_y_data#
Observed values in the multi-task (output-index-augmented) space, shape (N,).
- property fvgp_noise_variances#
Point-wise noise variances in the multi-task space, shape (N,), or None.
- update_gp_data(x_new, y_new, noise_variances_new=None, append=True, rank_n_update=None)[source]#
This function updates the data in the gp object instance. The data will only be overwritten if
append=False, otherwise the data will be appended. This is a change from earlier versions. Now, the default is not to overwrite the existing data.- Parameters:
x_new (np.ndarray or list) – The input point positions. Shape (V x Di), where Di is the
fvgp.fvGP.input_set_dim. For multi-task GPs, the index set dimension = input space dimension + 1. If dealing with non-Euclidean inputsx_newshould be a list, not a numpy array.y_new (np.ndarray) – The values of the data points. Shape (V,No). It is possible that not every entry in
x_newhas all corresponding tasks available. In that casey_newmay contain np.nan entries.noise_variances_new (np.ndarray, optional) – A numpy array or list defining the uncertainties/noise in the
y_datain form of a point-wise variance. Shape (V, No). Ify_datahas np.nan entries, the correspondingnoise_varianceshave to be np.nan. Note: if no noise_variances are provided here, the noise_function callable will be used; if the callable is not provided, the noise variances will be set toabs(np.mean(y_data)) / 100.0. If noise covariances are required (correlated noise), make use of thenoise_function. Only provide a noise function ORnoise_variances, not both.append (bool, optional) – Indication whether to append to or overwrite the existing dataset. Default = True. In the default case, data will be appended.
rank_n_update (bool, optional) – Indicates whether the GP marginal likelihood should be rank-n updated or recomputed. The default is
rank_n_update=append, meaning if data is only appended, the rank_n_update will be performed.