Analyze This! A Cosmological Constraint Package for CMBEASY
arXiv:astro-ph/0311311 · doi:10.1088/1475-7516/2004/09/003
Abstract
We introduce a Markov Chain Monte Carlo simulation and data analysis package that extends the CMBEASY software. We have taken special care in implementing an adaptive step algorithm for the Markov Chain Monte Carlo in order to improve convergence. Data analysis routines are provided which allow to test models of the Universe against measurements of the cosmic microwave background, supernovae Ia and large scale structure. We present constraints on cosmological parameters derived from these measurements for a CDM cosmology and discuss the impact of the different observational data sets on the parameters. The package is publicly available as part of the CMBEASY software at www.cmbeasy.org.
Published version, JCAP style, 16 pages, 7 figures. The software is available at http://www.cmbeasy.org
References in corpus (23)
- Efficient Computation of CMB anisotropies in closed FRW models
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Cosmological parameters from SDSS and WMAP
- Cosmological parameters from CMB and other data: a Monte-Carlo approach
- A Line of Sight Approach to Cosmic Microwave Background Anisotropies
- The 3D power spectrum of galaxies from the SDSS
- Cosmological Results from High-z Supernovae
- Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum
- The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe
- A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey
- The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology
- 23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at z>0.7
- High Resolution Observations of the CMB Power Spectrum with ACBAR
- Cosmic Microwave Background and Supernova Constraints on Quintessence: Concordance Regions and Target Models
- High sensitivity measurements of the CMB power spectrum with the extended Very Small Array
- Efficient Cosmological Parameter Estimation from Microwave Background Anisotropies
- II: Bayesian Methods for Cosmological Parameter Estimation from Cosmic Microwave Background Measurements
- The Age of the Universe and the Cosmological Constant Determined from Cosmic Microwave Background Anisotropy Measurements
- Gamma-Ray Bursts via the Neutrino Emission from Heated Neutron Stars
- An improved Markov-chain Monte Carlo sampler for the estimation of cosmological parameters from CMB data
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