Fisher Matrix Preloaded -- Fisher4Cast
arXiv:0906.0993 · doi:10.1142/S0218271811020548
Abstract
The Fisher Matrix is the backbone of modern cosmological forecasting. We describe the Fisher4Cast software: a general-purpose, easy-to-use, Fisher Matrix framework. It is open source, rigorously designed and tested and includes a Graphical User Interface (GUI) with automated LATEX file creation capability and point-and-click Fisher ellipse generation. Fisher4Cast was designed for ease of extension and, although written in Matlab, is easily portable to open-source alternatives such as Octave and Scilab. Here we use Fisher4Cast to present new 3-D and 4-D visualisations of the forecasting landscape and to investigate the effects of growth and curvature on future cosmological surveys. Early releases have been available at http://www.cosmology.org.za since May 2008 with 750 downloads in the first year. Version 2.2 is made public with this paper and includes a Quick Start guide and the code used to produce the figures in this paper, in the hope that it will be useful to the cosmology and wider scientific communities.
30 Pages, 15 figures. Minor revisions to match published version, with some additional functionality described to match the current version (2.2) of the code. Software available at http://www.cosmology.org.za. Usage, structure and flow of the software, as well as tests performed are described in the accompanying Users' Manual
References in corpus (12)
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- A 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3
- The Atacama Cosmology Telescope: Cosmological Parameters from the 2008 Power Spectra
- Distinguishing Modified Gravity from Dark Energy
- Improved forecasts for the baryon acoustic oscillations and cosmological distance scale
- Testing cosmological structure formation using redshift-space distortions
- Distance, Growth Factor, and Dark Energy Constraints from Photometric Baryon Acoustic Oscillation and Weak Lensing Measurements
- How to Distinguish Dark Energy and Modified Gravity?
- Optimising Baryon Acoustic Oscillation Surveys - I: Testing the concordance LCDM cosmology
- Extending the Gravitational Growth Framework
- Non-parametric Dark Energy Degeneracies
- Uncertainty on determining the dark energy equation of state due to the spatial curvature
Cited by in corpus (22)
- Cosmology and Fundamental Physics with the Euclid Satellite
- Cosmology and fundamental physics with the Euclid satellite
- CosmoSIS: modular cosmological parameter estimation
- DESI and other dark energy experiments in the era of neutrino mass measurements
- Future CMB tests of dark matter: ultra-light axions and massive neutrinos
- Cosmological performance of SKA HI galaxy surveys
- Breaking the spell of Gaussianity: forecasting with higher order Fisher matrices
- Probing dark energy with redshift-drift
- Probing deviations from General Relativity with the Euclid spectroscopic survey
- Exploring the sky localization and early warning capabilities of third generation gravitational wave detectors in three-detector network configurations
- Internal Robustness: systematic search for systematic bias in SN Ia data
- High Redshift Standard Candles: Predicted Cosmological Constraints
- Spatial curvature endgame: Reaching the limit of curvature determination
- Exploring degeneracies in modified gravity with weak lensing
- Photometric redshifts and intrinsic alignments: degeneracies and biases in 32pt analysis
- Describing variations of the Fisher-matrix across parameter space
- Calibrating the BAO scale using the CMB: Lifting the degeneracy between geometric and dynamic distortions using the sound horizon from the CMB
- The Physical Origin of Dark Energy Constraints from Rubin Observatory and CMB-S4 Lensing Tomography
- Probing the Anisotropy and Non-Gaussianity in the Redshift Space through the Conditional Moments of the First Derivative
- Joint Modelling of Astrophysical Systematics for Cosmology with LSST Cosmic Shear
- Partition function approach to non-Gaussian likelihoods: Formalism and expansions for weakly non-Gaussian cosmological inference
- Cosmological consequences of intrinsic alignments super-sample covariance