CMB Anisotropy Constraints on Open and Flat-Lambda CDM Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data

Abstract

We use combinations of ten small-scale cosmic microwave background anisotropy data sets from the UCSB South Pole 1994, ARGO, MAX 4 and 5, White Dish and SuZIE experiments to constrain cosmogonies. We consider open and spatially-flat-Lambda cold dark matter cosmogonies. Marginalizing over all parameters but ${\Omega }_0$, the combined data favors an Omega_0 simeq 1 for both open and flat-Lambda models. Excluding the smallest angular scale SuZIE data, an Omega_0 simeq 0.3 (1.0) open (flat-Lambda) model is favored. Considering only multi-frequency data with error bars consistent with sample variance and noise considerations, an Omega_0 simeq 0.1 (1) open (flat-Lambda) model is favored. For both open and flat-$\Lambda$ models, after marginalizing over all the other parameters, a lower Omega_B h^2 (sim 0.005) or younger (t_0 sim 10 Gyr) universe is favored. However, the data do not rule out other values of Omega_0 in the flat-Lambda model and other values of Omega_B h^2 in both models. (abriged)

31 pages, 8 figures, uses aaspp4.sty, accepted by ApJ

References in corpus (48)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Cosmological Imprint of an Energy Component with General Equation of State
• The Cosmic Baryon Budget
• Structure formation with a self-tuning scalar field
• Estimating the Power Spectrum of the Cosmic Microwave Background
• The Deuterium Abundance Towards Q1937-1009
• How to determine an effective potential for a variable cosmological term
• Ages of Globular Clusters from Hipparcos Parallaxes of Local Subdwarfs
• The Age Of Globular Clusters In Light Of Hipparcos: Resolving the Age Problem?
• The Luminosity-Temperature Relation at z=0.4 for Clusters of galaxies
• The Intracluster Gas Fraction in X-ray Clusters : Constraints on the Clustered Mass Density
• Constraining Omega with Cluster Evolution
• Luminosity Evolution of Early-type Galaxies to z=0.83: Constraints on Formation Epoch and Omega
• Limits on Cosmological Models From Radio-Selected Gravitational Lenses
• Younger and brighter - New distances to globular clusters based on Hipparcos parallax measurements of local subdwarfs
• Measuring Omega_0 using cluster evolution
• The ROSAT Brightest Cluster Sample (BCS): The cluster X-ray luminosity function within z=0.3
• A wide-field K-band survey. The luminosity function of galaxies
• Galactic microwave emission at degree angular scales
• A Very Hot, High Redshift Cluster of Galaxies: More Trouble for Omega_0 = 1
• Redshift Evolution of Galaxy Cluster Densities
• The Norris Survey of the Corona Borealis Supercluster: III. Structure and Mass of the Supercluster
• Perturbation evolution in cosmologies with a decaying cosmological constant
• Constraints from High Redshift Supernovae upon Scalar Field Cosmologies
• What Can Cosmic Microwave Background Observations Already Say About Cosmological Parameters in Open and Critical-Density Cold Dark Matter Models?
• Mapping the CMB III: combined analysis of QMAP flights
• On the mass distribution in the Shapley Supercluster inferred from X-ray observations
• An estimate of H_0 from Keck spectroscopy of the gravitational lens system 0957+561
• Large-scale structure in COBE-normalized cold dark matter cosmogonies
• A Massive Cluster of Galaxies at z = 0.996
• Constraining cosmological models with cluster power spectra
• An Upper Limit to Arcminute Scale Anisotropy in the Cosmic Microwave Background Radiation at 142 GHz
• A Group of Red, Ly-alpha Emitting, High Redshift Galaxies
• CMB Anisotropy Correlation Function and Topology from Simulated Maps for MAP
• On the Evolution of the Temperature-Viral Mass Relation for Clusters of Galaxies
• The Norris Survey of the Corona Borealis Supercluster: II. Galaxy Evolution with Redshift and Environment
• Globular Cluster Calibration of the Peak Brightness of the Type Ia Supernova 1992A and the Value of Ho
• Peculiar Velocities of Clusters in CDM Models
• Using SuZIE arcminute-scale CMB anisotropy data to probe open and flat-ΛCDM cosmogonies
• The D/H ratio at z = 3.57 toward Q 1937-1009
• MAX 4 and MAX 5 CMB anisotropy measurement constraints on open and flat-Lambda CDM cosmogonies
• New Cosmological Structures on Medium Angular Scales Detected with the Tenerife Experiments
• The IAC-Bartol Cosmic Microwave Background Anisotropy Experiment: Results of the 1994 Campaign
• ARGO CMB Anisotropy Measurement Constraints on Open and Flat-Lambda CDM Cosmogonies
• Australia Telescope Search for Cosmic Microwave Background Anisotropy
• Using White Dish CMB Anisotropy Data to Probe Open and Flat-Lambda CDM Cosmogonies
• Spontaneous Decay of the Effective Cosmological Constant

Cited by in corpus (41)

• The Cosmological Constant and Dark Energy
• The Cosmological Constant
• Median Statistics, H_0, and the Accelerating Universe
• Solving the Coincidence Problem: Tracking Oscillating Energy
• SUSY QCD and Quintessence
• Dark Energy and the CMB
• Supernovae Ia Constraints on a Time-Variable Cosmological "Constant"
• Planck 2015 constraints on the non-flat $\Lambda$CDM inflation model
• Binned Cosmic Microwave Background Anisotropy Power Spectra: Peak Location
• Binned Hubble parameter measurements and the cosmological deceleration-acceleration transition
• Characterizing the Peak in the CMB Angular Power Spectrum
• Using SPTpol, Planck 2015, and non-CMB data to constrain tilted spatially-flat and untilted non-flat $\Lambda$CDM, XCDM, and $\varphi$CDM dark energy inflation cosmologies
• Hubble parameter data constraints on dark energy
• Radio Galaxy Redshift-Angular Size Data Constraints on Dark Energy
• Planck 2015 constraints on the non-flat XCDM inflation model
• Inflation in a closed universe
• Gaussianity of Degree-Scale Cosmic Microwave Background Anisotropy Observations
• Cosmological-Model-Parameter Determination from Satellite-Acquired Type Ia and IIP Supernova Data
• The QMAP and MAT/TOCO Experiments for Measuring Anisotropy in the Cosmic Microwave Background
• Median Statistics Estimate of the Distance to the Galactic Center
• Improved Treatment of Cosmic Microwave Background Fluctuations Induced by a Late-decaying Massive Neutrino
• Open and closed CDM isocurvature models contrasted with the CMB data
• First Results from Viper: Detection of Small-Scale Anisotropy at 40 GHZ
• Window Function for Non-Circular Beam CMB Anisotropy Experiment
• Current data are consistent with flat spatial hypersurfaces in the $\Lambda$CDM cosmological model but favor more lensing than the model predicts
• Cosmological Tests Using the Angular Size of Galaxy Clusters
• Galaxy cluster angular size data constraints on dark energy
• Non-Gaussian Error Distributions of LMC Distance Moduli Measurements
• Galactic Foregrounds in OVRO and UCSB South Pole 1994 Cosmic Microwave Background Anisotropy Data
• Effects of Foreground Contamination on the Cosmic Microwave Background Anisotropy Measured by MAP
• Non-Gaussian Error Distribution of ${}^7\mathrm{Li}$ Abundance Measurements
• Galactic Foreground Constraints from the Python V Cosmic Microwave Background Anisotropy Data
• Python I, II, and III CMB Anisotropy Measurement Constraints on Open and Flat-Lambda CDM Cosmogonies
• The Age-Redshift Relationship of Old Passive Galaxies
• Cosmological Parameter Determination from Counts of Galaxies
• Generalizing thawing dark energy models: the standard vis-à-vis model independent diagnostics
• Effect of low anisotropy on cosmological models by using supernova data
• CMB Anisotropy Constraints on Flat-Lambda and Open CDM Cosmogonies from DMR, UCSB South Pole, Python, ARGO, MAX, White Dish, OVRO, and SuZIE Data
• Tilted non-spatially-flat inflation
• OVRO CMB Anisotropy Measurement Constraints on Flat-Lambda and Open CDM Cosmogonies
• Cosmological Parameter Estimation: Method