Optimal dataset combining in f_nl constraints from large scale structure in an idealised case
arXiv:0808.0044 · doi:10.1088/1475-7516/2009/03/004
Abstract
We consider the problem of optimal weighting of tracers of structure for the purpose of constraining the non-Gaussianity parameter f_NL. We work within the Fisher matrix formalism expanded around fiducial model with f_NL=0 and make several simplifying assumptions. By slicing a general sample into infinitely many samples with different biases, we derive the analytic expression for the relevant Fisher matrix element. We next consider weighting schemes that construct two effective samples from a single sample of tracers with a continuously varying bias. We show that a particularly simple ansatz for weighting functions can recover all information about f_NL in the initial sample that is recoverable using a given bias observable and that simple division into two equal samples is considerably suboptimal when sampling of modes is good, but only marginally suboptimal in the limit where Poisson errors dominate.
6 pages, 5 figures; v2: comment on weighting for PS determination, fixed a couple of typos; v3: revised, matches version accepted by JCAP
References in corpus (24)
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Large scale bias and the peak background split
- Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
- Acoustic Signatures in the Primary Microwave Background Bispectrum
- Power Spectrum Analysis of Three-Dimensional Redshift Surveys
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- The Three--Point Correlation Function of the Cosmic Microwave Background in Inflationary Models
- Constraints on local primordial non-Gaussianity from large scale structure
- How to measure CMB power spectra without losing information
- The effect of primordial non-Gaussianity on halo bias
- The halo mass function from the dark ages through the present day
- Large-scale structure, the cosmic microwave background, and primordial non-gaussianity
- Measuring primordial non-gaussianity without cosmic variance
- Detection of primordial non-Gaussianity (fNL) in the WMAP 3-year data at above 99.5% confidence
- Scale-dependent bias induced by local non-Gaussianity: A comparison to N-body simulations
- Halo mass function and scale-dependent bias from N-body simulations with non-Gaussian initial conditions
- Primordial non-gaussianity, statistics of collapsed objects, and the Integrated Sachs-Wolfe effect
- Primordial non-Gaussianity: large-scale structure signature in the perturbative bias model
- Limits on f_NL parameters from WMAP 3yr data
- Limits on Primordial Non-Gaussianity from Minkowski Functionals of the WMAP Temperature Anisotropies
- SDSS Galaxy Clustering: Luminosity & Colour Dependence and Stochasticity
- Fourier analysis of luminosity-dependent galaxy clustering
- Halo stochasticity in global clustering analysis
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- Scale-dependent bias induced by local non-Gaussianity: A comparison to N-body simulations
- Minimizing the stochasticity of halos in large-scale structure surveys
- Constraining Running Non-Gaussianity
- Constraints on primordial non-Gaussianity from 800,000 photometric quasars
- Signature of primordial non-Gaussianity of phi^3-type in the mass function and bias of dark matter haloes
- Optimal Constraints on Local Primordial Non-Gaussianity from the Two-Point Statistics of Large-Scale Structure
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- 1-loop Perturbative Corrections to the Matter and Galaxy Bispectrum with non-Gaussian Initial Conditions
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- Covariance of cross-correlations: towards efficient measures for large-scale structure
- Primordial non-Gaussianity in the large scale structure of the Universe
- Cosmological Parameters Degeneracies and Non-Gaussian Halo Bias
- Prospects for constraining the shape of non-Gaussianity with the scale-dependent bias
- The Halo Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
- The Hunt for Primordial Interactions in the Large Scale Structures of the Universe
- Testing the Running of non-Gaussianity through the CMB mu-distortion and the Halo Bias
- Fourier analysis of multi-tracer cosmological surveys
- Reducing sample variance: halo biasing, non-linearity and stochasticity
- The Matter Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
- Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias
- The initial shear field in models with primordial local non-Gaussianity and implications for halo and void abundances
- Constraining Scale-Dependent Non-Gaussianity with Future Large-Scale Structure and the CMB
- Taming assembly bias for primordial non-Gaussianity
- The nonlinear probability distribution function in models with local primordial non-Gaussianity
- The Multi-Tracer Optimal Estimator applied to VIPERS
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- The nonlinear redshift space probability distribution function in models with local primordial non-Gaussianity
- The HalfDome Multi-Survey Cosmological Simulations: N-body Simulations
- Constraints on primordial non-Gaussianity using multitracer technique for skew spectrum
- Quijote PNG: The information content of the halo power spectrum and bispectrum