cosmonet: fast cosmological parameter estimation in non-flat models using neural networks
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July 2008 |
Fast cosmological parameter estimation using neural networks
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March 2007 |
The 4 YearCOBENormalization and Large‐Scale Structure
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May 1997 |
Critical look at cosmological perturbation theory techniques
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August 2009 |
Memory of initial conditions in gravitational clustering
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March 2006 |
Bayesian Prediction of Deterministic Functions, with Applications to the Design and Analysis of Computer Experiments
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December 1991 |
Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology
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January 2008 |
Pico: Parameters for the Impatient Cosmologist
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January 2007 |
Power spectra to 1 per cent accuracy between dynamical dark energy cosmologies★: Power spectra to 1 per cent accuracy
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August 2007 |
Cosmic calibration: Constraints from the matter power spectrum and the cosmic microwave background
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October 2007 |
Reconstructing the primordial spectrum of fluctuations of the universe from the observed nonlinear clustering of galaxies
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June 1991 |
Cosmic Calibration
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July 2006 |
Computer Model Calibration Using High-Dimensional Output
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June 2008 |
Anisotropies in the cosmic microwave background: an analytic approach
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May 1995 |
The Damping Tail of Cosmic Microwave Background Anisotropies
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April 1997 |
Calibrating the nonlinear matter power spectrum: Requirements for future weak lensing surveys
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May 2005 |
Fast cosmological parameter estimation from microwave background temperature and polarization power spectra
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July 2004 |
The Influence of Baryons on the Clustering of Matter and Weak-Lensing Surveys
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March 2006 |
Rapid Calculation of Theoretical Cosmic Microwave Background Angular Power Spectra
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October 2002 |
Dark-energy constraints and correlations with systematics from CFHTLS weak lensing, SNLS supernovae Ia and WMAP5
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March 2009 |
FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION
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February 2009 |
Improved Cosmological Constraints from New, Old, and Combined Supernova Data Sets
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October 2008 |
Optimal orthogonal-array-based latin hypercubes
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June 2003 |
Going nonlinear with dark energy cosmologies
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September 2005 |
Resumming cosmological perturbations via the Lagrangian picture: One-loop results in real space and in redshift space
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March 2008 |
A Comparison of Three Methods for Selecting Values of Input Variables in the Analysis of Output from a Computer Code
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May 1979 |
Exploratory designs for computational experiments
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February 1995 |
Reconstructing the linear power spectrum of cosmological mass fluctuations
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April 1994 |
Non-linear evolution of cosmological power spectra
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June 1996 |
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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June 1999 |
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
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September 1998 |
Effects of Baryons and Dissipation on the Matter Power Spectrum
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January 2008 |
Design and Analysis of Computer Experiments
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November 1989 |
The Design and Analysis of Computer Experiments
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Simulations and cosmological inference: A statistical model for power spectra means and covariances
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September 2008 |
Maximum entropy sampling
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January 1987 |
Stable clustering, the halo model and non-linear cosmological power spectra
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June 2003 |
Orthogonal Array-Based Latin Hypercubes
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December 1993 |
Current Cosmological Constraints from a 10 Parameter Cosmic Microwave Background Analysis
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November 2000 |
Cosmological constraints from the SDSS luminous red galaxies
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December 2006 |
CHANDRA CLUSTER COSMOLOGY PROJECT III: COSMOLOGICAL PARAMETER CONSTRAINTS
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February 2009 |
Constraining Amplitude and Slope of the Mass Fluctuation Spectrum Using a Cluster Baryon Mass Function
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February 2004 |
ACED: Algorithms for the Construction of Experimental Designs
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May 1985 |
Baryons and weak lensing power spectra
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November 2004 |
Cosmological science enabled by Planck
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December 2006 |
Simulations of weak gravitational lensing
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October 2004 |
Orthogonal Column Latin Hypercubes and Their Application in Computer Experiments
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January 1998 |
Effect of Hot Baryons on the Weak-Lensing Shear Power Spectrum
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October 2004 |