NIFTY - Numerical Information Field Theory - a versatile Python library for signal inference
arXiv:1301.4499 · doi:10.1051/0004-6361/201321236
Abstract
NIFTY, "Numerical Information Field Theory", is a software package designed to enable the development of signal inference algorithms that operate regardless of the underlying spatial grid and its resolution. Its object-oriented framework is written in Python, although it accesses libraries written in Cython, C++, and C for efficiency. NIFTY offers a toolkit that abstracts discretized representations of continuous spaces, fields in these spaces, and operators acting on fields into classes. Thereby, the correct normalization of operations on fields is taken care of automatically without concerning the user. This allows for an abstract formulation and programming of inference algorithms, including those derived within information field theory. Thus, NIFTY permits its user to rapidly prototype algorithms in 1D, and then apply the developed code in higher-dimensional settings of real world problems. The set of spaces on which NIFTY operates comprises point sets, n-dimensional regular grids, spherical spaces, their harmonic counterparts, and product spaces constructed as combinations of those. The functionality and diversity of the package is demonstrated by a Wiener filter code example that successfully runs without modification regardless of the space on which the inference problem is defined.
9 pages, 3 tables, 4 figures, accepted by Astronomy & Astrophysics; refereed version, 1 figure added, results unchanged
References in corpus (3)
Cited by in corpus (53)
- Estimating extragalactic Faraday rotation
- On the non-Poissonian repetition pattern of FRB121102
- Design and Sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G)
- IMAGINE: A comprehensive view of the interstellar medium, Galactic magnetic fields and cosmic rays
- The Denoised, Deconvolved, and Decomposed Fermi -ray sky - An application of the DPO algorithm
- RESOLVE: A new algorithm for aperture synthesis imaging of extended emission in radio astronomy
- The Galactic Faraday depth sky revisited
- Variability of Red Supergiants in M31 from the Palomar Transient Factory
- Information theory for fields
- DPO - Denoising, Deconvolving, and Decomposing Photon Observations
- Using rotation measure grids to detect cosmological magnetic fields -- a Bayesian approach
- Matrix-free Large Scale Bayesian inference in cosmology
- High accuracy wide field imaging method in radio interferometry
- Re-Envisioning Numerical Information Field Theory (NIFTy.re): A Library for Gaussian Processes and Variational Inference
- Bayesian weak lensing tomography: Reconstructing the 3D large-scale distribution of matter with a lognormal prior
- A new approach to multi-frequency synthesis in radio interferometry
- Detection of open cluster rotation fields from Gaia EDR3 proper motions
- Spatially Coherent 3D Distributions of HI and CO in the Milky Way
- Physics-informed Information Field Theory for Modeling Physical Systems with Uncertainty Quantification
- Bayesian inference of three-dimensional gas maps: II. Galactic HI
- Generic inference of inflation models by non-Gaussianity and primordial power spectrum reconstruction
- Cosmic expansion history from SNe Ia data via information field theory -- the charm code
- Log-transforming the matter power spectrum
- Variability of massive stars in M31 from the Palomar Transient Factory
- Tomography of the Galactic free electron density with the Square Kilometer Array
- Exploiting the diversity of modeling methods to probe systematic biases in strong lensing analyses
- Denoising, deconvolving and decomposing multi-domain photon observations- The D4PO algorithm
- Information Field Theory and Artificial Intelligence
- Causal, Bayesian, & Non-parametric Modeling of the SARS-CoV-2 Viral Load Distribution vs. Patient's Age
- Noisy independent component analysis of auto-correlated components
- Multi-Component Imaging of the Fermi Gamma-ray Sky in the Spatio-spectral Domain
- Stochastic determination of matrix determinants
- fast-resolve: Fast Bayesian Radio Interferometric Imaging
- El Gordo needs El Anzuelo: Probing the structure of cluster members with multi-band extended arcs in JWST data
- Dynamic system classifier
- Radio Imaging With Information Field Theory
- Fast and precise way to calculate the posterior for the local non-Gaussianity parameter from cosmic microwave background observations
- Local dark matter density from Gaia DR3 K-dwarfs using Gaussian processes
- Enhancing CMB map reconstruction and power spectrum estimation with convolutional neural networks
- Improving self-calibration
- D2O - a distributed data object for parallel high-performance computing in Python
- Fast-Cadence High-Contrast Imaging with Information Field Theory
- Signal inference with unknown response: Calibration-uncertainty renormalized estimator
- Sharpening up Galactic all-sky maps with complementary data - A machine learning approach
- All-sky reconstruction of the primordial scalar potential from WMAP temperature data
- Exploring the MeV Sky with a Combined Coded Mask and Compton Telescope: The Galactic Explorer with a Coded Aperture Mask Compton Telescope (GECCO)
- Non-parametric Bayesian reconstruction of Galactic magnetic fields using Information Field Theory: The inclusion of line-of-sight information in ultra-high energy cosmic ray backtracking
- Classification and Uncertainty Quantification of Corrupted Data using Semi-Supervised Autoencoders
- Enhancing Compton telescope imaging with maximum a posteriori estimation: a modified Richardson-Lucy algorithm for the Compton Spectrometer and Imager
- Bayesian Multi-wavelength Imaging of the LMC SN1987A with SRG/eROSITA
- Latent-space Field Tension for Astrophysical Component Detection An application to X-ray imaging
- The influence of the 3D Galactic gas structure on cosmic-ray transport and -ray emission
- A Bayesian Method for Air-Shower Reconstruction using Information Field Theory