Eyes Wide Open - Optimising Cosmological Surveys in a Crowded Market
arXiv:astro-ph/0407201 · doi:10.1103/PhysRevD.71.083517
Abstract
Optimising the major next-generation cosmological surveys (such as {\em SNAP, KAOS etc...}) is a key problem given our ignorance of the physics underlying cosmic acceleration and the plethora of surveys planned. We propose a Bayesian design framework which (1) maximises the discrimination power of a survey without assuming any underlying dark energy model, (2) finds the best niche survey geometry given current data and future competing experiments, (3) maximises the cross-section for serendipitous discoveries and (4) can be adapted to answer specific questions (such as `is dark energy dynamical?'). Integrated Parameter Space Optimisation (IPSO) is a design framework that integrates projected parameter errors over an entire dark energy parameter space and then extremises a figure of merit (such as Shannon entropy gain which we show is stable to off-diagonal covariance matrix perturbations) as a function of survey parameters using analytical, grid or MCMC techniques. We discuss examples where the optimisation can be performed analytically. IPSO is thus a general, model-independent and scalable framework that allows us to appropriately use prior information to design the best possible surveys.
15 pages, 6 colour figures. Significantly more discussion and illustrative examples
References in corpus (3)
Cited by in corpus (28)
- Observational Probes of Cosmic Acceleration
- Cosmology and Fundamental Physics with the Euclid Satellite
- Cosmology and fundamental physics with the Euclid satellite
- Constraining dark energy with cross-correlated CMB and Large Scale Structure data
- Present and future evidence for evolving dark energy
- Universal fitting formulae for baryon oscillation surveys
- Investigating dark energy experiments with principal components
- Dynamical behavior of generic quintessence potentials: constraints on key dark energy observables
- How flat can you get? A model comparison perspective on the curvature of the Universe
- Model selection as a science driver for dark energy surveys
- Forecasting the Bayes factor of a future observation
- A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
- Statistical methods for cosmological parameter selection and estimation
- Deep Learning improves identification of Radio Frequency Interference
- Optimising Baryon Acoustic Oscillation Surveys - I: Testing the concordance LCDM cosmology
- Fisher Matrix Preloaded -- Fisher4Cast
- Understanding the origin of CMB constraints on Dark Energy
- Optimizing baryon acoustic oscillation surveys II: curvature, redshifts, and external datasets
- Comparing cosmic web classifiers using information theory
- Figures of Merit for Testing Standard Models: Application to Dark Energy Experiments in Cosmology
- Model Breaking Measure for Cosmological Surveys
- Sparsely Sampling the Sky: A Bayesian Experimental Design Approach
- Designing Decisive Detections
- Optimal machine-driven acquisition of future cosmological data
- A New Approach to the Optimal Target Selection Problem
- The decisive future of inflation
- Optimizing future dark energy surveys for model selection goals
- Testing Inflationary Cosmology